FLYING FOR ME

2007
KN4LF DAILY LF/MF/HF
FREQUENCY RADIOWAVE PROPAGATION FORECAST ARCHIVE



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KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-013

Date Format is MM/DD/YYYY

Published Thursday 12/20/2007 At 2200 UTC Valid 12/21-27/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

POOR to FAIR.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

-Expect FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect POOR Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR to GOOD Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

-Expect POOR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR.

 High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR.   

High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR.

 Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR.

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be POOR.

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be POOR.

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be POOR.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR. 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees N/S

Mid: 25-60 degrees N/S

High: 60-90 degrees N/S

 

Low Latitude- POOR on 80-30 meters ham /90-31 meters shortwave.

Mid Latitude- FAIR on 80-30 meters ham/90-31 meters shortwave.

High Latitude- POOR on 80-30 meters ham/90-31 meters shortwave.

 

Low Latitude- FAIR on 20-17 meters ham/25-17 meters shortwave.

Mid Latitude- FAIR on 20-17 meters ham/25-17 meters shortwave.

High Latitude- FAIR to POOR 20-17 meters ham/25-17 meters shortwave.

 

Low Latitude- POOR on 15-10 meters ham/13-11 meters shortwave.

Mid Latitude- POOR on 15-10 meters ham/13-11 meters shortwave.

High Latitude- POOR on 15-10 meters ham/13-11 meters shortwave.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 50-54 MC (6 METER) PROPAGATION MODES AND STRENGTHS ARE EXPECTED-

F2- NONE

Sporadic E- FAIR

Auroral E- POOR.

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- POOR

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

None-S0

For global real time information concerning 6 meter band openings check out the VHFDX website at:

http://www.vhfdx.net/spots/map.php?Frec=MUF

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be MODERATE thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ).

Northern hemisphere mid latitude regions can expect MODERATE to HIGH thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW to MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH to MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE to LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

 END OF FORECAST

 

DISCUSSION OF PAST CONDITIONS-

For 12/14-20/2007-

Per forecast #2007-012 the period began with exceptionally quiet conditions, then degraded to active by the middle of the period onward. Overall LF, MF and HF frequency propagation conditions were fair to poor.

A recurring southern hemisphere Coronal Hole #304 (old #300) became geoeffective (Earth facing) and the high velocity solar wind stream emanating from it was strong and the impact to propagation conditions was moderate.

Globally with the daily sunspot number as high as 39 and vaguely related solar flux level as high as 92, the Maximum usable Frequency (MUF) rose high enough to give 15, 17 and 20 meters a boost in propagation conditions via the F layer.

However F layer MUFs continued to low to boost propagation conditions on 6 and 10 meters.

The following propagation modes and strengths were observed on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- FAIR

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- GOOD

There were some Sporadic E (Es) propagation openings on 6-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There was also intermittent east-west F layer propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. There was intermittent east-west F layer propagation openings on 17 meters.

There was one sunspot group visible, #10978 with a twisted beta-gamma-delta magnetic signature, which has since slipped around the western horizon of the Sun. While visible it produced 7 C class solar flares.

A brief bit of excitement occurred during the period as a Plage rotated around the eastern horizon of the Sun. It has at a mid latitude location and had a solar cycle 24 magnetic polarity. At least through today the Plage has not developed into a sunspot group. So alas we cannot yet declare that solar cycle 24 has begun.

After 18 days consecutively with visible sunspots on the Earth facing side of the Sun, yesterday the count fell to 0. Sunspots had also been visible on the far side of the Sun via the SOHO holographic image. Unfortunately all of the sunspot groups were old solar cycle 23 ones.

Trans-equatorial (TEP) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was moderate signal absorption on the MF AM broadcast band, 160 and 120 meters on high and low latitude propagation paths in the Northern Hemisphere. The moderate absorption degraded propagation conditions.

There was moderate signal absorption on the MF AM broadcast band, 160 and 120 meters on high and low latitude propagation paths in the Southern Hemisphere. The moderate absorption degraded propagation conditions.

There was moderate signal absorption on the LF band on high and low latitude paths in the Northern Hemisphere. The moderate absorption degraded propagation conditions.

There was moderate signal absorption on the LF band on high and low latitude propagation paths in the Southern Hemisphere. The moderate absorption degraded propagation conditions.

At times moderate lightning QRN hampered receive conditions on 160 and 80 meters in the Northern Hemisphere.

At times major lightning QRN hampered receive conditions on 160, 80 and 40 meters in the Southern Hemisphere.

 

DISCUSSION OF FUTURE CONDITIONS-

For 12/21-27/2007-

Recurrent southern hemisphere Coronal Hole #304 (old #300) will continue to impact propagation conditions in a moderate to minor negative manner through 12/22/2007.

Globally with the daily sunspot number and vaguely related solar flux level at low levels (<73), decreased F layer MUFs will negatively impact 15, 17 and 20 meters.

There will be a few Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: #10976 with a beta magnetic signature on 12/24/2007 and #10977 with a beta magnetic signature on 12/27/2007.

Trans-equatorial (TEP) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be moderate to minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high and low latitude propagation paths in the northern hemisphere. The moderate to minor absorption will degrade propagation conditions.

There will be moderate signal absorption on the MF AM broadcast band, 160 and 120 meters on high and low latitude propagation paths in the Southern Hemisphere. The moderate absorption will degrade propagation conditions.

There will be moderate signal absorption on the LF band on high and low latitude paths in the Northern Hemisphere. The moderate signal absorption will degrade propagation conditions.

There will be moderate signal absorption on the LF band on high and low latitude propagation paths in the Southern Hemisphere. The moderate absorption will degrade propagation conditions.

At times major to moderate lightning QRN will hamper receive conditions on 160, 80 and 40 meters in the Northern Hemisphere?

At times major lightning QRN will hamper receive conditions on 160, 80, 40 and 20 meters in the Southern Hemisphere.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

Kp 0-4, isolated 5.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions MAY OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is LOW.

Daily solar flux index levels (SFI) should range between 68-73.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW.

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be POSITIVE.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 12/14/2007 TO 2200 UTC 12/20/2007

Sunspot Groups- Sunspot group #10978 contains a twisted beta-gamma-delta magnetic signature that was capable of producing small C class and moderate size M class solar flares.

Max/Min Solar Flux Readings- 72.5 to 91.9.

Max/Min SEC Sunspot Number- 00 to 39.

Max/Min Solar Wind Speed- 344 to 770.

Max/Min Averaged Daily Background X-Ray Flux- A0.0 to B1.1.

Max/Min Dst Index- -46 to +33, via Kyoto.

Max/Min Dst Index- -45 to -6, via G3YNK.

Solar Flares- C-7 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0.

Recurring southern hemisphere Coronal Hole #304 (old #300) became geoeffective (Earth facing) and the high velocity solar wind stream emanating from it was strong and the impact to propagation conditions was moderately negative.

Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 00-32.

The Kp index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The Boulder CO mid latitude K index had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 0 to 5.

The Fredericksburg, MD mid latitude K index had been at quiet to unsettled geomagnetic levels with a range of 0 to 3.

The College, AK high latitude K index had been at quiet geomagnetic levels to strong geomagnetic storming levels, with a range of 0 to 7. 

The Troms, Norway high latitude K index had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

14. Sunspot Group-

Sunspot groups are bipolar magnetic concentration regions on the photosphere of the Sun where magnetic field strengths many thousands of times stronger than the Earth's magnetic field reside. Sunspots appear as dark spots on the surface of the Sun because temperatures in the dark centers of sunspots drop to approximately 3700 K compared to 5700 K for the surrounding photosphere. The difference in temperature makes the spots appear darker than elsewhere. Sunspots typically last for several days to several weeks. They are seen to rotate around the sun, since they are on the surface, and the sun rotates fully every 27.5 days.

Sunspots usually come in groups with two opposing sets of spots. Whether two or twenty sunspots exist in a particular group they are counted as one sunspot group and numbered, such as 10500. That number would signify sunspot group number 10500 for solar cycle 23.

One set of sunspots will have a positive or north magnetic field while the other set will have a negative or south magnetic field. The magnetic field is strongest in the darker parts of the sunspots called the umbra and weaker and more horizontal in the lighter part called the penumbra. The twisted magnetic fields associated with sunspot groups are one source of the solar flares, coronal mass ejections and geomagnetic storms that wreak havoc with the ionosphere here on Earth.

The current system of counting sun spots hails from a previous era when direct observation of sun spots was inherently inaccurate. The sunspot number is derived by counting 10 points for each sunspot group and then adding one point for each spot. So if a sunspot group contains 1 individual sunspot the official count becomes 11. 4 individual sunspots in a sunspot group equals 44 sunspots. (See definition #24. Plage).

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

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KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-012

Date Format is MM/DD/YYYY

Published Thursday 12/13/2007 At 2200 UTC Valid 12/14-20/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

GOOD to FAIR 12/14-16/2007.

FAIR to POOR 12/16-20/2007.    

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

-Expect GOOD to FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect GOOD to FAIR Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect POOR to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect FAIR to POOR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect FAIR to POOR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD to FAIR.   

High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to POOR.

 

 Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD to FAIR.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to POOR.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD to FAIR.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to POOR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD to FAIR.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be GOOD to FAIR.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be FAIR. 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees N/S

Mid: 25-60 degrees N/S

High: 60-90 degrees N/S

 

Low Latitude- GOOD 12/14-16/2007. FAIR 12/17-20/2007 on 80-30 meters ham /90-31 meters shortwave.

Mid Latitude- GOOD to FAIR 12/14-16/2007. FAIR to POOR 12/17-20/2007 on 80-30 meters ham/90-31 meters shortwave.

High Latitude- FAIR 12/14-16/2007. POOR 12/17-20/2007 on 80-30 meters ham/90-31 meters shortwave.

 

Low Latitude- GOOD to FAIR 12/14-16/2007. FAIR to POOR 12/17-20/2007 on 20-17 meters ham/25-17 meters shortwave.

Mid Latitude- GOOD to FAIR 12/14-16/2007. FAIR to POOR 12/17-20/2007 on 20-17 meters ham/25-17 meters shortwave.

High Latitude- FAIR 12/14-16/2007. POOR 12/17-20/2007 on 20-17 meters ham/25-17 meters shortwave.

 

Low Latitude- GOOD to FAIR 12/14-16/2007. FAIR to POOR 12/17-20/2007 on 15-10 meters ham/13-11 meters shortwave.

Mid Latitude- FAIR 12/14-16/2007. POOR 12/17-20/2007 on 15-10 meters ham/13-11 meters shortwave.

High Latitude- POOR on 15-10 meters ham/13-11 meters shortwave.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 50-54 MC (6 METER) PROPAGATION MODES AND STRENGTHS ARE EXPECTED-

F2- NONE

Sporadic E- FAIR

Auroral E- NONE 12/14-16-2007. FAIR 12/17-18/2007. NONE 12/18-20/2007.

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- FAIR to GOOD 12/14-15/2007. POOR to NONE 12/16-20/2007. This will be due to the Geminid meteor shower which peaks on Friday December 14, 2007.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

None-S0

For global real time information concerning 6 meter band openings check out the VHFDX website at:

http://www.vhfdx.net/spots/map.php?Frec=MUF

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

 

During the outlook period there will be MODERATE thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ).

Northern hemisphere mid latitude regions can expect MODERATE to HIGH thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW to MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH to MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE to LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF FORECAST

 

DISCUSSION OF PAST CONDITIONS-

For 12/07-13/2007-

Per forecast #2007-011 the period saw exceptionally quiet conditions. Towards the end of the period unsettled to active conditions occurred. Overall LF, MF and HF frequency propagation conditions were good.

A recurring transequatorial Coronal Hole #303 (old #298) became geoeffective (Earth facing) but the solar wind stream emanating from it was weak and the impact to propagation conditions was minimal.

Globally with the daily sunspot number as high as 44 and vaguely related solar flux level as high as 94, the Maximum usable Frequency (MUF) rose high enough to give 15, 17 and 20 meters a boost in propagation conditions via the F layer.

However F layer MUFs continued to low to boost propagation conditions on 6 and 10 meters.

The following propagation modes and strengths were observed on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor- NONE

There were some Sporadic E (Es) propagation openings on 6-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There was also intermittent east-west F layer propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. There was intermittent east-west F layer propagation openings on 17 meters.

There were two new sunspot groups visible, #10977 with a simple beta magnetic signature, which has since slipped around the western horizon of the Sun. Also significant sunspot group #10978 with a twisted beta-gamma-delta magnetic signature that so far has produced two small C class solar flares.

We have now reached 12 days consecutively with visible sunspot groups on the Earth facing side of the Sun. Sunspot groups had also been visible on the far side of the Sun via the SOHO holographic image. Unfortunately all of the sunspot groups were old solar cycle 23 ones.

Trans-equatorial (TEP) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was nil signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The nil absorption allowed for some of the best propagation conditions in a good while.

There was minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The minor absorption allowed for improved propagation conditions.

There was nil signal absorption on the LF band on high latitude paths in the Northern Hemisphere. The nil absorption allowed for some of the best propagation conditions in a good while.

There was minor signal absorption on the LF band on high latitude propagation paths in the Southern Hemisphere. The minor absorption allowed for improved propagation conditions.

At times moderate lightning QRN hampered receive conditions on 160 and 80 meters in the Northern Hemisphere.

At times major lightning QRN hampered receive conditions on 160, 80 and 40 meters in the Southern Hemisphere.

 

DISCUSSION OF FUTURE CONDITIONS-

For 12/14-20/2007-

Recurrent southern hemisphere Coronal Hole #304 (old #300) will rotate into geoeffective (Earth facing) position beginning on 12/14/2007. It will impact propagation conditions in a moderate negative manner beginning on 12/16-17/2007.

Globally with the daily sunspot number and vaguely related solar flux level at a continued moderate levels, increased F layer MUFs will positively impact 15, 17 and 20 meters.

There will be a few Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: #10975 on 12/14/2007.

Current sunspot group #10978 with a twisted beta-gamma-delta magnetic signature has the potential to produce moderate sized M class solar flares.

Trans-equatorial (TEP) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be moderate signal absorption beginning on 12/17/2007 on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. The moderate absorption will degrade propagation conditions.

There will be moderate signal absorption beginning on 12/17/2007 on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate absorption will degrade propagation conditions.

There will be moderate signal absorption beginning on 12/17/2007 on the LF band on high latitude paths in the Northern Hemisphere. The moderate absorption will degrade propagation conditions.

There will be moderate signal absorption beginning on 12/17/2007 on the LF band on high latitude propagation paths in the Southern Hemisphere. The moderate absorption will degrade propagation conditions.

At times major lightning QRN will hamper receive conditions on 160, 80 and 40 meters in the Northern Hemisphere.

At times major lightning QRN will hamper receive conditions on 160, 80, 40 and 20 meters in the Southern Hemisphere.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

Kp 0-5, isolated 6.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions MAY OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW to MODERATE.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW to MODERATE.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW to MODERATE.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, southern hemisphere CH #304 (old #300) beginning on 12/14/2007.

Daily solar flux index levels (SFI) should range between 90-96.

The probability of a small C class solar flare is MODERATE.

The probability of a large M class solar flare is LOW to MODERATE.

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE between 12/14-18/2007 and POSITIVE between 12/18-20/2007.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 12/07/2007 TO 2200 UTC 12/13/2007

Sunspot Groups- Sunspot group #10978 contains a twisted beta-gamma-delta magnetic signature that was capable of producing small C class and moderate size M class solar flares.

Max/Min Solar Flux Readings- 80.8 to 94.4. This is the highest daily solar flux level since November 2006.

Max/Min SEC Sunspot Number- 22 to 44

Max/Min Solar Wind Speed- 270 to 684

Max/Min Averaged Daily Background X-Ray Flux- A1.7 to C4.5

Max/Min Dst Index- -36 to +20, via Kyoto

Max/Min Dst Index- -30 to -6, via G3YNK

Solar Flares- C-3 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0

A recurring transequatorial Coronal Hole #303 (old #298) became geoeffective (Earth facing) but the solar wind stream emanating from it was weak and the impact to propagation conditions was minimal.

Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to active geomagnetic levels, with a range of 00-22.

The Kp index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The Boulder CO mid latitude K index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The high latitude K index (via Troms, Norway) had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

13.) Polar Cap Absorption (PCA)-

An anomalous condition of the polar Ionosphere whereby medium frequency (300-3000 kc) radio waves are absorbed, and LF and VLF (3-300 kHz) radio waves are wave guided at lower altitudes than normal. In practice, the absorption is inferred from the proton flux at energies greater than 10 MeV (10+0), so that PCA's, Polar Radio Blackouts and Proton Events are interrelated and often simultaneous.

((((NOTE!!! high latitude radio propagation paths may still be disturbed for days, up to weeks, following the end of an official proton event.)))) This fact is still stubbornly opposed by some otherwise very knowledgeable space weather physicists, hung up on threshold Riometer readings.

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

Back To The Top 

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-011

Date Format is MM/DD/YYYY

Published Thursday 12/06/2007 At 2200 UTC Valid 12/07-13/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

FAIR to GOOD.    

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

If the background solar flux level rises into the B range from the current A 5.0 level, MF propagations will not be quite as good as I currently have forecasted.

-Expect GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR to GOOD Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR to POOR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.   

High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR.

 

 Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be GOOD.


Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be FAIR. 

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees N/S

Mid: 25-60 degrees N/S

High: 60-90 degrees N/S

 

Low Latitude- FAIR to GOOD on 80-30 meters ham /90-31 meters shortwave.

Mid Latitude- GOOD on 80-30 meters ham/90-31 meters shortwave.

High Latitude- GOOD to FAIR on 80-30 meters ham/90-31 meters shortwave.

 

Low Latitude- FAIR on 20-17 meters ham/25-17 meters shortwave.

Mid Latitude- FAIR to GOOD on 20-17 meters ham/25-17 meters shortwave.

High Latitude- FAIR to GOOD on 20-17 meters ham/25-17 meters shortwave.

 

Low Latitude- POOR on 15-10 meters ham/13-11 meters shortwave.

Mid Latitude- POOR to FAIR on 15-10 meters ham/13-11 meters shortwave.

High Latitude- POOR to FAIR on 15-10 meters ham/13-11 meters shortwave.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 50-54 MC (6 METER) PROPAGATION MODES AND STRENGTHS ARE EXPECTED-

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- POOR

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

None-S0

For global real time information concerning 6 meter band openings check out the VHFDX website at:

http://www.vhfdx.net/spots/map.php?Frec=MUF

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

 

During the outlook period there will be MODERATE thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ).

Northern hemisphere mid latitude regions can expect LOW to MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW to NIL thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH to MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE to LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

For 11/30-12/06/2007-

Per forecast #2007-010 the period saw quiet conditions. Actually at times conditions were exceptionally quiet!

A new southern hemisphere small Coronal Hole #302 formed but the solar wind stream emanating from it was too weak to impact propagation conditions in a negative manner.

Globally with the daily sunspot number and vaguely related solar flux level low, reduced F layer MUFs negatively impacted 6, 10, 12, 15 and 17 meters.

The following propagation modes and strengths were observed on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor- NONE

There were some Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There was also intermittent east-west F layer propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. There was intermittent east-west F layer propagation openings on 17 meters.

There were three new sunspot groups visible, #10976 with a beta magnetic signature, #10977 with a beta magnetic signature and a recurrent but newly numbered sunspot group #10978 (old 10974) with a beta-gamma magnetic signature, that has just risen above the eastern horizon of the Sun.

However the solar flux index did not exceed 77 and the sunspot number was no higher than 26, so there was no HF propagation boost on 10-17 meters during the period but a bit did occur on 20 meters.

We have now reached 6 days consecutively with visible sunspot groups on the Earth facing side of the Sun. Sunspot groups had also been visible on the far side of the Sun via the SOHO holographic image. Unfortunately all of the sunspot groups were old solar cycle 23 ones.

Trans-equatorial (TEP) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was nil signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The nil absorption allowed for some of the best propagation conditions in a good while.

There was minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The minor absorption allowed for improved propagation conditions.

There was nil signal absorption on the LF band on high latitude paths in the Northern Hemisphere. The nil absorption allowed for some of the best propagation conditions in a good while.

There was minor signal absorption on the LF band on high latitude propagation paths in the Southern Hemisphere. The minor absorption allowed for improved propagation conditions.

At times moderate lightning QRN hampered receive conditions on 160 and 80 meters in the Northern Hemisphere.

At times major lightning QRN hampered receive conditions on 160, 80 and 40 meters in the Southern Hemisphere.

 

DISCUSSION OF FUTURE CONDITIONS-

For 12/07-13/2007-

Recurrent transequatorial Coronal Hole #303 (old #298) will rotate into geoeffective (Earth facing) position beginning on 12/08/2007. It could impact propagation conditions in a very minor negative manner beginning on 12/11/2007.

Globally with the daily sunspot number and vaguely related solar flux level low, reduced F layer MUFs will negatively impact 6, 10, 12, 15 and 17 meters. However 20 meter propagation could see a bit of a boost.

The following propagation modes and strengths will occur on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- NONE

There will be a few Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit:

Recurrent but newly renumbered sunspot group #10978 (old 10974) with a beta-gamma magnetic signature, that has just risen above the eastern horizon of the Sun. It has the potential to produce C class solar flares and wreck the second half of my forecast.

Trans-equatorial (TEP) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

I expect nil signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. The nil absorption will allow for some of the best propagation conditions in a good while.

There will be minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The minor absorption will allow for improved propagation conditions.

There will be nil signal absorption on the LF band on high latitude paths in the Northern Hemisphere. The nil absorption will allow for some of the best propagation conditions in a good while.

There will be minor signal absorption on the LF band on high latitude propagation paths in the Southern Hemisphere. The minor absorption will allow for improved propagation conditions.

At times moderate lightning QRN will hamper receive conditions on 160 and 80 meters in the Northern Hemisphere.

At times major lightning QRN will hamper receive conditions on 160, 80 and 40 meters in the Southern Hemisphere.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

Kp 0-3, isolated Kp-4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions MAY OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW but will become MODERATE.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW but will become MODERATE.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW but will become MODERATE.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, transequatorial CH #303 (old #298), between 12/08-11/2007.

Daily solar flux index levels (SFI) should range between 77-85.

The probability of a small C class solar flare is LOW but will become MODERATE.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 11/30/2007 TO 2200 UTC 12/06/2007

Sunspot Groups- No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 71.4 to 77.4

Max/Min SEC Sunspot Number- 00 to 26

Max/Min Solar Wind Speed- 272 to 371

Max/Min Averaged Daily Background X-Ray Flux- A0.0 to A5.0

Max/Min Dst Index- -13 to +16, via Kyoto

Max/Min Dst Index- -17 to -8, via G3YNK

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

A new southern hemisphere small Coronal Hole #302 formed but the solar wind stream emanating from it was too weak to impact propagation conditions in a negative manner.

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet geomagnetic levels, with a range of 00-06.

The Kp index had been at quiet geomagnetic levels, with a range of 0 to 2.

The Boulder CO mid latitude K index had been at quiet geomagnetic levels, with a range of 0 to 2.

The high latitude K index (via Troms, Norway) had been at quiet to active geomagnetic levels, with a range of 0 to 4. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

 

12.) Geological/Meteorological Effects On Medium Frequency Propagation-

Geological effects such as earthquakes and volcanic eruptions, as well as
meteorological effects such as Troposphere originating Internal Buoyancy/Gravity Waves (IBGW's), Stratosphere level Quasi Biennial Oscillations (QBO) and warming (STRATWARM) have a negative effect on medium frequency RF signals in the form of small to medium increased absorption variations of medium frequency RF signals via the D layer, due to traveling ionospheric disturbances (TID's).

Also temperature and moisture discontinuities involved with cold frontal inversions and air mass triple points involved with extra-tropical low pressure systems can refract, diffract or scatter medium frequency radio signals in unpredictable ways, most notably on high transmitted RF power levels. This is another concept that a fellow Physicist and expert in optics took me to task over.

As far as medium frequency refraction it's more significant at say 3000 kc, then 1850 kc or 1500 kc. But it's also more noticeable with higher transmitted RF powers, i.e. WSAI 1530 50 KW and even more so with BSKA 1521 KC 1000 KW and now defunct 2000 kc region 100 KW marine stations.

We know that the medium frequency spectrum is defined as 300-3000 kc but the differences in refractive properties between 300 and 3000 is very significant At 3000 kc refraction is a good description, on 160 scattering, at 300 kc diffraction.

Using the strictest definition of RF refraction, its effect on 160 meters is small but it has been measured by government researchers as significant enough to impact 160 but near the air mass triple point. In my opinion scattering is actually the more consistent propagation medium for 160 meters along a cold front, away from the extra-tropical cyclone center.

However the temperature and moisture discontinuities in the vicinity of a triple point air mass structure such as seen with a mature extra-tropical cyclone is very complex and fluid. The NW quadrant of the extra-tropical cyclone is the location that the original government researchers identified as the region of existence for the complex temperature/moisture discontinuity structure that allows for refraction of RF signals as low as 1500 kc. I have not been successful at garnering data from the federal government that can be released to the general public. NOAA has been similarly stymied and therefore is now conducting similar research.

The QBO is a wind shift in the equatorial stratosphere, an oscillation from easterly to westerly and back on the time scale of approximately two years (26 months) and is a source of Internal Buoyancy/Gravity Waves (IBGW) which create absorptive perturbations in the D and E layers and even possibly the F 1/2 layer. A note, the E-valley/Flayer ducting propagation mechanism does not exist only during greyline periods. Internal Buoyancy/Gravity Waves (IBGW's) are a source of the ducting mechanism and allow for occurrences of ducting along any propagation path in total darkness. Measurement of the timing of arrival of propagated medium frequency RF signals demonstrates the existence of the ducting mechanism, versus conventional numerous E layer land/ocean surface hops.

The HAARP ionospheric program, earthquakes, volcanic eruptions, thunderstorms, lightning (especially positive cloud to ground strokes), elves, tornadoes and hurricanes and even man made activities such as rocket launches including the space shuttle, are all sources of (IBGW's).

Many times I've heard ham's lament that propagation was going to go to crap due to another NASA Space Shuttle launch, in a sense they are correct.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

Back To The Top

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-010

Date Format is MM/DD/YYYY

Published Thursday 11/29/2007 At 2200 UTC Valid 11/30-12/06/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

POOR to FAIR between 11/30-12/01/2007.

FAIR to GOOD between 12/02-06/2007.    

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR to GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR to GOOD Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect GOOD to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect POOR to FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR to FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be POOR to FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007.   

High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 11/30-12/01/2007, then becoming FAIR between 12/02-06/2007.   

 

 Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007.   

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 11/30-12/01/2007, then becoming FAIR between 12/02-06/2007.    

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007.   


Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR between 11/30-12/01/2007, then becoming FAIR between 12/02-06/2007.   

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

 

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees N/S

Mid: 25-60 degrees N/S

High: 60-90 degrees N/S

 

Low Latitude- FAIR between 11/30-12/01/2007, then becoming GOOD between 12/02-06/2007on 80-30 meters.

Mid Latitude- FAIR between 11/30-12/01/2007, then becoming GOOD between 12/02-06/2007on 80-30 meters.

High Latitude- POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007on 80-30 meters.

 

Low Latitude- POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007 on 20-17 meters.

Mid Latitude- POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007 on 20-17 meters.

High Latitude- POOR to FAIR between 11/30-12/01/2007, then becoming FAIR to GOOD between 12/02-06/2007 on 20-17.

 

Low Latitude- FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 50-54 MC (6 METER) PROPAGATION MODES AND STRENGTHS EXPECTED-

F2-NONE

Sporadic E- POOR

Auroral E-NONE

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- NONE

 

For global real time information concerning 6 meter band openings check out the VHFDX website at: http://www.vhfdx.net/spots/map.php?Frec=MUF

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

None-S0

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 11/23-29/2007-

Per forecast #2007-009 the period saw quiet to occasionally active conditions. The source for the active conditions was a high velocity solar wind stream emanating from geoeffective (Earth facing) southern Coronal Hole #300 (#296).

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters.

The following propagation modes and strengths were observed on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- NONE

There were very few Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There was one brief sunspot group visible, #10975  with a beta magnetic signature but the solar flux index did not exceed 71 and the sunspot number was no higher than 15, so there was no HF propagation boost on 10-20 meters during the period. We have now reached 3 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. No sunspot groups had been visible on the far side of the Sun either via the SOHO holographic image.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The minor absorption allowed for improved propagation conditions.

There was minor to moderate signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate absorption produced continued poor propagation conditions.

There was moderate to major signal absorption on the LF band on high and mid latitude paths.  The major absorption produced continued poor propagation conditions.

At times intense lightning QRN hampered receive conditions on 160, 80 and 40 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 11/30-12/06/2007-

No recurrent significant Coronal Holes will rotate into geoeffective (Earth facing) position. However a couple of new but insignificant in size transequatorial Coronal Holes (#301 & #302) will rotate into geoeffective (Earth facing) position be by 11/30/2007 but should not impact propagation conditions in a negative manner.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 6, 10, 12, 15, 17 and 20 meters.

The following propagation modes and strengths will occur on 6 meters.

F2- NONE

Sporadic E- FAIR

Auroral E- NONE

Tropospheric Ducting- FAIR to GOOD

Meteor Scatter- NONE

There will be very few Sporadic E (Es) propagation openings on 10-160 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: None.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

I expect minor to nil signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. This should lead to continued improvement in propagation conditions, especially in comparison to last week.

I expect moderate to minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the southern hemisphere. The moderate absorption will produce continued poor propagation conditions.

I expect minor to nil signal absorption on the LF band on high latitude paths in the northern hemisphere. This should lead to continued improvement in propagation conditions, especially in comparison to last week.

I expect minor to nil signal absorption on the LF band on high latitude paths in the northern hemisphere. This should lead to improvement in propagation conditions.

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80, 60 and 40 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60 and 49 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

Kp 0-3, isolated Kp-4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions MAY OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, southern hemisphere CH #303 (old #297), through 11/30/2007.

Daily solar flux index levels (SFI) should range between 68-71.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be POSITIVE.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 11/23/2007 TO 2200 UTC 11/29/2007

 

Sunspot Groups- No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 69.9 to 71.5

Max/Min SEC Sunspot Number- 00 to 15

Max/Min Solar Wind Speed- 381 to 751

Max/Min Averaged Daily Background X-Ray Flux- A0.0 to A0.0

Max/Min Dst Index- -39 to -7, via Kyoto

Max/Min Dst Index- -35 to -19, via G3YNK

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- A southern hemisphere high velocity solar wind stream emanating from geoeffective (Earth facing) Coronal Hole #300 (old #296) did create a minor negative impact on propagation conditions.

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to active geomagnetic levels, with a range of 00-22.

The Kp index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The Boulder mid latitude K index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The high latitude K index (via Troms, Norway) had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

11.) Geomagnetic/Ionospheric Storm-

A worldwide disturbance of the Earth's magnetosphere and or ionosphere, induced by direct connection to the Sun's Interplanetary Magnetic Field (IMF), distinct from regular diurnal variations. Basically it's a precipitation of electrons trapped within our magnetosphere, as the electrons collide. The end result is a reduction of the MUF of the F2 layer. (See definition #3. Equatorial Ring Current). (See definition #4. Coronal Mass Ejection). (See definition #5. Coronal Hole). (See definition #6. Solar Filament).

((((Note! Unfortunately elevated Kp indices of as little as a 3 will create absorptive conditions for medium frequency signal propagation on higher propagation paths)))).

Initial phase of a geomagnetic storm is that period when there may be an increase of the middle latitude horizontal intensity.

Main phase of a geomagnetic storm is that period when the horizontal magnetic field at middle latitudes is generally decreasing.

Recovery phase of a geomagnetic storm is that period when the depressed northward field component returns to normal levels.

By the way effects of the solar wind on the magnetosphere decreases as we approach the Summer/Winter solstice and increase at the Fall/Spring Equinox. Why? Basically it's the orientation of Earth's magnetic field with respect to the Interplanetary Magnetic Field within the Solar Wind. When solar material and shock waves reach Earth their effects may be enhanced or dampened depending on the angle at which they arrive. http://science.nasa.gov/headlines/y2001/ast26oct_1.htm?list101234 .

The Wang-Sheeley Interplanetary Magnetic Field (IMF) Model is used to predict Sun's IMF polarity. When the polarity of the IMF is negative a visible mid latitude Aurora display is likely as a Coronal Mass Ejection (CME) strikes the Earth's magnetic field.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

Back To The Top

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-009

Date Format is MM/DD/YYYY

Published Thursday 11/22/2007 At 2200 UTC Valid 11/23-29/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

POOR for ham signals and POOR to FAIR for broadcast signals through 11/27/2007. Then becoming FAIR for ham signals and FAIR to GOOD for broadcast signals between 11/28/2007-11/29/2007.    

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect POOR to FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect POOR to FAIR Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR to GOOD Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect POOR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be POOR to FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR through 11/27/2007. Then becoming FAIR broadcast signals between 11/28/2007-11/29/2007.    


High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR through 11/27/2007. Then becoming FAIR broadcast signals between 11/28/2007-11/29/2007.    

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR through 11/27/2007. Then becoming FAIR to GOOD for broadcast signals between 11/28/2007-11/29/2007.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR through 11/27/2007. Then becoming FAIR broadcast signals between 11/28/2007-11/29/2007.    


Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be POOR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be POOR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR through 11/27/2007. Then becoming FAIR broadcast signals between 11/28/2007-11/29/2007.    


Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR to FAIR through 11/27/2007. Then becoming FAIR broadcast signals between 11/28/2007-11/29/2007.    

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

 

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees N/S

Mid: 25-60 degrees N/S

High: 60-90 degrees N/S

 

Low Latitude- POOR to FAIR through 11/27/2007. Then becoming FAIR to GOOD between 11/28/2007-11/29/2007on 80-30 meters.

Mid Latitude- POOR to FAIR through 11/27/2007. Then becoming FAIR to GOOD between 11/28/2007-11/29/2007on 80-30 meters.

High Latitude- POOR through 11/27/2007. Then becoming FAIR between 11/28/2007-11/29/2007on 80-30 meters.

 

Low Latitude- POOR to FAIR through 11/27/2007. Then becoming FAIR to GOOD between 11/28/2007-11/29/2007on 20-17 meters.

Mid Latitude- POOR to FAIR through 11/27/2007. Then becoming FAIR to GOOD between 11/28/2007-11/29/2007on 20-17 meters.

High Latitude- POOR through 11/27/2007. Then becoming FAIR between 11/28/2007-11/29/2007on 20-17.

 

Low Latitude- FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 50-54 MC (6 METER) PROPAGATION CONDITIONS EXPECTED-

F2- Poor

Sporadic E- POOR

Auroral E- POOR

Tropospheric Ducting- FAIR to GOOD

Meteor- POOR

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 11/16-22/2007-

Per propagation forecast #2007-008 the period saw quiet geomagnetic conditions to moderate geomagnetic storming conditions. A high velocity solar wind stream emanating from geoeffective (Earth facing) southern Coronal Hole #300 (298) was the culprit for the conditions.

During the period the Kp index reached a 6 for three hours (moderate geomagnetic storming), a 5 for three hours (minor geomagnetic storming) and a 4 for 21 hours (active geomagnetic conditions).

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters.

 

The following propagation conditions were observed on 6 meters.

F2- No

Sporadic E-Yes

Auroral E- No

Tropospheric Ducting- Yes

Meteor- No

There were very few Sporadic E (Es) propagation openings on 10-160 meters.

 

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There were two brief sunspot groups visible, #10973 and #10974 but the solar flux index did not exceed 71 and the sunspot number was no higher than 13, so there was no HF propagation boost on 10-20 meters during the period. We have now reached 5 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. Also a couple of sunspot groups had been visible on the far side of the Sun via the SOHO holographic image.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor to major signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The major absorption produced poor propagation conditions.

There was moderate to major signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The major absorption produced continued poor propagation conditions.

There was moderate to major signal absorption on the LF band on high and mid latitude paths.  The major absorption produced continued poor propagation conditions.

At times intense lightning QRN hampered receive conditions on 160, 80 and 40 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 11/23-29/2007-

Recurrent southern hemisphere Coronal Hole #301 (297) may rotate into geoeffective (Earth facing) position if it survived back side transit. It could begin impacting propagation conditions in some negative manner between 11/27-28/2007. As old #297 it created a maximum Kp of 5 (minor geomagnetic storming) and an Ap of 48 (minor geomagnetic storming) and a repeat is possible.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters.

 

The following propagation conditions will occur on 6 meters.

F2- No

Sporadic E- Yes

Auroral E- No

Tropospheric Ducting- Yes

Meteor- No

There will be very few Sporadic E (Es) propagation openings on 10-160 meters.

 

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: #1097? by 11/25/2007.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

I expect minor to nil signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. This should lead to improvement in propagation conditions especially in comparison to last week.

I expect moderate to minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the southern hemisphere. The moderate to minor absorption will produce continued poor propagation conditions.

I expect minor to nil signal absorption on the LF band on high latitude paths in the northern hemisphere. This should lead to continued improvement in propagation conditions especially in comparison to last week.

I expect moderate to minor signal absorption on the LF band on high latitude paths in the northern hemisphere. This should lead to continued poor propagation conditions.

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80, 60 and 40 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60 and 49 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

Kp 0-3, isolated Kp-4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, southern hemisphere CH #301 (old #297) beginning on 11/27/2007. That is if it survived back side transit.

Daily solar flux index levels (SFI) should range between 68-70.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be POSITIVE.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 11/16/2007 TO 2200 UTC 11/22/2007

 

Sunspot Groups- No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 68.2-71.0

Max/Min SEC Sunspot Number- 00 to 13

Max/Min Solar Wind Speed- 333-719

Max/Min Averaged Daily Background X-Ray Flux- A0.0-A0.0

Max/Min Dst Index- -63 to +37, via Kyoto

Max/Min Dst Index- -50 to -12, via G3YNK

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- A southern hemisphere high velocity solar wind stream emanating from geoeffective (Earth facing) Coronal Hole #300 (old #296) did create a negative impact on propagation conditions.

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to geomagnetic levels to major geomagnetic storming levels, with a range of 00-80.

The Kp index had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6.

The Boulder mid latitude K index had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6.

The high latitude K index (via Troms, Norway) had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

 

10.) Medium Frequency Radio Signal Propagation Path Skewing-

Medium frequency radio signal propagation path skewing occurs due to changes in the "horizontal" electron gradient. Put in simple layman's terms the transmitted RF signal will "always" seek to propagate along the path with least absorption, which almost always means via a darkness path.

As an example a signal transmitted from Norway to New England, which is via a polar great circle path, will be directly absorbed most of the time by the Aurora Oval, with the remaining medium frequency signal skirting south and then west on the darkness path, arriving in New England from say the SE rather then the expected NE path. Also medium frequency skewed propagation paths are the norm rather then the exception, especially past approximately 3200 miles.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

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KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-008A

Date Format is MM/DD/YYYY

Published Wednesday 11/21/2007 At 1500 UTC

Per propagation forecast #2007-008, a high velocity solar wind stream emanating from geoeffective (Earth facing) southern hemisphere Coronal Hole #300 (old #296), triggered a moderate geomagnetic storm on 11/20/2007. The Kp index reached a 6 for three hours (moderate geomagnetic storming) and a 5 for three hours (minor geomagnetic storming).

This lowered maximum usable frequencies (MUFs), degrading propagation conditions on 17 and 20 meters and increased E layer absorption, degrading signals on 17, 20, 30, 40, 80 and 160 meters.

Yesterday evening through early this morning UTC I was working DX on phone and PSK31 on 80 meters and signal levels were much weaker compared to 11/19/2007.

Propagation conditions will slowly recover during the next 48 hours.

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KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-008

Date Format is MM/DD/YYYY

Published Thursday 11/15/2007 At 2200 UTC Valid 11/16-22/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- POOR for ham signals and POOR to FAIR for broadcast signals.

Nighttime- FAIR for ham signals and FAIR to GOOD for broadcast signals through 11/20/2007, then POOR to FAIR between 11/21-22/2007.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR to GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR to GOOD Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect GOOD to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect POOR to FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR to FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR to GOOD.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD through 11/20/2007, then POOR to FAIR between 11/21-22/2007.

 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR through 11/20/2007, then POOR between 11/21-22/2007.

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.
 

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD through 11/20/2007, then POOR to FAIR between 11/21-22/2007.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR to FAIR, through 11/20/2007, then POOR between 11/21-22/2007.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- FAIR to GOOD on 80-30 meters.

Mid Latitude- FAIR to GOOD on 80-30 meters through 11/20/2007, then POOR to FAIR between 11/21-22/2007.

High Latitude- FAIR to GOOD on 80-30 meters through 11/20/2007, then POOR between 11/21-22/2007.

 
Low Latitude- FAIR to GOOD on 20-17 meters.

Mid Latitude- FAIR to GOOD on 20-17 meters through 11/20/2007, then POOR to FAIR between 11/21-22/2007.

High Latitude- FAIR on 20-17 meters through 11/20/2007, then POOR between 11/21-22/2007.

 

Low Latitude- POOR to FAIR on 15-10 meters.

Mid Latitude- POOR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 11/09-15/2007-

The period saw quiet to unsettled conditions. A high velocity solar wind stream emanating from geoeffective (Earth facing) southern Coronal Hole #298 was the culprit for the unsettled conditions.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters. There were few Sporadic E (Es) openings on 6 through 20 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There were no sunspot groups visible and the solar flux index stayed near 70, so there was no HF propagation boost on 10-20 meters during the period. We reach 7 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. Also no sunspot groups had been visible on the far side of the Sun via the SOHO holographic image, so we can say that the Sun was totally spotless during the period.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor to nil night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The minor to nil absorption allowed for improved propagation conditions, especially in comparison to the previous week. There were several nights where the 160 meter band was wide open between the U.S. and the rest of the globe in the northern hemisphere.

There was moderate to minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate to minor absorption produced continued poor propagation conditions.

There was normal daytime signal absorption and minor to nil signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

At times intense lightning QRN hampered receive conditions on 160 and 80 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 11/16-22/2007-

Newly formed northern hemisphere Coronal Hole #299 rotated into geoeffective (Earth facing) position on 11/14/2007 and will begin impacting propagation conditions in some manner beginning on 11/18/2007. As it’s new it will be difficult to predict its impact and it could ruin my propagation forecast during the early part of the forecast period.

Also the fact that a brand new coronal hole has formed put’s in doubt the anecdotal evidence that solar cycle #23 bottomed out in 09/2007. The same goes for the brief spike in the sunspot number to 11 on 11/06/2007.

Southern hemisphere Coronal Hole #300 (old #296) will rotate into geoeffective (Earth facing) position by 11/17/2007 and will begin impacting propagation conditions in some negative manner beginning on 11/21/2007. As old #296 and #292 it created a maximum Kp of 6 (moderate geomagnetic storming) and an Ap of 67 (major geomagnetic storming) and a repeat is possible.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters.

There will be no F layer and little in the way of Sporadic E (Es) propagation openings on 6. There will be little in the way of Sporadic E (Es) propagation openings on 20-10 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: None.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

I expect minor to nil night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. This should lead to continued improvement in propagation conditions especially in comparison to last week. However by 11/21/2007 I expect minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the northern hemisphere. This will lead to degraded propagation conditions through at least 11/22/2007.

I expect moderate to minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the southern hemisphere. The minor to moderate absorption will produce continued poor propagation conditions.

I expect normal daytime signal absorption and minor to nil night time signal absorption on the LF band on high and mid latitude paths in the northern hemisphere.  This should lead to continued improvement in propagation conditions especially in comparison to last week. However by 11/21/2007 I expect minor to moderate night time signal absorption on the LF band on high latitude propagation paths in the northern hemisphere. This will lead to poor propagation conditions through at least 11/22/2007.

I expect normal daytime signal absorption and minor night time signal absorption on the LF band on high and mid latitude paths in the southern hemisphere.  The minor absorption will produce continued fair to poor propagation conditions. However by 11/21/2007 I expect moderate night time signal absorption on the LF band on high latitude propagation paths in the southern hemisphere. This will lead to poor propagation conditions through at least 11/22/2007.

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160 and 80 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120 and 90 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

Kp 0-5, isolated Kp-6.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions MAY OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, southern hemisphere CH #300 (old #296) beginning on 11/17/2007.

Daily solar flux index levels (SFI) should range between 69-71.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE.

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 11/09/2007 TO 2200 UTC 11/15/2007

 

Sunspot Groups-

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 68.7-70.5

Max/Min SEC Sunspot Number- 00 to 00

Max/Min Solar Wind Speed- 283-692

Max/Min Averaged Daily Background X-Ray Flux- A0.0-A0.0

Max/Min Dst Index- -11 to +20, via Kyoto

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- A southern hemisphere high velocity solar wind stream emanating from geoeffective (Earth facing) Coronal Hole #298 (old #295) did create a negative impact on propagation conditions.

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to unsettled geomagnetic levels, with a range of 00-15.

The Kp index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3.

The Boulder mid latitude K index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3.

The high latitude K index (via Troms, Norway) had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 0 to 5. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

9.) Electron Gyro Frequency Absorption-

Unfortunately medium frequencies fall within or very near the electron gyro-frequency which is in the approximate range of 630 to 1630 kHz and of course the AM broadcast band and 160 meter band is very close to these electron gyro frequencies. There is a direct correlation between the strength of Earth's magnetic field lines and electron gyro frequencies.

Basically, the electron gyro frequency is a measure of the interaction between an electron in the Earth's atmosphere and the Earth's magnetic field. The closer a transmitted medium frequency carrier or sideband wave frequency is to the electron gyro frequency, the more energy that is absorbed by the gyro (spinning) electrons from that carrier wave frequency. This is especially true for medium frequency signals traveling perpendicular to the Earth's magnetic field, meaning high latitude NW and NE propagation paths. Unfortunately this form of medium frequency signal absorption is ALWAYS present.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

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KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-007

Date Format is MM/DD/YYYY

Published Thursday 11/08/2007 At 2200 UTC Valid 11/09-11/15/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- POOR for ham signals and POOR to FAIR for broadcast signals.

Nighttime- FAIR for ham signals and FAIR to GOOD for broadcast signals.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR to GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR to GOOD Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect GOOD to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect POOR to FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR to FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR to GOOD.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.
 

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR to FAIR.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- FAIR to GOOD on 80-30 meters.

Mid Latitude- FAIR to GOOD on 80-30 meters.

High Latitude- FAIR to GOOD on 80-30 meters.
 

Low Latitude- FAIR on 20-17 meters.

Mid Latitude- FAIR on 20-17 meters.

High Latitude- FAIR on 20-17 meters.

 

Low Latitude- POOR to FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR to FAIR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

http://thunderstorm.vaisala.com/explorer.html

http://www.uspln.com/images/uspln.jpg  

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts, associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.
 
Northern hemisphere high latitude regions can expect LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 11/02-08/2007-

The period saw quiet conditions. A weak high velocity solar wind stream emanating from a newly formed un-numbered geoeffective (Earth facing) southern Coronal Hole did not create a negative impact.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters. There were few Sporadic E (Es) openings on 6 through 20 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There was one sunspot group visible, #10973 but the solar flux index stayed below 70, so there was no HF propagation boost on 10-20 meters during the period. We reach 30 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. However that streak came to an end on 11/06/2007 when sunspot group #10973 formed. Ironically the sunspot group lasted less than 24 hours before dissipating. One sunspot group or two had been visible on the far side of the Sun via the SOHO holographic image.

By the way anecdotal evidence points to solar cycle 23 minimum in September 2007 with a monthly international sunspot number of 2.4. The lowest daily solar flux reading since July 1996 of 64.4 occurred on September 28, 2007. The lowest maximum daily solar flux reading since October 1996 of 71 occurred on September 01, 2007.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor to nil night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The minor to nil absorption allowed for improved propagation conditions, especially in comparison to the previous weeks.

There was moderate to minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate to minor absorption produced continued poor propagation conditions.

There was normal daytime signal absorption and minor to nil signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

At times intense lightning QRN hampered receive conditions on 160 and 80 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 11/09-15/2007-

Southern hemisphere Coronal Hole #298 (old #295) will be in geoeffective (Earth facing) position by 11/10/2007. However the associated high velocity solar wind stream should not create a significant negative impact on propagation conditions between 11/13-15/2007.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters.

There will be no F layer and little in the way of Sporadic E (Es) propagation openings on 6. There will be little in the way of Sporadic E (Es) propagation openings on 20-10 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit:

None.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

I expect minor to nil night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. This should lead to continued improvement in propagation conditions especially in comparison to last week.

I expect moderate to minor signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate to minor absorption will produce continued poor propagation conditions.

I expect normal daytime signal absorption and minor to nil night time signal absorption on the LF band on high and mid latitude paths. 

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160 and 80 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120 and 90 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

Kp 0-3, isolated Kp- 4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions MAY OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, southern hemisphere CH #298 (old #295).

Daily solar flux index levels (SFI) should range between 67-69.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 11/02/2007 TO 2200 UTC 11/08/2007

 

Sunspot Groups-

Sunspot group #10973 formed on 11/06/2007. Ironically the sunspot group lasted less than 24 hours before dissipating.

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 66.8-68.4

Max/Min SEC Sunspot Number- 00 to 11

Max/Min Solar Wind Speed- 273-349

Max/Min Averaged Daily Background X-Ray Flux- A0.0-A0.0

Max/Min Dst Index- -14 to +22, via Kyoto

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- A weak southern hemisphere high velocity solar wind stream emanating from a newly formed un-numbered geoeffective (Earth facing) southern Coronal Hole did not create a negative impact on propagation conditions.

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet geomagnetic levels, with a range of 00-07.

The Kp index had been at quiet geomagnetic levels, with a range of 0 to 2.

The Boulder mid latitude K index had been at quiet geomagnetic levels, with a range of 0 to 2.

The high latitude K index (via Troms, Norway) had been at quiet geomagnetic levels to active geomagnetic levels, with a range of 0 to 4. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

8.) E Valley/F Layer Propagation Ducting Mechanism/Chordal Hop Propagation-

Antenna polarization plays a large role in the success of a long haul DX contact. As a medium frequency RF signal traverses our planets magnetic lines of force in a perpendicular manner on high and mid latitude paths say between W3 land and SM, higher angle horizontally polarized signals are more readily absorbed then lower angle vertically polarized signals. On other paths on the globe opposite results can be found, i.e. horizontally polarized signals suffer less absorption on a propagation path between VK6 and W4.

You would expect a true long path QSO on 160 to be theoretically possible but improbable on most paths during any season. However a G to VK long path might be possible if the E Valley/F layer ducting propagation mechanism or the Chordal Hop propagation mechanism is involved. A 160 meter signal can traverse a daylight path via these propagation modes if the transmitted signal enters/exits at each end of the path at or near sunrise/sunset when the D layer ionization is weak (ionospheric tilting).

The downward tilt of ionospheric layers is eastward at sunrise. As a result, signals coming from the west are refracted downward at steeper angles and are therefore heard better on higher angle antennas. The opposite is true at local sunset.

A note though, the E-valley/F layer ducting propagation mechanism does not exist only during gray line periods. Internal Buoyancy/Gravity Waves (IBGW's) are a source of the ducting mechanism and allow for occurrences of ducting along any propagation path in total darkness. Measurement of the timing of arrival of propagated medium frequency RF signals demonstrates the existence of the ducting mechanism, versus conventional numerous E layer land/ocean surface hops.

The majority of the time medium frequency RF signals in excess of approximately 3200 miles propagate via the E Valley/F Layer propagation mechanism or via the Chordal Hop (mostly on HF near local sunrise and sunset) propagation mechanism. High solar flux values above 150 can aid in long haul medium frequency propagation, as high solar flux values ensure a strong F layer half of the E Valley/F Layer duct mechanism. Typically the majority of transmit antenna's radiation must be focused between 40-60 deg. to enter the E Valley/F Layer duct.

Well Known Chordal Hop LP Routes Courtesy Of Larry Duncan K4WLS

Here are some well known Chordal Hop LP routes from the East Coast and Mid-West:

Late Afternoon, Mid-February to Mid-March - Western Australia and beyond, and Southern Malaysia: Predominately 20M.

0700-1000 Local, Early to Late Summer - Eastern and Southern Africa, and Indian Ocean: 20, 15, 17, 12, and 10M (17 through 10M depending on Solar Flux).

0800-1000 Local, Early Fall - Western Australia and S.E. Indian Ocean: 20M

0500-0700 Local, * December - Malaysia, Indonesia, and S.E. Asia: 40M

Sunset to 1 Hour Before, Fall to Mid-December - Middle and Eastern Asia: 40M

0700-0800 Local, Mid-December - Middle East: Predominately 20M

Sunset to 1 Hour Before, Mid-December - Northern Middle and Eastern Asia: 20 and 40M (20M depending on Solar Flux).

* Sporadically as late as early March

If one is lucky enough to be on the receive end of a ducted medium frequency signal due to an IBGW or two, a change in the vertical and/or horizontal electron gradient will allow the RF to drop out of the duct at your QTH.

A note, high solar activity in the form of increased ionization created by ultraviolet and X-ray radiation, can fill in the E Valley/F Layer ducting region with medium frequency absorptive ionization and interfere with the E Valley/F Layer ducting mechanism. In a sense the E/F layer duct is shut down and the medium frequency RF signal can only propagate between the E layer and land/ocean surface, at a higher angle and with more signal loss. This closing of the duct can be reciprocal on each end of the propagation path or one way only. (((((When closing of the duct occurs the advantage of a low angle vertical radiator is lost, with a higher takeoff angle horizontal dipole making the contact still possible, albeit maybe weaker.)))))

Medium frequency radio waves possess elliptical polarization, with the signal splitting into ordinary and extra-ordinary rays. These rays can propagate in or out of phase, more often out of phase. The out of phase extra-ordinary ray represents a 50% power loss on the receive end of a propagation path.

As follows is a recent experience I had in Florida with this propagation mode on 160 meters.

I began listening for DX on 160 meters at 5:00 pm EST this evening February 05-06, 2006. I was watching the OH2AQ spot and the stations in ME to VA were working stations in Europe and Africa. I could hear the stateside stations real well but not a peep out of any DX.

Then right at my local sunset which was at 6:15 pm EST it was like flipping a switch as all the DX stations just showed up. It was a classic example of the E Valley-F Layer ducting mechanism propagation mode with the duct opening up right over Florida as the ionized layers changed height with the arrival of the grey line terminator.

Once the DX showed up I heard oodles of CW DX stations including VQ9LA and 6W/G4WFQ who were 55 on the receive loop. MM0SJH, G3FPQ and I7RIZ showed up on phone between 1841 and 1849 kc and they were 57. I didn't bother to work anything this time as the only countries I heard that I've never worked were VQ9LA and 6W/G4WFQ and I couldn't break the pileups with 100 watts.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

Back To The Top

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-006

Date Format is MM/DD/YYYY

Published Thursday 11/01/2007 At 2200 UTC Valid 11/02-11/08/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- POOR for ham signals and FAIR for broadcast signals.

Nighttime- FAIR for ham signals and GOOD for broadcast signals.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR to GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR to GOOD Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect GOOD to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

 

-Expect POOR to FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect POOR to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be POOR to FAIR.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be POOR to FAIR.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- FAIR to GOOD on 80-30 meters.

Mid Latitude- FAIR to GOOD on 80-30 meters.

High Latitude- FAIR on 80-30 meters.
 

Low Latitude- FAIR on 20-17 meters.

Mid Latitude- FAIR on 20-17 meters.

High Latitude- POOR to FAIR on 20-17 meters.

 

Low Latitude- FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

https://thunderstorm.vaisala.com/tux/jsp/explorer/explorer.jsp 

http://www.uspln.com/images/uspln.jpg  

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts, associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.
 
Northern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 10/26-11/01/2007-

The period saw quiet to active conditions with brief minor (Kp-5) geomagnetic storming conditions, courtesy of a high velocity solar wind stream emanating from geoeffective (Earth facing) southern Coronal Hole #297.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters. There were few Sporadic E (Es) openings on 6 through 20 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There were no sunspot groups visible and the solar flux index stayed below 70, so there was no HF propagation boost on 10-20 meters during the period. We are now at 25 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. However one had been visible on the far side of the Sun via the SOHO holographic image.

By the way anecdotal evidence points to solar cycle 23 minimum in September 2007 with a monthly international sunspot number of 2.4. The lowest daily solar flux reading since July 1996 of 64.4 occurred on September 28, 2007. The lowest maximum daily solar flux reading since October 1996 of 71 occurred on September 01, 2007.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. The moderate absorption produced poor propagation conditions, especially in comparison to recent weeks that had seen some of the best propagation conditions since 1996.

There was minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. The moderate absorption produced poor propagation conditions.

There was at times reduced daytime signal absorption and minor to moderate signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

At times intense lightning QRN hampered receive conditions on 160, 80, 40 and 30 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 11/02-08/2007-

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters. There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters. Little in the way of Sporadic E (Es) openings will occur on 10-20 meters either.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit:

None.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters.

I expect minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. This should lead to some improvement in propagation conditions especially in comparison to last week.

I expect moderate signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

I expect normal daytime signal absorption and normal minor night time signal absorption on the LF band on high and mid latitude paths. 

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80 and 40.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60, 49 and 41 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

Kp 0-3, isolated Kp- 4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions MAY OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is LOW.

Daily solar flux index levels (SFI) should range between 67-68.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be POSITIVE.

Propagation Forecast Scales-

LOW- 25%

MEDIUM- 50%

HIGH- 75%

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 10/26/2007 TO 2200 UTC 11/01/2007

 

Sunspot Groups-

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 66.8-68.4

Max/Min SEC Sunspot Number- 00 to 00

Max/Min Solar Wind Speed- 357-690

Max/Min Averaged Daily Background X-Ray Flux- A0.0-A0.0

Max/Min Dst Index- -34 to +4, via Kyoto

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- southern hemisphere CH #297 (old #293)

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 2-48.

The Kp index had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 0 to 5.

The Boulder mid latitude K index had been at quiet geomagnetic levels to active geomagnetic levels, with a range of 0 to 4.

The high latitude K index had been at quiet geomagnetic levels to strong geomagnetic storming levels, with a range of 1 to 7, via Troms, Norway. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

7.) Correlation Of Energetic Protons, Solar Flux and Ap & Kp Indices With Medium Frequencies-

I've been observing energetic proton levels, as well as the Ap & Kp indices for 31 years and see a direct correlation between high energetic proton levels above 10 MeV (10+0) and poor propagation on high and at times mid latitude medium frequency paths at day AND night, where as the A & K indices don't as readily correlate. (See paragraph three of definition #2. Aurora Oval Blockage, Absorption And Refraction) and (definition #7. High Latitude Path Skewing) for a further explanation on the lack of correlation of Ap & Kp indices with medium frequency propagation conditions.

High solar flux values are "incorrectly" considered to be detrimental to medium frequency signals both domestic and TA/TP, as more absorption can be present as the transmitted signal makes two trips through the D layer, near sunrise and sunset. However most medium wave frequency RF signals in excess of 3100 miles are propagated via the E valley/F layer ducting and/or Chordal Hop/Pederson Ray propagation mechanism and a high solar flux value ensures a strong E valley/F layer duct mechanism. Actually a solar flux of at least 150 is needed for the E valley/F layer ducting mode.

The main reason that medium frequency radio propagation "seems to be better" at the bottom of a sunspot cycle is not so much due to lower solar flux levels BUT due to much less geomagnetic activity.

Keep in mind though that the 10.7 cm (2800 mhz) solar flux index is not a "reliable" gauge of ionization in our atmosphere, as the energy of photons at this frequency is to low on the order of one million times. However most are used to solar flux and sunspot number and it's a hard habit to break. A better indicator is the inter-related background X-ray flux. (See definition #1 paragraphs e & f).

An elevated energetic proton flux level greater then (10+0) creates noticeably increased winter time day and year round night time D layer absorption of medium wave frequencies, especially on high latitude propagation paths but it can also negatively impact mid latitudes, depending on the intensity of the event.

Elevated energetic proton events too small to be categorized as a Polar Cap Absorption event (PCA) can still impact high and at times mid latitude medium frequency propagation paths in the form of excessive D layer absorption.

((((Note, high latitude medium frequency radio propagation paths can still be disturbed for days and up to weeks, following the end of an official >10 MeV (10+0) proton event.))))

GENERAL GUIDELINES CONCERNING CORRELATION OF PROPAGATION INDICES TO ACTUAL MF/HF PROPAGATION CONDITIONS.

NOTE!!!  The propagation indices "interpretations" are my personal intellectual property. Therefore the propagation indices interpretations contained herein is copyrighted © 1988-2007 by Thomas F. Giella, KN4LF, all rights reserved. Reproduction of information herein is allowed without permission in advance as long as proper credit is given.

1.) Dropping indices numbers are better.

2.) A solar flux of 150 or higher, 200+ best, for medium frequencies under 100, under 70 best.

Keep in mind though that the 10.7 cm (2800 mhz) solar flux index is not a "reliable" gauge of ionization in our atmosphere for F layer medium frequency refractions, as the energy of photons at this frequency is to low on the order of one million times. However most are used to solar flux and sunspot number and it's a hard habit to break. A better indicator is the background X-Ray Flux. See #7 below.

3.) Solar flux of at least 150 for E Valley/F Layer ducting mechanism.

4.) Previous 24 hour Ap index under 10, under 7 for several days consecutively is best.

5.) Previous 3 hour Kp index under 3 for mid latitude paths, under 2 for high latitude paths, 0-1 for several days consecutively is best.

6.) Energetic protons no greater then 10 MeV (10+0).

7.) Background X-Ray flux levels less than A1 for several days consecutively.

8.) No current STRATWARM alert.

9.) Interplanetary Magnetic Field (IMF) Bz with a (positive number) sign, indicates a lesser chance of high latitude path auroral absorption/unpredictable refraction or scattering of medium frequency RF signals, when the Kp is above 3.

10.) A -50 or better towards a positive number Dst index during the recovery time after a Geomagnetic Storm, as related to the Equatorial Ring Current. A positive is number best.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

 

Back To The Top

 

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-005

Date Format is MM/DD/YYYY

Published Thursday 10/25/2007 At 2200 UTC Valid 10/26-11/01/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- POOR for ham signals and FAIR for broadcast signals.

Nighttime- POOR for ham signals and POOR for broadcast signals between 10/26-28/2007.

POOR to FAIR for ham signals and FAIR to GOOD for broadcast signals between 10/29-11/01/2007.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect POOR to FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

*Expect POOR to FAIR Northern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect GOOD to FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

-Expect POOR to FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect GOOD to FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR to FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 10/26-28/2007, then FAIR between 10/29-11/01/2007.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 10/26-28/2007, then FAIR between 10/29-11/01/2007.

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR between 10/26-28/2007, then GOOD between 10/29-11/01/2007.

Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR between 10/26-28/2007, then GOOD between 10/29-11/01/2007.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR to GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be FAIR.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be FAIR between 10/26-28/2007, then GOOD between 10/29-11/01/2007.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be FAIR between 10/26-28/2007, then GOOD between 10/29-11/01/2007.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- GOOD on 80-30 meters.

Mid Latitude- FAIR to GOOD on 80-30 meters.

High Latitude- POOR between 10/26-27/2007, then FAIR between 10/28-11/01/2007 on 80-30 meters.
 

Low Latitude- FAIR on 20-17 meters.

Mid Latitude- FAIR on 20-17 meters.

High Latitude- POOR between 10/26-27/2007, then FAIR between 10/28-11/01/2007 on 80-30 meters.

 

Low Latitude- FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

https://thunderstorm.vaisala.com/tux/jsp/explorer/explorer.jsp 

http://www.uspln.com/images/uspln.jpg  

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts, associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.
 
Northern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION OF PAST CONDITIONS-

 

For 10/19-25/2007-

Per my last forecast the period was a mixed bag, with minor (Kp-5) geomagnetic storming conditions on the 19th, active (Kp-4) geomagnetic conditions on the 20th, quiet to unsettled (Kp-0 to 3) geomagnetic conditions between the 20-24th and minor to moderate (Kp-5 to 6) geomagnetic storming conditions beginning at 1800 UTC on the 25th.  The conditions late on the 25th were courtesy of a high velocity solar wind stream emanating from geoeffective (Earth facing) Coronal Hole #296.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters. There were few Sporadic E (Es) openings on 6 through 20 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was significant east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There were no sunspot groups visible and the solar flux index stayed below 70, so there was no HF propagation boost on 10-20 meters during the period. We are now at 17 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. However one had been visible on the far side of the Sun via the SOHO holographic image.

By the way anecdotal evidence points to solar cycle 23 minimum in September 2007 with a monthly international sunspot number of 2.4. The lowest daily solar flux reading since July 1996 of 64.4 occurred on September 28, 2007. The lowest maximum daily solar flux reading since October 1996 of 71 occurred on September 01, 2007.Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. At times propagation conditions along low, mid and high latitude paths was excellent, reminiscent of the fall of 1996.

There was minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

There was at times reduced daytime signal absorption and minor to moderate signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

At times intense lightning QRN hampered receive conditions on 160, 80, 40 and 30 meters.

 

DISCUSSION OF FUTURE CONDITIONS-

 

For 10/26-11/01/2007-

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters. There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters. Little in the way of Sporadic E (Es) openings will occur on 10-20 meters either.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit:

#10972 on 10/26/2007 with a beta magnetic signature.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters.

I expect minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere.

I expect moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

I expect normal to at times reduced daytime signal absorption and minor to moderate signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80, 40 and 30 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60, 49, 41 and 31 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

10/26-11/01/2007 Kp 0-5, isolated Kp- 6.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions MAY OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, #297 which is a recurrent southern hemispheric (old #293).

Daily solar flux index levels (SFI) should range between 66-69.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be POSITIVE.

 

Propagation Forecast Scales-

LOW- 25%

MEDIUM- 50%

HIGH- 75%

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 2200 UTC 10/18/2007 TO 2200 UTC 10/25/2007

 

Sunspot Groups-

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Max/Min Solar Flux Readings- 67.0-69.1

Max/Min SEC Sunspot Number- 00 to 00

Max/Min Solar Wind Speed- Unavailable

Max/Min Averaged Daily Background X-Ray Flux- A0.0-A0.0

Max/Min Dst Index- -32 to -12 via G3YNK

Solar Flares- C-0 M-0 X-0

Elevated Energetic Protons >10 MeV (10+0)- 0

Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- transequatorial CH #296 (old #292)

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to unsettled geomagnetic levels, with a range of 0-15.

The Kp index had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6.

The Boulder mid latitude K index had been at quiet geomagnetic levels to minor geomagnetic storming levels, with a range of 0 to 5.

The high latitude K index had been at quiet geomagnetic levels to moderate geomagnetic storming levels, with a range of 0 to 6, via Troms, Norway. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

 

6.) Solar Filament-

A relatively cool and dense ribbon of gas held together by solar magnetic fields. From Earth they usually appear as relatively dark lines across the face of the Sun. At times the magnetic lines holding the filament open up creating a tremendous eruption similar in size and impact of a Coronal Mass Ejection (CME). (See definition #4. Coronal Mass Ejection). (See definition #11. Geomagnetic/Ionospheric Storm).

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

 

Back To The Top

 

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-004

Date Format is MM/DD/YYYY

Published Thursday 10/18/2007 At 2200 UTC Valid 10/19-25/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- POOR for ham signals and FAIR for broadcast signals.

Nighttime- POOR for ham signals and FAIR for broadcast signals on 10/19. FAIR for ham signals and GOOD for broadcast signals between 10/20-22. POOR for ham signals and FAIR for broadcast signals between 10/24-25/2007.

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR TO GOOD Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect FAIR TO POOR Northern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

-Expect FAIR TO GOOD Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect FAIR TO POOR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be FAIR TO GOOD.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR on 10/19, to GOOD between 10/20-22, then FAIR on 10/24-25.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR on 10/19, to GOOD between 10/20-22, then FAIR on 10/24-25.
 

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be FAIR on 10/19, TO GOOD between 10/20-22, then FAIR on 10/24-25.

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be FAIR on 10/19, TO GOOD between 10/20-22, then FAIR on 10/24-25.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

 

Lower frequency (80-30 meters) propagation conditions tend to be impacted in a negative manner not by the maximum usable frequency (MUF) along a particular propagation path and time but rather due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). Also D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0).

Higher frequency (20-10 meters) propagation conditions tend to be impacted in a negative manner by the maximum usable frequency (MUF) along a particular propagation path and time and to a lesser extent due to geomagnetic storms that increase signal absorption via the E layer (the altitude of the Radio Aurora). D layer signal absorption due elevated proton flux at energies greater than 10 MeV (10+0) is inconsequential on 20-10 meters.

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- GOOD on 80-30 meters.

Mid Latitude- GOOD on 80-30 meters.

High Latitude- FAIR on 10/19, GOOD between 10/20-22, then FAIR between 10/24-25/2007 on 80-30 meters.

 

Low Latitude- FAIR on 20-17 meters.

Mid Latitude- FAIR on 20-17 meters.

High Latitude- FAIR to POOR on 10/19, then FAIR between 10/20-22, then FAIR to POOR between 10/24-25/2007 on 20-17 meters.

 

Low Latitude- FAIR on 15-10 meters.

Mid Latitude- POOR to FAIR on 15-10 meters.

High Latitude- POOR on 15-10 meters.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

https://thunderstorm.vaisala.com/tux/jsp/explorer/explorer.jsp 

http://www.uspln.com/images/uspln.jpg  

A global view of near real time lightning strike data:

http://webflash.ess.washington.edu  

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts, associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.
 
Northern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION-

 

For 10/12-18/2007-

Overall the period was very quiet.

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs negatively impacted 6, 10, 12, 15, 17 and 20 meters. There were few Sporadic E (Es) openings on 6 through 20 meters.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 10, 12 and 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There were no sunspot groups visible and the solar flux index stayed below 70, so there was no HF propagation boost on 10-20 meters during the period. We are now at 11 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. However one has been visible on the far side of the Sun via the SOHO holographic image.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere.

There was minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

There was normal daytime signal absorption and little signal absorption on night time propagation conditions on the LF band on high and mid latitude paths.

At times intense lightning QRN hampered receive conditions on 160, 80, 40, 30 and to a lesser extent on 20 meters.

 

DISCUSSION-

 

For 10/19-25/2007-

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters. There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters. Little in the way of Sporadic E (Es) openings will occur on 10-20 meters either.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 10, 12 and 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit:

#10971 on 10/19/2007 as a beta magnetic signature.

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters.

I expect minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere.

I expect minor to moderate night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

I expect normal to at times reduced daytime signal absorption and minor to moderate signal absorption on night time propagation conditions on the LF band on high and mid latitude paths. 

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80, 40 and 30 meters and to a lesser extent on 20 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60, 49, 41 and 31 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

10/19-25/2007 Kp 0-4, isolated Kp- 5.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions WILL OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions MAY OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, #296 which is a recurrent southern hemispheric (old #292).

Daily solar flux index levels (SFI) should range between 66-70

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE.

 

Propagation Forecast Scales-

LOW- 25%

MEDIUM- 50%

HIGH- 75%

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 0000 UTC 10/12/2007 TO 2200 UTC 10/18/2007

 

Sunspot Groups-

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Solar Flux Readings- 67.0-69.1

SEC Sunspot Number- 00 to 00

Solar Wind Speed- 273-475

Solar Flares- C-0 M-0 X-0
 
Averaged Daily Background X-Ray Flux- A0.0-A0.0

Dst Index- -22 to -6 via G3YNK

Elevated Energetic Protons >10 MeV (10+o)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- transequatorial CH #295 (old #291)

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to unsettled geomagnetic levels, with a range of 0-9.

The Kp index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3

The Boulder mid latitude K index had been at quiet to active geomagnetic levels, with a range of 0 to 4.

The high latitude K index had been at quiet to active geomagnetic levels, with a range of 0 to 4, Troms, Norway. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

 

5.) Coronal Hole-

The Corona is not part of the Sun's surface. It is instead part of the Sun's atmosphere, much like Earth's troposphere. Coronal Holes are low density areas associated with open magnetic field lines and are found near the Sun's poles at the bottom of a sunspot cycle and everywhere during a cycle maximum. A Coronal Hole is a dark region where a breakdown in the magnetic field structure in the solar corona has occurred. From these regions stream the high velocity solar wind that are a source of geomagnetic storming on Earth.

Coronal Holes occur most often on the downside of a solar cycle and their absence at the bottom of a solar cycle and at the beginning of the next, allow for the best medium frequency radio propagation conditions. Many think it's the lower solar flux values seen at the bottom of a solar cycle that accounts for improved propagation conditions but it's actually pretty much a lack of Coronal Holes and geomagnetic storming. (See definition #11. Geomagnetic/Ionospheric Storm).

One thing to keep in mind is that the high velocity solar wind stream emanating from a Coronal Hole is a neutral phenomena with respect to the Bz (magnetic component) of the Interplanetary Magnetic Field (IMF). If the Bz component is negative (southward) prior to arrival of the solar stream, there will exist a tendency to see a larger swing negative after the disturbance arrives. If the Bz component is positive (northward) prior to arrival of the solar stream, there will exist a tendency to see a larger swing positive after the disturbance arrives.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

 

Back To The Top

 

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-003

Date Format is MM/DD/YYYY

Published Thursday 10/11/2007 At 2200 UTC Valid 10/12-18/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- Poor for ham signals and fair for broadcast signals.

Nighttime- Fair for ham signals and good for broadcast signals.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect POOR TO FAIR Northern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

-Expect FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR TO FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be GOOD.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR TO GOOD.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR TO GOOD. 

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Northern Hemisphere high latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Southern Hemisphere high latitude propagation conditions in excess of 3200 miles should be GOOD.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL HF 3000-30000 KC PROPAGATION CONDITIONS EXPECTED-

 

Low: 0-25 degrees

Mid: 25-60 degrees

High: 60-90 degrees

 

Low Latitude- Good.

Mid Latitude- Good.

High Latitude- Good.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL NOISE (QRN) OUTLOOK-
 
U.S. near real time lightning strike data:

https://thunderstorm.vaisala.com/tux/jsp/explorer/explorer.jsp  

http://www.uspln.com/images/uspln.jpg  

 

A global view of near real time lightning strike data:

http://flash.ess.washington.edu  

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Northern hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Northern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts, associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.
 
Northern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to fall season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

During the outlook period there will be HIGH thunderstorm lightning induced QRN levels in low latitude areas of the Southern Hemisphere due to the proximity of the Inter Tropical Convergence Zone (ITCZ) and tropical warm core low pressure systems.

Southern hemisphere mid latitude regions can expect HIGH TO MODERATE thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems and tropical warm core low pressure systems.

Southern hemisphere high latitude regions can expect MODERATE TO LOW thunderstorm lightning induced QRN tied to spring season cold/warm/occluded fronts and associated extra-tropical cold core low pressure systems.

 

END OF OUTLOOK

 

DISCUSSION-

 

For 10/05-11/2007-

Overall the period was quiet.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there was east-west F layer propagation on 17 meters. There were intermittent east-west propagation openings on 10, 12 and 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there was little east-west F layer propagation on 10, 12 and 15, meters. However there were intermittent east-west propagation openings on 17 meters.

There was one sunspot group briefly visible #10972 but the solar flux index stayed below 70, so there was no HF propagation boost on 10-20 meters during the period. We are now at 4 days consecutively with no visible sunspot groups on the Earth facing side of the Sun. However a few have been visible on the far side of the Sun via the SOHO holographic image.

Trans-equatorial (TEQ) HF propagation between North and South America occurred, as well as between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There was minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere.

There was minor night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere.

There was normal daytime signal absorption and little signal absorption on night time propagation conditions on the LF band on high and mid latitude paths.

 

DISCUSSION-

 

For 10/12-18/2007-

Globally with the daily sunspot number and vaguely related solar flux level very low, reduced F layer MUFs will negatively impact 10, 12, 15, 17 and 20 meters. There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters. Little in the way of Sporadic E (Es) openings will occur on 10-20 meters either.

In the Northern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore higher MUFs, there will be east-west F layer propagation on 17 meters. There will be intermittent east-west propagation openings on 10, 12 and 15 meters.

In the Southern Hemisphere due to seasonal chemical changes in the F layer of the ionosphere and therefore lower MUFs, there will be little east-west F layer propagation on 10, 12 and 15, meters. However there will be intermittent east-west propagation openings on 17 meters.

The following old sunspot groups may rotate around the east limb of the Sun during the forecast period if they survived the back side transit: None..

Trans-equatorial (TEQ) HF propagation between North and South America will occur, as well between southern Africa to Europe/West Asia and also Australia to Eastern Asia/Oceania.

There will be no F layer and little in the way of Sporadic E (Es) openings on 6 meters..

I expect no appreciable night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Northern Hemisphere. This will lead to some of the best propagation conditions since the fall of 1996.

I expect no appreciable night time signal absorption on the MF AM broadcast band, 160 and 120 meters on high latitude propagation paths in the Southern Hemisphere. This will lead to some of the best propagation conditions since the fall of 1996.

I expect normal daytime signal absorption and little signal absorption on night time propagation conditions on the LF band on high and mid latitude paths between. 

Occasionally high thunderstorm lightning QRN levels will continue to plague amateur radio operations on 160, 80, 40 and 30 meters and to a lesser extent on 20 meters.

Occasionally high thunderstorm lightning QRN levels will continue to plague SWL radio operations on 120, 90, 60, 49, 41 and 31 meters.

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC CONDITIONS EXPECTED-

 

10/12-18/2007 Kp 0-3, isolated Kp- 4.

During the period quiet (Kp 0-2) geomagnetic conditions WILL OCCUR.

During the period unsettled (Kp- 3) geomagnetic conditions WILL OCCUR.

During the period active (Kp- 4) geomagnetic conditions MAY OCCUR.

During the period minor (Kp- 5) geomagnetic storming conditions WILL NOT OCCUR.

During the period moderate (Kp- 6) geomagnetic storming conditions WILL NOT OCCUR.

During the period strong (Kp- 7) geomagnetic storming conditions WILL NOT OCCUR.

During the period severe (Kp- 8) geomagnetic storming conditions WILL NOT OCCUR.

During the period extreme (Kp- 9) geomagnetic storming conditions WILL NOT OCCUR.

The chance of polar cap absorption on high latitude propagation paths due to excessive energetic protons >10 Mev (10+0) is LOW.

The chance of daylight side SID radio blackouts from solar flares is LOW.

The chance of a geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a partially geoeffective (Earth facing) Coronal Mass Ejection (CME) is LOW.

The chance of a geoeffective (Earth facing) Coronal Hole is HIGH, #295 which is a recurrent transequatorial (old #291).

Daily solar flux index levels (SFI) should range between 65-69.

The probability of a small C class solar flare is LOW.

The probability of a large M class solar flare is LOW

The probability of a huge X class solar flare is LOW.

The NOAA/SEC Wang-Sheeley-Arge model forecasts the interplanetary magnetic field (IMF) polarity to be NEGATIVE between 10/12-18/2007.

 

Propagation Forecast Scales-

LOW- 25%

MEDIUM- 50%

HIGH- 75%

 

SOLAR, SPACE WEATHER AND GEOMAGNETIC INDICES FOR THE PERIOD 0000 UTC 10/05/2007 TO 2200 UTC 10/11/2007

 

Sunspot Groups-

No partially or totally geoeffective (Earth Facing) sunspot groups contained a twisted magnetic signature capable of producing large M class and huge X class solar flares.

Solar Flux Readings- 66.8-69.7

SEC Sunspot Number- 00 to 15

Solar Wind Speed- 278 to 491

Solar Flares- C-0  M-0 X-0
 
Averaged Daily Background X-Ray Flux- A0.0-A2.0

Dst Index- -30 to -7 via G3YNK

Elevated Energetic Protons >10 MeV (10+o)- 0
 
Geoeffective (Earth Facing) Coronal Mass Ejections- 0

Partially geoeffective (Earth Facing) Coronal Mass Ejections- 0

Geoeffective (Earth facing) Coronal Holes- CH #294

Polar cap absorption on high latitude propagation paths did not occur due to excessive energetic protons >10 Mev (10+0).

The Ap index had been at quiet to unsettled geomagnetic levels, with a range of 0-12.

The Kp index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3.

The Boulder mid latitude K index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3.

The high latitude K index had been at quiet to unsettled geomagnetic levels, with a range of 0 to 3, Troms, Norway. 

 

PROPAGATION LESSON-

From http://www.kn4lf.com/kn4lf8.htm

 

4.) Coronal Mass Ejection (CME)-

A Coronal Mass Ejection is the name given to an ejection of a large amount of matter from the Sun's outer atmosphere or corona. These ejections typically comprise millions of tons of material in the form of charged particles and can be seen because the material reflects sunlight. When one of these ejections is directed towards the Earth (or conversely, directly away from the Earth), it looks like a roughly circular "halo" surrounding the blanked out Sun.

The "Halo CME's" are those CME's which are more likely to impact the Earth than those which are shot out at right angles to the Earth-Sun line. Energetic protons emitted during CME's play a major role in increased day time and night-time D layer absorption of medium frequencies.

Coronal Mass Ejections were once thought to be completely initiated by solar flares. However it is now known that many (CME's) are not associated with Solar Flares but instead with collapsing Solar Filaments. If a (CME) collides with the Earth, it can excite a Geomagnetic Storm if the polarity of the Interplanetary Magnetic Field (IMF) has a negative sign. We must be vigilant in watching for geo-effective (CME's), in order to not be caught by surprise with a seemingly sudden and unexpected Geomagnetic Storm.

Coronal Mass Ejections are not random meaningless eruptions but instead a process by which the Sun expels complex magnetic signatures enroute to changing its magnetic polarity or said a different way the swapping of the Sun's magnetic poles. Basically the Sun swapped its magnetic polarity at the peak of present solar cycle 23 somewhere between July 2000 and December 2001. The next polarity swap will occur during solar cycle 24 somewhere around 2010-2011.

 

SPACE WEATHER SCALES-
 
Kp Indices-
 
G5 = Extreme Storm - Kp = 9
G4 = Severe Storm - Kp = 8
G3 = Strong Storm - Kp = 7
G2 = Moderate Storm - Kp = 6
G1 = Minor Storm - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

 

Ap Indices-
 
Ap 100-400 Severe Storm
Ap 50-99 Major Storm
Ap 30-49 Minor Storm
Ap 16-29 Active
Ap 8-15 Unsettled
Ap 0-7 Quiet
 
Correlation Of Kp To Ap Indices-
 
K- 0= A- 0
K- 1= A- 3
K- 2= A- 7
K- 3= A- 15
K- 4= A- 27
K- 5= A- 48
K- 6= A- 80
K- 7= A- 140
K- 8= A- 240
K- 9= A- 400

 

Back To The Top

 

KN4LF Daily LF/MF/HF Frequency Radiowave Propagation Forecast #2007-002

Date Format is MM/DD/YYYY

Published Thursday 10/04/2007 At 2200 UTC Valid 10/05-11/2007

 

GLOBAL LF 30-300 KC PROPAGATION CONDITIONS EXPECTED-

 

Daytime- Fair for ham signals and broadcast signals on 10/05/2007.

Nighttime- Poor for ham signals and fair for broadcast signals on 10/05/2007.

 

Daytime- Poor for ham signals and fair for broadcast signals between 10/06-11/2007.

Nighttime- Fair for ham signals and good for broadcast signals between 10/06-11/2007.

 

Propagation Forecast Scales-
 
Excellent- +1 db Over S9 Or better
Good- S7-9
Fair- S4-6
Poor- S1-3

 

GLOBAL MF 300-3000 KC PROPAGATION CONDITIONS EXPECTED WITH AN EMPHASIS ON THE MF AM BROADCAST BAND, 160 METERS AND 120 METERS-

 

-Expect FAIR Northern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.
 
*Expect POOR TO FAIR Northern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

+Expect FAIR Northern Hemisphere domestic conditions on south TO north paths out to approximately 1100 miles.

-Expect FAIR Southern Hemisphere domestic propagation conditions on east-west paths out to approximately 1100 miles.

+Expect FAIR Southern Hemisphere domestic conditions on north TO south paths out to approximately 1100 miles.

*Expect POOR TO FAIR conditions on south TO north paths in the Southern Hemisphere out to approximately 1100 miles.

 

Equatorial region domestic propagation conditions out to approximately 1100 miles should be GOOD.

 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 10/05-06/2007 .
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be POOR between 10/05-06/2007 . 

High latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR TO GOOD between 10/06-11/2007.
 
High latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be FAIR TO GOOD between 10/06-11/2007. 

 

Mid latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Mid latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific and cross equatorial propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Low latitude Northern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.
 
Low latitude Southern Hemisphere (TA) Trans Atlantic, (TI) Trans Indian, (TP) Trans Pacific propagation conditions in excess of approximately 3200 miles should be GOOD.

 

Equatorial region to Northern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

Equatorial region to Southern Hemisphere mid latitude propagation conditions in excess of approximately 3200 miles should be GOOD.

&