Solar Weather

Solar Weather

Region 6 Army MARS would like to thank the scientists and research teams at The University of Massachusetts Lowell Center for Atmospheric Research for providing this valuable resource allowing us to determine the critical frequency (foF2) and maximum usable frequency (MUF).

Other Solar Weather Links of Interest


Latest Austin Ionosonde

This is the latest ionogram captured from the Austin Ionosonde. Updated every 5 minutes. This data is pushed to region6armymars.org as soon as it becomes available.

Latest Austin ionogram

Unusual D-Region Absorption Patterns

D-Region Absorption

Planetary K Index

Created with Highcharts 8.0.4Universal Time (captured @ 2025-04-05T17:52:38.153Z)Kp indexEstimated Planetary K index (3 hour data)00:00Apr 300:00Apr 400:00Apr 512:0012:0012:0000:00Apr 601234567892025-04-05T17:52:38.153ZBegin: Thu, 03 Apr 2025 00:00:00 GMT


Generally, as planetary K-Index rises, critical frequency is suppressed.

K-IndexEffect
0-2Inactive/Quiet, no impact on HF
3-4Unsettled/Active, minor HF fade in higher latitudes
5-6HF fade at higher latitudes
7-8HF sporadic
9HF impossible above 40M

Solar X-ray Flux

Created with Highcharts 8.0.4SWPC Warning ThresholdABCMXUniversal Time (captured @ 2025-04-05T17:52:38.269Z)Watts · m⁻²Xray Flare ClassGOES X-Ray Flux (1-minute data)GOES-16 ShortGOES-16 Long00:00Apr 312:0000:00Apr 412:0000:00Apr 512:002025-04-05T17:52:38.269Z
10-910-810-710-610-510-410-310-2


The X-ray radiation that ionizes the D-layer is the 1.0 - 8.0 A (red) plot. These measurements currently taken from the GOES 16 satelite.

Flare CategoryEffect
A1-B9No or minor impact on HF
C1Low absorption of HF signals
M1Occaisional loss of radio contact on sun-lit side
M5Limited HF blackout for several minutes
X1Wide area HF blackout for approx. 1 hr
X10HF blackout over most of sun-lit side for 1-2 hrs
X20Complete HF blackout of all sun-lit areas lasting hours

GOES Hp

Created with Highcharts 8.0.4Universal Time (captured @ 2025-04-05T17:52:38.367Z)NanoTesla (nT)GOES Magnetometers (1-minute data)GOES-16 Hp00:00Apr 312:0000:00Apr 412:0000:00Apr 512:000501001502002025-04-05T17:52:38.367Z


The GOES (Geo-Stationary) Hp plot is a measure of the earth's magnetic field in orbit above the earth. More details on the GOES-16 satellite.

Electron Flux

Created with Highcharts 8.0.4SWPC Alert ThresholdUniversal Time (captured @ 2025-04-05T17:52:38.408Z)Particles · cm⁻² · s⁻¹ · sr⁻¹GOES Electron Flux (5-minute data)GOES-16 ≥ 2 MeV00:00Apr 312:0000:00Apr 412:0000:00Apr 512:002025-04-05T17:52:38.408Z
100101102103104105106107


The red and blue lines correspond to the different measurements taken from the GOES 16 satellite.

Electron FluxEffect
>1.0e+03Partial to complete HF blackout in polar regions
<1.0e+03Degraded HF propagation in polar regions
<1.0e+02Minor impacts on HF in polar regions
<1.0e+01No impacts on HF

Proton Flux

Created with Highcharts 8.0.4SWPC 10 MeV Warning ThresholdUniversal Time (captured @ 2025-04-05T17:52:38.458Z)Particles · cm⁻² · s⁻¹ · sr⁻¹GOES Proton Flux (5-minute data)GOES-16 ≥ 10 MeVGOES-16 ≥ 50 MeVGOES-16 ≥ 100 MeV00:00Apr 312:0000:00Apr 412:0000:00Apr 512:002025-04-05T17:52:38.458Z
10-210-1100101102103104105106107


The NOAA Space Weather Prediction Center's proton event threshold is the 10 protons/cm2-s-sr at >=10 MeV (red) plot.

Proton FluxEffect
1.0e+06Complete HF blackout in polar regions
1.0e+05Partial HF blackout in polar regions
1.0e+04Degraded HF propagation in polar regions
1.0e+03Small effects on HF in polar regions
1.0e+02Minor impacts on HF in polar regions
1.0e+01Very minor impacts on HF in polar regions
1.0e+00No impacts on HF