Space Weather for January 4, 2024 UTC Time  

HMI Intensity
Latest | Movie | HARP

HMI Magnetogram
Latest | Movie

Coronal Holes
Analysis | Movie

SUVI 131 (Latest)
Movie

SUVI 304 (Latest)
Movies
Latest Imagery: SDO | AIA | GOES | GONG | STEREO | LASCO
Video: SDO | SOHO | STEREO | Helioviewer | YouTube
     

Solar Indices  (Jan. 4 @ 00:35 UTC)
SFI
SSN
AREA
140
63
350
2
4
50
WWV  |  Flux Data  |  Last 30 Days

3 Day Geomagnetic Forecast
Jan 4
Jan 5
Jan 6
3 (G0)
2 (G0)
2 (G0)

Max Kp

M-Lat   05%
H-Lat   25%
M-Lat   01%
H-Lat   20%
M-Lat   01%
H-Lat   20%

Probabilities

Geomagnetic Field and Aurora
Past 24 Hours:  Unsettled

Kp-Index  |  A-Indices  |  Magnetometers


Auroral Oval Forecast  |  South Pole

CME Tracking

No Event(s) Logged

Farside Watch

Latest Image  |  JSOC  |  STEREO

           


X-Rays

Current

Global D-LAYER Absorption
Current Solar Flare Threat
C-Flare: 95%
M-Flare: 45%
X-Flare: 15%
Proton: 90%

Flare Events (M2+) Past 48 Hours   |   Event Report   |   Top Solar Flares
M3.8
3536

Visible Sunspot Regions  |   Sunspot Summary   |   SRS (txt)
3534
B
3536
BG
3537
B
3538
B

Latest Space Weather News
Minor (S1) Radiation Storm
January 3, 2024 @ 20:10 UTC
Low energy proton levels streaming past Earth continue to gradually rise and is now finally at the minor (S1) radiation storm threshold. This is a direct result of the X5 solar flare now almost 72 hours ago. Needless to say, had AR 3536 been directly facing Earth when the flare was observed, a proton event and strong geomagnetic storm would have been very likely. Only minor HF signal degradation through the polar zones should be expected because of the minor (S1) storm.

CME Mostly A Miss / Storm Watch Cancelled
January 2, 2024 @ 20:05 UTC (Updated)
As of this update, the CME that left the Sun late on December 31st generated by an X5 solar flare has yet to be clearly detected. This means the western flank of the CME shock is likely traveling slower than predicted. Low energy proton levels remain elevated, so it is possible it could still pass our planet at some point during the next 12 hours. It is also possible that the impact would be weak, or it will pass too far behind Earth to notice. A minor (G1) geomagnetic storm watch remains in effect for now.

CME Mostly A Miss: According to the latest NOAA/SWPC update, the X5/CME was mostly a miss. Geomagnetic storming is no longer in the forecast. A further update will be provided should conditions change.

X5 CME Event Update
January 1, 2024 @ 18:40 UTC (Updated)
An official tracking model courtesy of NOAA/SWPC is now available for the X5.0 flare event. They are in fact calling for the extreme western edge of the associated CME to pass Earth by January 2nd. Geomagnetic storming will be possible should an impact be observed as predicted. Stay tuned for updates during the next 24 hours.


Site Information

SolarHam.com launched on March 15, 2006 with the purpose of providing real time Space Weather news and data from various sources, all in one location for easy navigation. The site was created and is still maintained solely by amateur (HAM) radio station Kevin VE3EN.

Data Sources

This website relays data and imagery from the following sources.

- NOAA Space Weather Prediction Center (SWPC)
- Solar Dynamics Observatory (SDO)
- Atmospheric Imaging Assembly (AIA)
- Solar Terrestrial Relations Observatory (STEREO)
- Deep Space Climate Observatory (DSCOVR)
- Large Angle and Spectrometric Coronagraph Experiment (LASCO)
- Solar and Heliospheric Observatory (SOHO)
- Lockheed Martin Solar & Astrophysics Laboratory (LMSAL)
- Global Oscillation Network Group (GONG)
- Space Weather Canada
- Australia Space Weather Services (SWS)

Contact Information

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