Space Weather for April 29, 2024 UTC Time  

HMI Intensity
Latest | Movie | HARP

HMI Magnetogram
Latest | Movie

Coronal Holes
Analysis | Movie

AIA 131 (Latest)
AIA Movie

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

Solar Indices  (Apr. 29 @ 00:35 UTC)
SFI
SSN
AREA
140
119
510
13
7
10
WWV  |  Flux Data  |  Last 30 Days

3 Day Geomagnetic Forecast
Apr 29
Apr 30
May 1
2-3 (G0)
2-3 (G0)
3-4 (G0)

Max Kp

M-Lat   05%
H-Lat   30%
M-Lat   05%
H-Lat   25%
M-Lat   10%
H-Lat   40%

Probabilities

Latest SWPC Forecast (@ 00:30 + 12:30 UTC)

Geomagnetic Field and Aurora
Past 24 Hours:  Quiet

Kp-Index  |  A-Indices  |  Magnetometers


Auroral Oval Forecast  |  South Pole

CME Tracking

No Event(s) Logged

Cactus  |  GMU Lab Detection

Farside Watch

Latest Image  |  JSOC  |  STEREO

           


X-Rays

Current

Global D-LAYER Absorption
Current Solar Flare Threat
C-Flare: 99%
M-Flare: 35%
X-Flare: 05%
Proton: 05%

Flare Events (M2+) Past 48 Hours   |   Event Report   |   Top Solar Flares
M3.1
3654
M2.5
3654
M3.7
3654

Visible Sunspot Regions  |   Sunspot Summary   |   SRS (txt)
3644
B
3646
A
3652
A
3654
BGD
3655
A
3658
B
3660
B
3661
A

Latest Space Weather News
M3.7 Solar Flare
April 29, 2024 @ 01:25 UTC (UPDATED)
A secondary and somewhat stronger M-Flare reaching M3.7 was detected around AR 3654 at 01:11 UTC (Apr 29). Coronal dimming is slightly evident in the latest imagery courtesy of SDO meaning a weak coronal mass ejection (CME) may be generated. This will only be confirmed once updated coronagraph imagery is available. A further update will be provided if necessary.

UPDATE: Coronagraph imagery shows that a CME does not appear to be associated with this solar flare.

Moderate Solar Activity
April 27, 2024 @ 22:10 UTC
Solar activity on Saturday was at moderate levels with a pair of M-Class solar flares around AR 3654, currently rotating into the southwest quadrant. The largest event was an M3.1 flare at 21:40 UTC (Apr 27). None of these events appear to be associated with coronal mass ejections. Magnetically speaking, the region does have some complexity and additional M-Flares will remain possible during the next 24 hours. All other regions in direct Earth view have been for the most part stable.

SolarHam.COM Now Primary Domain
April 26, 2024 @ 23:50 UTC
The SolarHam website has migrated back to .COM as the primary domain. https://www.solarham.com is now the main URL to use. There is still a few things left to work on, but mostly everything appears to be back to normal. Fingers crossed and thanks for your patience.


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

Any comments or questions regarding this website can be sent via E-Mail by clicking HERE.

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