Space Weather for April 27, 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  (Apr. 27 @ 00:35 UTC)
SFI
SSN
AREA
153
154
600
14
42
470
WWV  |  Flux Data  |  Last 30 Days

3 Day Geomagnetic Forecast
Apr 27
Apr 28
Apr 29
3-4 (G0)
3-4 (G0)
2-3 (G0)

Max Kp

M-Lat   20%
H-Lat   50%
M-Lat   15%
H-Lat   45%
M-Lat   05%
H-Lat   30%

Probabilities

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

Geomagnetic Field and Aurora
Past 24 Hours:  Storm (G1)

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: 75%
X-Flare: 15%
Proton: 15%

Flare Events (M2+) Past 48 Hours   |   Event Report   |   Top Solar Flares
No Noteworthy Flare Events Detected.

Visible Sunspot Regions  |   Sunspot Summary   |   SRS (txt)
3644
A
3646
B
3648
BG
3652
A
3654
BG
3655
A
3657
B
3658
B

Latest Space Weather News
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.

Pair of CMEs Observed
April 26, 2024 @ 23:60 UTC
Two coronal mass ejections are visible in the latest coronagraph imagery. The first was the result of an eruption beyond the northwest limb and is directed away from Earth. The second was the result of a prominence eruption near the southeast limb and so far appears to be off the Sun-Earth line.

Space Weather Update
April 25, 2024 @ 19:45 UTC
The cluster of sunspots in the southwest quadrant consisting of AR 3638, 3643, 3645 and 3647 is now turning onto the west limb. Other than minor C-Flares and a number of low level M-Flares, this region was not responsible for much in the way of solar excitement. Any potential eruptions around this region at this point should be directed away from Earth.

Elsewhere, AR 3648 in the northwest quadrant produced occasional C-Flares on Thursday. All other regions have been fairly quiet.

Geomagnetic activity is also at quiet levels. An increase to active levels (Kp4) is in the forecast for the next 48 hours when a combination of coronal hole stream and possible weak CME effects is predicted.

Stay tuned to SolarHam.com for the latest space weather news and information.


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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