The Sun Today :
Updated May 26, 2020
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| Solar Flare Risk |
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M-Class:
01%
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X-Class:
01%
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| Active Watches |
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Geomag. Storm
NO
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Radiation Storm
NO
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Solar X-Rays:
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Geomagnetic Field:
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| 3-Day Geomagnetic Forecast [Details] |
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May 26 |
May 27 |
May 28 |
2-3 (G0)
Max Kp |
2-3 (G0)
Max Kp |
2-3 (G0)
Max Kp |
Prob-M
01%
Prob-H
15% |
Prob-M
01%
Prob-H
15% |
Prob-M
01%
Prob-H
15% |
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SolarHam is a website all about the Sun and how it affects Earth. It is also an Amateur (Ham) Radio website.
SolarHam is routinely updated with breaking news, sometimes hours before other Space News websites. You can trust SolarHam.com for the most up to date and accurate solar information on the internet.
SolarHam.com launched on March 15, 2006. The purpose of the website is to provide real time solar news, as well as data from various sources, all located in one spot for easy navigation. Sources include,
NOAA Space Weather Prediction Center (SWPC),
Solar Dynamics Observatory (SDO),
Solar and Heliospheric Observatory (SOHO),
Solar Terrestrial Relations Observatory (STEREO),
Advanced Composition Explorer (ACE),
Large Angle and Spectrometric Coronagraph Experiment (LASCO),
as well as many others.
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Since April, 2006
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| Latest Space Weather News and Updates |
| May 17, 2020 @ 12:40 UTC |
| Plage Regions | |
Both regions belonging to Cycle 25 are now turning into view and appear to be spotless. Solar activity should remain at very low levels. Image below by SDO/HMI.
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| May 15, 2020 @ 01:30 UTC |
| Approaching Sunspot? | |
Good evening. A potential active region is currently hiding behind the east limb. Based on the high latitude location, it likely belongs to Solar Cycle 25. We will begin to see the region this weekend as it begins to turn into view. Image below by STEREO Ahead.
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| May 3, 2020 @ 19:00 UTC |
| Solar Update | |
Good afternoon. Solar activity remains at very low levels. The visible disk is currently void of visible sunspots, although a plage region belonging to Cycle 25 did pop up in the southeast quadrant. Image by SDO/HMI.
Geomagnetic activity is also at quiet levels. A weak transient from a coronal mass ejection (CME) observed on April 27th may pass our planet over the next 24-48 hours and could disturb our geomagnetic field. More updates will follow whenever necessary.
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Prepared jointly by the U.S. Dept. of Commerce, NOAA,
Space Weather Prediction Center
UPDATED 2019 May 26 0030 UTC
.24 hr Summary...
Solar activity was at very low levels. No Earth-directed CMEs were
observed in available satellite imagery.
.Forecast...
Solar activity is expected to persist at very low levels 26-28 May.
[Report of Solar-Geophysical Activity]
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A - Alpha (single polarity spot).
B - Beta (bipolar spot configuration).
G - Gamma (atypical mixture of polarities).
BG - Beta-Gamma (mixture of polarities in a dominantly bipolar configuration).
D - Delta (opposite polarity umbrae within single penumbra).
BD - Beta with a Delta configuration.
BGD - Beta-Gamma with a Delta configuration.
[Latest NOAA Sunspot Summary]
[Latest Solar Region Summary (SRS)]
[SolarHam Sunspot Summary]
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Sunspots 3.0
