On this page you will find all the information you need to spot any coronal holes on the earth-facing solar disk. Coronal holes are the source of fast solar wind streams which sometimes have the potential to produce minor to moderate geomagnetic storms. If our automated detection system recently detected an earth-facing coronal hole it will also be mentioned on this page.
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:59 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 20:02 UTC
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 13:56 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.5 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 130.4 -16.1 |