Begin Max End Rgn Loc Xray Op 245MHz 10cm Sweep 0133 0136 0136 200 0213 0213 0213 750 0918 0926 0937 8103 N22W21 C1.0 SF 120 0942 0943 0943 230
10 CM 094 SSN 060 AFR/AP 030/042 X-RAY BACKGROUND B2.4 DAILY PROTON FLUENCE (FLUX ACCUMULATION OVER 24 HRS) GT 1 MEV 9.7E+07 GT 10 MEV 2.1E+07 P/(CM2-STER-DAY) GOES-9 SATELLITE SYNCHRONOUS ORBIT W135 DEGREES) DAILY ELECTRON FLUENCE GT 2 MEV //// E/(CM2-STER-DAY) GOES-9 SATELLITE SYNCHRONOUS ORBIT W135 DEGREES) 3 HOUR K-INDICES: BOULDER 6 6 4 2 3 3 3 2 PLANETARY 5 7 6 4 4 4 3 1
A POLAR CAP ABSORPTION (PCA) EVENT ASSOCIATED WITH THE PROTON EVENTS DESCRIBED IN PART B. REMAINS IN PROGRESS. THE ELECTRON FLUENCE IS Not available DUE TO PROTON CONTAMINATION OF THE GOES ELECTRON SENSOR.
All times in UTC
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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The OVATION model predicts the Hemispheric Power Index to reach 50GW at 03:23 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 21:36 UTC
Severe G4 geomagnetic storm (Kp8) Threshold Reached: 20:55 UTC
Strong G3 geomagnetic storm (Kp7) Threshold Reached: 19:25 UTC
Moderate G2 geomagnetic storm (Kp6) Threshold Reached: 18:38 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/15 | M1.2 |
Last geomagnetic storm | 2025/04/16 | Kp8- (G4) |
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 | 120.7 -13.5 |
Last 30 days | 118.3 -22.1 |