Issued: 2013 May 09 1220 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
09 May 2013 | 127 | 007 |
10 May 2013 | 127 | 007 |
11 May 2013 | 128 | 007 |
Flaring activity remains at low level. A C3.4 flare peaked at 05:23 UT in NOAA AR 1734 (Cat 59). More C-class flaring can be expected in the coming days, with a slight chance for an M-flare. Two filament eruptions are visible in AIA 304 data around 05:20 UT, one to the north and one to the south. Several CMEs were observed in coronagraph data, but none are earth- directed. Geomagnetic conditions remain quiet. The solar wind speed remains elevated (around 500 km/s) due to the influence of a coronal hole.
Today's estimated international sunspot number (ISN): 078, based on 11 stations.
Wolf number Catania | /// |
10cm solar flux | 127 |
AK Chambon La Forêt | 012 |
AK Wingst | 009 |
Estimated Ap | 008 |
Estimated international sunspot number | 082 - Based on 18 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
---|---|---|---|---|---|---|---|---|---|---|
None |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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 04:56 UTC
Active geomagnetic conditions (Kp4) Threshold Reached: 01:32 UTC
Moderate M2.5 flare
Minor R1 radio blackout in progress (≥M1 - current: M1.45)
Begin Time: 01/04/2025 06:45 UTC Maximum Time: 01/04/2025 06:45 UTC Duration: 1 minutes. Peak flux: 190 sfu
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 | |
---|---|
February 2025 | 154.6 +17.6 |
April 2025 | 152.5 -2.1 |
Last 30 days | 130.7 -17.9 |