Issued: 2016 Jul 30 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
30 Jul 2016 | 071 | 011 |
31 Jul 2016 | 072 | 007 |
01 Aug 2016 | 074 | 007 |
Flaring activity has been very low, no C-class flares in past 24 h. Two simple active regions on the visible disk, Catania 13 (no NOAA number) and Catania 14 (NOAA 2570). No large flares expected (although C-class flares are possible).
Unsettled geomagnetic conditions were registered in the past 24 h, due to the vanishing effect of a high speed solar wind stream. Solar wind speed is now at 480 km/s with interplanetary magnetic field magnitude of 5 nT. Quiet to unsettled conditions are expected for the next 48 h.
Today's estimated international sunspot number (ISN): 019, based on 17 stations.
Wolf number Catania | 026 |
10cm solar flux | 071 |
AK Chambon La Forêt | 021 |
AK Wingst | 016 |
Estimated Ap | 018 |
Estimated international sunspot number | 018 - Based on 32 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
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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A southern hemisphere coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days
Active geomagnetic conditions (Kp4) Threshold Reached: 20:39 UTC
The OVATION model predicts the Hemispheric Power Index to reach 51GW at 18:18 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/05 | M1.0 |
Last geomagnetic storm | 2025/04/06 | 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 | 151.3 +17.1 |
Last 30 days | 135.2 -4.5 |