Issued: 2015 Aug 04 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
04 Aug 2015 | 110 | 008 |
05 Aug 2015 | 115 | 007 |
06 Aug 2015 | 120 | 006 |
Solar activity was very low with flaring restricted to B-class flares. All regions have a simple configuration (alpha or beta). NOAA active region 2396 showed some fast growth. A backsided filament eruption was followed by a slow, small CME with first measurement in LASCO-C2 at 13:25 UT. No Earth-directed CMEs were observed. Chances for strong flares remain low.
The solar wind speed has gradually decreased to 440 km/s. Geomagnetic conditions were mainly quiet and are expected to remain so.
Today's estimated international sunspot number (ISN): 082, based on 17 stations.
Wolf number Catania | /// |
10cm solar flux | 106 |
AK Chambon La Forêt | 011 |
AK Wingst | 009 |
Estimated Ap | 008 |
Estimated international sunspot number | 052 - Based on 35 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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Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC
The OVATION model predicts the Hemispheric Power Index to reach 76GW at 08:57 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 01:45 UTC
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 00:44 UTC
Moderate M1.57 flare
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/08 | M1.5 |
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 | 144.7 +10.5 |
Last 30 days | 138.4 +2.2 |