Issued: 2015 Feb 04 1231 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
04 Feb 2015 | 149 | 007 |
05 Feb 2015 | 149 | 007 |
06 Feb 2015 | 149 | 007 |
Solar activity was moderate with NOAA AR 2277 (Catania 78, 79) producing an M1.2 flare peaking at 02:15UT. Apart from that, only some minor C flares were detected, mostly from NOAA 2277 (Catania 78, 79), but also from Catania 82 (NOAA 2280). NOAA region 2277 continues to carry opposite polarity field is its intermediate region. A new region rotated onto disc in the northern hemisphere and is numbered NOAA 2281. We expect C flaring for the coming days, especially from NOAA region 2277 with also a chance for an M flare. There is a slight chance for a proton event should 2277 produce significant flaring. A filament eruption occurred at 10N35E at 12:00 UT February 3. The associated CME was directed northeast and narrow. SoHA LASCO C2 showed two westbound CME's respectively souhwest from 3:12 UT onwards and northwest from 5:24 onwards. Both are judged to be originating from on or behind the west limb. No Earth directed CMEs were recorded. Solar wind conditions have been recovering from the influence of a high speed stream. solar wind speed has dropped continuously from around 580 km/s to about 470 km/s. Total magnetic field was roughly in the 2.5 to 4 nT range. with Bz variable but predominantly negative. The geomagnetic conditions were quiet to unsettled (NOAA Kp and local K Dourbes 2-3). A further decrease to nominal solar wind conditions is expected with associated and quiet to unsettled geomagnetic conditions over the next days.
Today's estimated international sunspot number (ISN): 074, based on 14 stations.
Wolf number Catania | 123 |
10cm solar flux | 149 |
AK Chambon La Forêt | 017 |
AK Wingst | 017 |
Estimated Ap | 017 |
Estimated international sunspot number | 062 - Based on 17 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
04 | 0208 | 0215 | 0221 | N10W14 | M1.2 | 2N | 78/2277 | III/1 |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
Current data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future
Norilsk, VorkutaCurrent data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
ArkhangelskCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
Surgut, SyktyvkarA lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 13:07 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 13:21 UTC
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 | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 130.4 -16.1 |