Issued: 2021 Mar 02 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
02 Mar 2021 | 071 | 013 |
03 Mar 2021 | 071 | 017 |
04 Mar 2021 | 071 | 010 |
Apart from a small new Alpha region that is already decaying again, the Sun is spotless, and it did not produce any C flares in the past 24 hours. The chance for a C flare in the next 24 hours is estimated at only 1%.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels in the past 24 hours; moderate values are possible in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels during the past 24 hours, and is expected to remain so in the next 24 hours.
Solar wind speed near Earth as registered by DSCOVR first decreased from about 470 km/s to about 350 km/s and then increased again to about 590 km/s, possibly related to the expected arrival of a high speed stream associated with the negative polarity southern crown coronal hole that crossed the Central Meridian on February 26. The Interplanetary Magnetic Field (IMF) was predominantly oriented towards the Sun and its magnitude varied between about 1 and 12 nT, with current values around 8 nT. Bz was not below -5 nT for extended periods. Enhanced solar wind conditions are expected in the next 24 hours.
Quiet to active conditions (K Dourbes between 1 and 4; NOAA Kp between 2 and 3) were registered in the past 24 hours. Active geomagnetic levels (K Dourbes = 4) are possible on March 2, 3 and 4, with a chance for minor geomagnetic levels (K Dourbes = 5).
Today's estimated international sunspot number (ISN): 012, based on 16 stations.
Wolf number Catania | /// |
10cm solar flux | 071 |
AK Chambon La Forêt | 024 |
AK Wingst | /// |
Estimated Ap | 028 |
Estimated international sunspot number | 010 - Based on 28 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 high possibility for aurora to appear at the following high latitude regions in the near future
ReykjavikCurrent data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future
TórshavnCurrent data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
KuopioCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
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Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:17 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 21:49 UTC
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
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 | |
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March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 129.8 -16.3 |