Существующий: 2017 Mar 25 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 25 Mar 2017 | 072 | 008 |
| 26 Mar 2017 | 072 | 024 |
| 27 Mar 2017 | 072 | 024 |
In the past 24 hours, no C flares were observed. Very low solar activity (no C flares) is expected in the next 24 hours. Over the past 24 hours, solar wind speed measured by DSCOVR decreased from about 570 to 495 km/s, while the magnitude of the Interplanetary Magnetic Field (IMF) ranged between about 1 and 5 nT. This is indicative of a transition to nominal solar wind conditions after the passage of the high speed stream from a positive coronal hole. Quiet geomagnetic conditions (K Dourbes between 1 and 2; NOAA Kp between 0 and 2) were registered in the past 24 hours. Quiet to unsettled geomagnetic conditions (K Dourbes < 4) are expected on March 25 and 26. The arrival of a high speed stream from a large, recurrent coronal hole is expected on March 27. Consequently, active geomagnetic conditions (K Dourbes = 4) are possible, with a chance for minor geomagnetic storm intervals (K Dourbes = 5).
Today's estimated international sunspot number (ISN): 016, based on 24 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 072 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 006 |
| Estimated Ap | 005 |
| Estimated international sunspot number | 013 - Based on 27 stations |
| Day | Begin | Max | Конец | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| Нет | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Все время в UTC
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