Существующий: 2018 May 17 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 17 May 2018 | 070 | 024 |
| 18 May 2018 | 070 | 007 |
| 19 May 2018 | 070 | 007 |
No active regions on the visible solar disc. No C-class flares in past 24 h and the situation is not expected to change.
No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 h.
The solar wind speed at L1 is at 450 km /s with interplanetary magnetic field magnitude of 10 nT. The speed has increased about 150 km/s since yesterday, showing the first signs of the upcoming arrival of the high speed solar wind stream from a negative polarity coronal hole located in the southern hemisphere. Geomagnetic conditions have ranged from quiet to unsettled and active periods can be expected for the next 48 h (with isolated minor storm periods).
Today's estimated international sunspot number (ISN): 000, based on 27 stations.
| Wolf number Catania | 000 |
| 10cm solar flux | 070 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 004 |
| Estimated Ap | 004 |
| Estimated international sunspot number | 000 - Based on 30 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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