Существующий: 2018 Oct 05 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 05 Oct 2018 | 067 | 007 |
| 06 Oct 2018 | 066 | 007 |
| 07 Oct 2018 | 065 | 017 |
The only active region visible on the solar disc (NOAA 2723) has decayed from beta to alpha magnetic field configuration. No C-class flares in past 24 h. Solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 hours.
The solar wind speed is at 400 km/s with interplanetary magnetic fields of 2 nT. Geomagnetic conditions have been quiet. The fast solar wind associated with a positive polarity coronal hole will arrive to the Earth on October 7-8, causing disturbed geomagnetic conditions (most likely up to K = 6).
Today's estimated international sunspot number (ISN): 000, based on 26 stations.
| Wolf number Catania | 012 |
| 10cm solar flux | 067 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 005 |
| Estimated Ap | 003 |
| Estimated international sunspot number | 011 - Based on 23 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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