Существующий: 2019 Mar 26 1304 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 26 Mar 2019 | 071 | 010 |
| 27 Mar 2019 | 071 | 013 |
| 28 Mar 2019 | 070 | 008 |
Solar activity is low with only few B-class flares reported during last 24 hours. Since there are presently no active regions observed on the visible side of the solar disc, we expect that even number of B-class flares will decrease in the coming hours. There were no Earth directed CMEs reported during last 24 hours and the solar protons remained at the background level.
The solar wind speed is presently about 350 km/s and the interplanetary magnetic field magnitude is 7 nT. The fast solar wind associated with the negative polarity equatorial coronal hole (seemingly connected to the southern polar coronal hole), which reached central meridian yesterday afternoon, is expected at the Earth in the morning of March 29. The geomagnetic conditions are presently quiet and we expect quiet to unsettled conditions in the coming hours. The arrival of the fast solar wind, associated with the negative polarity equatorial coronal hole that is expected later today, might induce unsettled to possibly but not very probably, active geomagnetic conditions.
Today's estimated international sunspot number (ISN): 000, based on 26 stations.
| Wolf number Catania | 000 |
| 10cm solar flux | 071 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 006 |
| Estimated Ap | 004 |
| Estimated international sunspot number | 000 - Based on 33 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
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