Существующий: 2016 Oct 30 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 30 Oct 2016 | 079 | 016 |
| 31 Oct 2016 | 081 | 013 |
| 01 Nov 2016 | 083 | 008 |
A B2 flare peaking at 23:05UT was most likely associated with an eruptive event from NOAA 2603 from behind the northwest solar limb. The related CME was not earth-directed. NOAA 2604 (Catania 50) is decaying, while old active region NOAA 2599 is rounding the southeast limb, currently as a spotless faculae area. No earth-directed coronal mass ejections (CMEs) were observed.
Quiet flaring conditions are expected to continue, with a small chance on an isolated C-class flare.
Earth remained under the influence of the high speed stream (HSS) from the huge coronal hole (CH). Solar wind speed ranged from 550 to 670 km/s (DSCOVR), and is currently hovering around 550 km/s (ACE). Bz oscillated mostly between -6 and +6 nT. The interplanetary magnetic field (IMF) was directed away from the Sun (positive). Kp ranged from unsettled to active conditions, while K Dourbes ranged from quiet to unsettled conditions.
The geo-environment is expected to remain under the gradually weakening influence of the CH HSS. Quiet to active conditions are expected.
Today's estimated international sunspot number (ISN): 013, based on 19 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 079 |
| AK Chambon La Forêt | 031 |
| AK Wingst | 022 |
| Estimated Ap | 026 |
| Estimated international sunspot number | 024 - Based on 31 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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