Существующий: 2014 Feb 08 1506 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| 10cm flux | Ap | |
|---|---|---|
| 08 Feb 2014 | 175 | 025 |
| 09 Feb 2014 | 172 | 015 |
| 10 Feb 2014 | 167 | 006 |
The flaring activity of the Sun decreased significantly. The strongest flare of the past 24 hours was the C3.0 flare peaking yesterday at 14:52 UT in the Catania sunspot group 28 (NOAA AR 1967), which maintains the beta-gamma-delta configuration of its photospheric magnetic field. Catania sunspot groups 27 and 36 (NOAA ARs 1968 and 1974 respectively) have beta-gamma configuration of the photospheric magnetic field. We expect flaring activity at the C-level with isolated M-class flares. Due to position of the Catania sunspot groups 27 and 28 (NOAA ARs 1968 and 1967 respectively) in the western hemisphere, a major CME in one of them may lead to a proton event, so we maintain the warning condition. After the arrival of an interplanetary shock yesterday (16:18 UT at ACE, 16:28 UT at SOHO), the Earth is inside a post-shock solar wind flow. Currently the solar wind speed is around 450 km/s, and the interplanetary magnetic field (IMF) magnitude is around 10 nT. The north-south IMF component Bz was fluctuating, and K index reached 4 during four intervals (as reported by IZMIRAN and NOAA). The arrival of the ICME-driven shock associated with the partial halo CME first detected by SOHO/LASCO at 16:36 UT on February 4 is possible later today. Intervals of active (K = 4) or, less likely, minor storm (K = 5) conditions are expected.
Today's estimated international sunspot number (ISN): 099, based on 07 stations.
| Wolf number Catania | 122 |
| 10cm solar flux | 178 |
| AK Chambon La Forêt | 027 |
| AK Wingst | 012 |
| Estimated Ap | 011 |
| Estimated international sunspot number | 112 - Based on 15 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
<< Перейти на сегодняшнюю страницу обзора
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Последняя X-вспышка | 04/02/2026 | X4.21 |
| Последняя M-вспышка | 18/03/2026 | M2.7 |
| Последняя геомагнитная буря | 23/03/2026 | Kp5 (G1) |
| Безупречные дни | |
|---|---|
| Последние 365 дней | 3 дней |
| 2026 | 3 дней (4%) |
| Последний безупречный день | 24/02/2026 |
| Среднемесячное количество солнечных пятен | |
|---|---|
| февраля 2026 | 78.2 -34.3 |
| марта 2026 | 77.7 -0.5 |
| Последние 30 дней | 72.3 -15.7 |