Существующий: 2016 Apr 11 1230 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 11 Apr 2016 | 111 | 005 |
| 12 Apr 2016 | 111 | 011 |
| 13 Apr 2016 | 111 | 031 |
One C flare was released by the Sun in the past 24 hours: a C1.1 flare produced by beta region NOAA AR 2529, peaking at 02:02 UT on April 11. More C flares (probability 70%) are expected in the next 24 hours, with a slight chance (probability 10%) for an M flare, especially from AR 2529. A filament eruption centered near 10N25E was observed around 10:13 UT on April 10 and an associated CME was first observed by LASCO C2 at 11:48 UT. This CME may deliver a glancing blow on April 14. Solar wind speed varied between about 335 and 430 km/s in the past 24 hours, while the magnitude of the Interplanetary Magnetic Field ranged between 1 and 10 nT. Over the past 24 hours, geomagnetic conditions have been quiet to unsettled (K Dourbes between 1 and 3; NOAA Kp between 1 and 3). Quiet to unsettled geomagnetic levels (K Dourbes < 4) are expected on April 11 and most of April 12. Late on April 12, and on April 13, the expected arrival of a high speed stream associated with a negative equatorial coronal hole may cause active (K Dourbes = 4) to moderate storm (K Dourbes = 6) conditions.
Today's estimated international sunspot number (ISN): 040, based on 22 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 111 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 007 |
| Estimated Ap | 007 |
| Estimated international sunspot number | 028 - 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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