Существующий: 2015 May 13 1230 UTC
Eruptive (C-class flares expected, probability >=50%)
Major magstorm expected (A>=50 or K>=6)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 13 May 2015 | 160 | 038 |
| 14 May 2015 | 158 | 038 |
| 15 May 2015 | 156 | 018 |
NOAA 2339 is decaying and produced only low-level C-class flares. NOAA 2342 produced the strongest flare of the period, a C3.5 flare peaking at 05:59UT and located in its trailing portion. The flare was associated with a series Type III radio-burst, and a surge was observed in H-alpha. The greater than 10 MeV proton flux is nearly back at nominal levels. No earth-directed coronal mass ejections (CME) were observed over the period.
Further C-class flaring is expected, with a chance on an M-class flare.
Moderate geomagnetic storming has been observed as the Earth is under the influence of the high speed stream (HSS) of a recurrent coronal hole. Kp reached 6 between 03:00 and 09:00UT, while Dourbes reported a maximum K of 4. Solar wind speed is currently at about 700 km/s, while Bz-values were at -14 nT between 04:00 and 04:30UT.
Further episodes of minor to moderate geomagnetic storming are expected.
Today's estimated international sunspot number (ISN): 121, based on 20 stations.
| Wolf number Catania | 216 |
| 10cm solar flux | 163 |
| AK Chambon La Forêt | 031 |
| AK Wingst | 016 |
| Estimated Ap | 019 |
| Estimated international sunspot number | 115 - Based on 28 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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