Существующий: 2015 May 16 1230 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 16 May 2015 | 132 | 007 |
| 17 May 2015 | 127 | 016 |
| 18 May 2015 | 122 | 021 |
NOAA 2339 and 2342 produced a C2 class flare each. No other flaring events were observed. A large filament in the northeast quadrant erupted shortly before midnight. No obvious x-ray signature was associated with this event. No earth-directed coronal mass ejections (CMEs) have been observed.
Further C-class flaring is expected, with a slight chance on an M-class flare.
Solar wind speed declined further from 530 km/s to its current value of about 430 km/s. Bz varied between -4 and +2 nT. Quiet to unsettled geomagnetic conditions were observed. A recurrent positive polarity coronal hole (CH) has completed its central meridian transit.
The arrival of the 13 May CME and the high speed stream from the aforementioned CH are expected for late 17 or 18 May. This may result in active conditions, with a minor storming episode not excluded. Until then, quiet to unsettled geomagnetic conditions are expected.
Today's estimated international sunspot number (ISN): 069, based on 07 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 137 |
| AK Chambon La Forêt | 011 |
| AK Wingst | 008 |
| Estimated Ap | 009 |
| Estimated international sunspot number | 089 - Based on 26 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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