Issued: 2015 Nov 25 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 25 Nov 2015 | 115 | 018 |
| 26 Nov 2015 | 117 | 021 |
| 27 Nov 2015 | 119 | 015 |
In the past 24 hours, beta region NOAA AR 2454 produced one C1.9 flare which peaked around 8:26 UT on November 25. C flares are expected within the next 24 hours, with a 10% chance for an M flare. STEREO COR2 A first observed a bright CME in its East to Southeast direction at 8:54 UT on November 25. LASCO data are not yet available. This CME is most probably associated with the C1.9 flare of 8:26 UT. Awaiting LASCO imagery, and in view of the location of the flare near the West limb, this CME is not expected to be Earthbound. The Earth is currently within a slow solar wind region regime. Solar wind speed varied between 260 and 360 km/s in the past 24 hours, while the magnitude of the Interplanetary Magnetic Field ranged between 2 and 5 nT. Over the past 24 hours, geomagnetic conditions have been quiet (K Dourbes between 0 and 2; NOAA Kp between 0 and 1). The expected arrival of a coronal hole high speed stream may cause active (K Dourbes = 4) geomagnetic levels on November 25, 26 and 27, with a slight chance for minor storm intervals (K Dourbes = 5).
Today's estimated international sunspot number (ISN): 060, based on 10 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 113 |
| AK Chambon La Forêt | 002 |
| AK Wingst | 000 |
| Estimated Ap | 001 |
| Estimated international sunspot number | 062 - Based on 16 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
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