Issued: 2013 Apr 08 1134 UTC
Eruptive (C-class flares expected, probability >= 50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 08 Apr 2013 | 141 | 004 |
| 09 Apr 2013 | 144 | 005 |
| 10 Apr 2013 | 145 | 003 |
Three out of nine active regions reported by NOAA today have beta-gamma configuration of the photospheric magnetic field (NOAA ARs 1713, 1718, and 1719). So, despite no C-class flares today, we expect flaring activity on the C-level, with an M-class flare possible but not very likely. An eruption in the NOAA AR 1714 (Catania sunspot group 34) was detected around 02:00 UT on April 8, accompanied by a local soft X-ray flux peak at 01:44 UT at C1.1 level (no flare was reported). Coronal dimmings and a post-eruption arcade observed by SDO/AIA indicate the eruption of a CME. However, SOHO/LASCO did not detect any CME in association with this event, and STEREO coronagraphs have a data gap. Due to presumed weakness of the event (below the detectability threshold of LASCO), any geomagnetic consequences are unlikely. The Earth is currently inside a slow (around 350 km/s) solar wind flow with weak to average (3-4 nT) interplanetary magnetic field magnitude. We expect quiet geomagnetic conditions.
Today's estimated international sunspot number (ISN): 090, based on 09 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 138 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 005 |
| Estimated Ap | 005 |
| Estimated international sunspot number | 082 - Based on 21 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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