Publié: 2014 Oct 22 1246 UTC
Major flares expected (X-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 22 Oct 2014 | 204 | 011 |
| 23 Oct 2014 | 208 | 011 |
| 24 Oct 2014 | 210 | 011 |
Three M-class flares were detected in the past 24 hours, all of them produced by the Catania sunspot group 88 (NOAA AR 2192). The strongest flare was the M8.7 flare peaking at 01:59 UT. Based on the still incomplete SOHO/LASCO data and the absence of conspicuous eruptive signatures in the SDO/AIA data, we conclude that there was no CME associated with this flare. We expect flaring activity mostly on the M-level in this group, with a good chance for an X-class flare. As the Catania sunspot group 88 approaches the solar central meridian, a major eruption in this active region may lead to a geoeffective CME and a proton event. The Earth is currently inside a slow (around 460 km/s) solar wind flow with average (around 5 nT) interplanetary magnetic field magnitude. The geomagnetic conditions are quiet and are expected to remain so.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 095, sur la base de 10 stations.
| Nombre de Wolf, observé par Catania | 151 |
| Flux solaire à 10 cm | 199 |
| AK Chambon La Forêt | 028 |
| AK Wingst | 017 |
| Ap estimé | 017 |
| Nombre international de taches solaires estimé | 082 - Basé sur 16 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 21 | 1335 | 1338 | 1340 | ---- | M1.2 | 510 | --/---- | III/2II/2 | |
| 22 | 0116 | 0159 | 0228 | ---- | M8.7 | 580 | 88/2192 | IV/1 | |
| 22 | 0511 | 0517 | 0521 | ---- | M2.7 | 88/2192 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
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