Publié: 2013 May 12 1221 UTC
Active (M-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 12 May 2013 | 142 | 011 |
| 13 May 2013 | 142 | 010 |
| 14 May 2013 | 139 | 007 |
Solar activity has been eruptive during the past 24 hours, featuring eighteen C flares. The largest flare was released by NOAA AR 11746 and reached a C8.0 peak around 19:48 UT on May 11. More C flares and even M flares are likely within the next 48 hours, especially from NOAA AR 11744, 11745, and 11746. A large filament eruption took place near 40W 35N around 21:45 UT on May 11. An associated CME was registered by LASCO C2, STEREO COR2 A and B. A glancing blow from this CME is possible, with an expected arrival time at Earth in the first half of May 15. In the last 24 hours, the IMF has varied between 2.5 and 3.5 nT, while solar wind speeds have decreased from about 400 and to 360 km/s. In the second half of May 12, a weak coronal hole high speed stream may cause solar wind speeds to increase again up to 500 km/s. Geomagnetic activity has been at quiet levels (K Dourbes between 0 and 3; NOAA Kp between 1 and 2) during the past 24 hours. Quiet geomagnetic conditions (K Dourbes < 4) are expected for May 12 to 14, with a chance for active levels (K Dourbes = 4) in the second half of May 12, due to a weak coronal hole high speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 094, sur la base de 06 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 137 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 004 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 089 - Basé sur 17 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Types de sursaut radio | Catania/NOAA | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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| Jours sans taches solaires | |
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