Publié: 2014 Mar 16 1228 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 16 Mar 2014 | 141 | 006 |
| 17 Mar 2014 | 141 | 018 |
| 18 Mar 2014 | 141 | 008 |
There were five C flares on the Sun during the past 24 hours, released by NOAA AR 12003, 12005, and 11998. The brightest flare was a C7.3 flare produced by AR 12003 peaking at 06:45 UT on March 16. In the next 48 hours, the probability for C flares is high (over 90%) and for M flares around 55%, mainly from AR 12003 and returning region AR 11986. CACTUS detected a CME on LASCO C2 and C3 images starting at 3:36 UT on March 16. This CME was also observed by the coronagraphs COR2 A and COR2 B, and is most probably related to the filament eruption that took place around 02:54 UT near 25S45E. This CME will probably not be geoeffective. In the past 24 hours, solar wind speed as observed by ACE varied between about 360 and 410 km/s, while the magnitude of the Interplanetary Magnetic Field (IMF) fluctuated between about 1.5 and 4.5 nT. In the past 24 hours, quiet geomagnetic levels were registered (K Dourbes between 0 and 2; NOAA Kp between 0 and 1). Quiet geomagnetic conditions (K Dourbes < 4) are expected on March 16. Quiet to active conditions (K Dourbes < 5) are possible on March 17 and 18, due to a coronal hole high speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 087, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 139 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 005 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 079 - Basé sur 17 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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