Publié: 2015 May 12 1230 UTC
Eruptive (C-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 12 May 2015 | 165 | 026 |
| 13 May 2015 | 165 | 034 |
| 14 May 2015 | 163 | 024 |
NOAA 2339 produced only low-level C-class flares, mainly over its mixed polarity trailing portion. The strongest flare was a C3.0 flare peaking at 11:51UT, with radio-bursts observed at Humain. A filament erupted at the west solar limb between 02:10 and 03:00UT. It was associated with a C2.6 flare peaking at 03:02UT. Probably in response to this event, the greater than 10 MeV proton flux started to increase shortly after 04:00UT, but did not reach event threshold (10 pfu), reaching a maximum of 6.2 pfu at 07:30UT. No earth-directed coronal mass ejections (CME) were observed over the period.
Further C-class flaring is expected, with a chance on an M-class flare.
Mostly quiet to unsettled geomagnetic conditions were observed, with an active interval at Dourbes (K = 4). Starting around 05:30UT, solar wind speed gradually picked up from 340 km/s to its current value of about 380 km/s. With temperature increasing and density slightly decreasing, this may herald the anticipated arrival of the high speed stream from the negative polarity coronal hole. Bz was mostly negative throughout the period, varying between -8 and + 4 nT.
Unsettled to minor storming conditions are expected.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 121, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | 180 |
| Flux solaire à 10 cm | 163 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 016 |
| Ap estimé | 018 |
| Nombre international de taches solaires estimé | 114 - Basé sur 26 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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