Publié: 2014 May 23 1241 UTC
Eruptive (C-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 23 May 2014 | 113 | 021 |
| 24 May 2014 | 116 | 013 |
| 25 May 2014 | 116 | 007 |
There were four low C flares during the past 24 hours. The brightest one was a C1.5 flare released by NOAA AR 12065 with peak time at 04:58 UT on May 23. No new CMEs were observed. In the next 48 hours, the probability for C flares is high (85%, from NOAA AR 12071, 12072, 12073, 12065, and 12066) and for M flares around 25%, especially from NOAA AR 12071 and 12065. Over the last 24 hours, the solar wind speed as observed by ACE was around 350 km/s until it suddenly jumped to about 500 km/s around 3h30 UT on May 23. This was probably due to the arrival of a coronal hole high speed stream. Meanwhile the magnitude of the Interplanetary Magnetic Field (IMF) had increased from 5 nT to about 12 nT. Over the past 24 hours, geomagnetic conditions were quiet (K Dourbes between 1 and 3; NOAA Kp between 1 and 3) due to the IMF's positive Bz angle. As an effect of the high speed stream, quiet geomagnetic levels (K Dourbes < 4) with active (K Dourbes = 4) to minor storm (K Dourbes = 5) periods are expected on May 23 and 24. Quiet conditions are expected on May 25.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 058, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 111 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 013 |
| Ap estimé | 012 |
| Nombre international de taches solaires estimé | 047 - Basé sur 22 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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