Publié: 2016 Apr 05 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 05 Apr 2016 | 083 | 008 |
| 06 Apr 2016 | 084 | 007 |
| 07 Apr 2016 | 083 | 008 |
Over the past 24 hours solar activity has been low. The largest flare was a B4.6 class flare, produced by Active Region (AR) 2528 (Macintosh class:Bxo; Mag. type:Beta), which peaked at 07:37 UT this morning. This AR 2528 is currently the only significant region on disk with evidence of small amounts of flux cancellation in HMI magnetogram observations. There are two other ARs 2527 and AR 2526 (Hsx; Alpha), and 2526 has moved onto the West limb. No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. The solar wind speed has fluctuated between 350 to 450 km/s over the past 24 hours. The total magnetic field strength remained stable with the magnitude varying between 6 and 8 nT. The Bz component remained around 0 nT, varying between +9 and -7 nT. Geomagnetic conditions ranged between Kp index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. There is currently a small coronal hole on disk. Geomagnetic activity is expected to remain low within next 2 days.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 033, sur la base de 19 stations.
| Nombre de Wolf, observé par Catania | 045 |
| Flux solaire à 10 cm | 083 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 008 |
| Ap estimé | 006 |
| Nombre international de taches solaires estimé | 038 - Basé sur 28 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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