Publié: 2013 Jul 08 1216 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 08 Jul 2013 | 122 | 004 |
| 09 Jul 2013 | 120 | 003 |
| 10 Jul 2013 | 120 | 003 |
Solar activity was eruptive during the past 24 hours with one C9.6 class flare originating from Catiana sunspot group 24 (NOAA AR 1785) on July 8 at 1h22 UT. Though this group has reduced in number of sunspots, it's photospheric magnetic field remains to have beta-gamma-delta configuration. It is capable of producing more C-class flares and maybe an M-class flare. No geo-effective CMEs were observed. We are currently under influence of a slow solar wind (speed around 300 km/s). The magnitude of the interplanetary magnetic field is low (about 5 nT). Geomagnetic conditions are quiet and are expected to remain so for the next 48 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 078, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 126 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 007 |
| Ap estimé | 007 |
| Nombre international de taches solaires estimé | 094 - Basé sur 21 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
Toutes les heures sont indiquées en UTC
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