Publié: 2014 Jan 10 1253 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Proton event in progress (>10 MeV)
| Flux de 10 cm | Ap | |
|---|---|---|
| 10 Jan 2014 | 180 | 004 |
| 11 Jan 2014 | 170 | 023 |
| 12 Jan 2014 | 160 | 014 |
The background flaring activity is close to C class level. The large active region NOAA AR 1944 is declining in size and complexity. NOAA AR 1946 is also past is stable in size. Both regions still have some flaring potential while rotating towards the west limb. The proton flux for >10MeV protons is still above the event threshold of 10 pfu, but declining. The probability for C flares is around 60%. M flares are also still possible with a likelihood of 40%. Chances for an X-flare are estimated at 5%. A shock in the solar wind data was observed on January 9 at 19:35 UTC. Solar wind speed, density and temperature showed an abrupt increase, as well as the magnitude of the interplanetary magnetic field. The solar wind speed increased from 400 to 500 km/s and then declined towards 400 km/s. The magnitude of the interplanetary magnetic field reached a maximum value of 17 nT, with a mainly positive Bz-component. Geomagnetic conditions were at most unsettled (K=3). Quiet to active levels (K=3 to 4) are expected due to the arrival of a coronal hole high speed stream on January 11.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 098, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | 164 |
| Flux solaire à 10 cm | 184 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 008 |
| Ap estimé | 009 |
| Nombre international de taches solaires estimé | 086 - Basé sur 13 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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