Affichage des archives de dimanche, 8 décembre 2013

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2013 Dec 08 1250 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 08 Dec 2013 jusqu'à 10 Dec 2013
Éruptions solaires

Eruptive (C-class flares expected, probability >=50%)

Géomagnétisme

Active conditions expected (A>=20 or K=4)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
08 Dec 2013157024
09 Dec 2013157008
10 Dec 2013157014

Bulletin

The X-ray curve is situated near the top/bottom of the B/C-level. C-flares are very likely, the probability for M-flares is around 20%. The December 7 M1.2 flare (07:29UT peak time) from NOAA AR 1909 was associated with a CME. CACTus determined it as a (partial) halo CME with a speed around 900 km/s. The bulk of the plasma is ejected under the ecliptic plane. The side of the CME may impact the Earth. This glancing blow can possibly arrive late December 9, early December 10 and may result in geomagnetic disturbances. Late December 7, a co-rotating interaction region (CIR) arrived. The density increased gradually together with the magnetic field. The z-component fluctuated strongly, even to -25nT which resulted in a planetary K of 6 and 5 and local K Dourbes of 5 and 4 early December 8. Following the density increase and slow decrease, the solar wind speed increased gradually. The CIR and fast solar wind is possibly linked with the coronal hole which reached the central meridian on December 3. A shock is visible on ACE data on December 8, 7:30UT: the solar wind speed increased from 500 km/s to around 650 km/s, the temperature, density and magnetic field dropped. This fast reverse shock is possibly linked with the filament eruption of December 5. The geomagnetic impact will be limited and smaller compared to the CIR because of the drop in magnetic field strength. Bz rotated from negative (-5nTEstimation du nombre international de taches solaires (ISN) pour aujourd'hui : 065, sur la base de 10 stations.

Indices solaires pour 07 Dec 2013

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm157
AK Chambon La Forêt026
AK Wingst008
Ap estimé007
Nombre international de taches solaires estimé062 - Basé sur 14 stations

Résumé des événements marquants

JourCommencerMaxFinLocForceOP10cmCatania/NOAATypes 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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