Affichage des archives de jeudi, 14 mai 2015

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2015 May 14 1230 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 14 May 2015 jusqu'à 16 May 2015
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
14 May 2015153014
15 May 2015150015
16 May 2015148015

Bulletin

The eruption of a filament near NOAA 2345 was accompanied by the strongest flaring event of the period, a C9.2 flare peaking on 13 May at 18:18UT. Coronagraphic imagery indicates that the bulk of the coronal mass ejection (CME) was directed to the north and away from Earth. However, difference imagery (CACTus) shows the faint outline of an asymmetric halo CME having a plane-of-the-sky speed of about 240 km/s. Provided this is not from a backside event, an impact from the shock is possible on 18 May, but the geomagnetic effects are expected to be limited. NOAA 2339 produced 2 low-level C-class flares near its leading sunspots, while the other regions were quiet. The other observed CMEs had no earth-directed component.

Further C-class flaring is expected, with a chance on an M-class flare.

Solar wind speed slowly undulated around 700 km/s as a result of the high speed stream (HSS) from the recurrent coronal hole. Bz-values were small and varied mostly between -6 and +4 nT. Only quiet to active geomagnetic conditions were observed.

Quiet to active geomagnetic conditions are expected to persist, with a chance on a minor storming episode.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 121, sur la base de 21 stations.

Indices solaires pour 13 May 2015

Nombre de Wolf, observé par Catania200
Flux solaire à 10 cm157
AK Chambon La Forêt037
AK Wingst040
Ap estimé042
Nombre international de taches solaires estimé122 - Basé sur 26 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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