Affichage des archives de dimanche, 8 mars 2015

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2015 Mar 08 1230 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 08 Mar 2015 jusqu'à 10 Mar 2015
Éruptions solaires

Active (M-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 Mar 2015144016
09 Mar 2015147018
10 Mar 2015150018

Bulletin

NOAA 2297 produced several C-class flares and one M-class event, an M9.2 flare peaking at 22:22UT (07 March). An associated type II radio burst (shock speed of 704 km/s) was observed, while the proton flux remained at nominal levels. The related partial halo coronal mass ejection (CME) was first seen by CACTus at 22:24UT, had a width of about 230 degrees and a plane-of-the-sky speed of 672 km/s. The bulk of the CME is directed to the east and south of the ecliptic, however a glancing blow of the CME impacting on 10 March around noon (+/- 12 hours) can currently not be excluded. Minimal geomagnetic effects are expected. NOAA 2297 is a compact and magnetically complex region that has still all the potential to produce strong flares over the next few days. Associated CMEs may become more geo- effective as the region rotates further onto the disk. M-class flaring is expected, with a good chance on an X-class flare. Quiet to active geomagnetic conditions were observed. Solar wind speed has slightly increased over the period, being mostly between 500 and 600 km/s. Bz oscillated between -6 and +7 nT. The interplanetary magnetic field was mostly directed away from the Sun. A negative polarity equatorial coronal hole (CH) will reach the central meridian on 09 March. Quiet to active geomagnetic conditions are expected, under the continued influence of the high speed stream from an extended coronal hole.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 022, sur la base de 21 stations.

Indices solaires pour 07 Mar 2015

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm138
AK Chambon La Forêt034
AK Wingst022
Ap estimé024
Nombre international de taches solaires estimé012 - Basé sur 21 stations

Résumé des événements marquants

07 2145 2222 2258 ////// M9.2 260 ///2297 II/1IV/2
JourCommencerMaxFinLocForceOP10cmCatania/NOAATypes de sursaut radio

Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive

Toutes les heures sont indiquées en UTC

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