Affichage des archives de mardi, 8 septembre 2015

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2015 Sep 08 1243 UTC

Prévisions SIDC

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

Quiet conditions (<50% probability of C-class flares)

Géomagnétisme

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

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
08 Sep 2015084032
09 Sep 2015083008
10 Sep 2015080010

Bulletin

Only four sunspot groups are currently visible on the solar disc, and the most complex one is NOAA AR 12412 with beta configuration of its photospheric magnetic field. Only low B-class flares were reported during last 24 hours, and we expect this low solar activity to persist with possibility of only an isolated C-class flare in the coming hours. No Earth directed CMEs were observed in the last 24 hours.

Newly available data suggest that the geomagnetic storm which started yesterday afternoon and continued until early this morning, was associated with the arrival of ICME. The partial halo CME first seen at 19:24 UT on September 4 (associated with the filament eruption from the south-east quadrant of the Sun) arrived at the Earth at about 12 UT on September 07. The ACE data showed simultaneous increase of the solar wind speed from 500 km/s up to about 600 km/s, and the increase of the interplanetary magnetic field magnitude to value of about 22 nT. The Bz component of the interplanetary magnetic field had long southward intervals (down to -12nT). This rather strong southward field and the fast solar wind produced long lasting geomagnetic storm, NOAA reported Kp=6 and local stations Dourbes and Izmiran reported K=5. Currently solar wind speed is about 500 km/s and the interplanetary magnetic field magnitude is about 22 nT. During last 8 hours the Bz component of the interplanetary magnetic field was positive, however if the Bz turns negative, and with the currently rather high value of the solar wind speed, we can expect active to storm conditions in the coming hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 040, sur la base de 13 stations.

Indices solaires pour 07 Sep 2015

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm084
AK Chambon La Forêt064
AK Wingst036
Ap estimé039
Nombre international de taches solaires estimé041 - Basé sur 29 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

<< Aller à l'aperçu quotidien

Dernières nouvelles

Aidez SpaceWeatherLive.com !

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Abonnements
Donations
Aidez SpaceWeatherLive.com ! Faites un don
Soutenir SpaceWeatherLive avec nos produits dérivés
Découvrez nos produits dérivés

La Météo Spatiale en faits

Dernière classe X18/01/2026X1.9
Dernière classe M21/01/2026M3.4
Dernier orage géomagnétique22/01/2026Kp5+ (G1)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
décembre 2025124 +32.2
janvier 2026118.7 -5.3
30 derniers jours120.4 +5.6

A ce jour dans l'histoire*

Éruptions solaires
12014M7.04
22014M5.27
32014M5.01
42014M3.79
52001M2.27
DstG
11985-125G2
21971-97G2
31972-56G1
41980-55G1
51982-47
*depuis 1994

Les réseaux sociaux