Affichage des archives de dimanche, 3 mai 2015

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2015 May 03 1230 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 03 May 2015 jusqu'à 05 May 2015
Éruptions solaires

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

Géomagnétisme

Quiet (A<20 and K<4)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
03 May 2015110012
04 May 2015115006
05 May 2015120008

Bulletin

A couple of C1 flares were observed during the past 24 hours. The source regions were NOAA active region 2335 and a region that is currently rounding the East limb (at N10). Several CMEs were observed in SOHO/LASCO C2 and C3 images. A partial halo, with first measurement in LASCO C2 at 20:36 UT on May 2, is propagating to the East with a projected speed of 350 km/s. A second CME, with first measurement at 00:48 UT on May 3, is travelling to the SW. A third CME is seen, with first measurement at 4:00 UT on May 3, that travels in the NE direction with a projected speed of 480 km/s. The first two CMEs are associated to backsided activity and the third CME is due to an eruption at the East limb (N10). None is expected to be geo-effective. A filament near S40E35 disappeared between 15 and 18 UT (on May 2), but no eruption or associated CME has been observed as most of the material was reabsorbed when propagating to the West on the solar disk. Flaring activity is expected to increase with multiple C-class flares. Earth is inside a slow solar wind with a solar wind speed around 400 km/s. The magnitude of the Interplanetary Magnetic Field (IMF) remains below 10 nT and is even slightly decreasing. The geomagnetic conditions are quiet to unsettled (K=0 to 3 for local K at Dourbes and global estimated NOAA Kp) and are expected to continue.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 025, sur la base de 05 stations.

Indices solaires pour 02 May 2015

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm106
AK Chambon La Forêt020
AK Wingst008
Ap estimé009
Nombre international de taches solaires estimé021 - Basé sur 21 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 géomagnétique20/01/2026Kp8 (G4)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
décembre 2025124 +32.2
janvier 2026107.3 -16.8
30 derniers jours111.9 +4

A ce jour dans l'histoire*

Éruptions solaires
12026M3.4
22025M3.3
32003M2.86
42005M2.56
52000M2.06
DstG
11957-250G4
21989-107G1
32005-89G4
41972-79G2
51986-76G2
*depuis 1994

Les réseaux sociaux