Affichage des archives de samedi, 3 décembre 2022

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2022 Dec 03 1235 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 03 Dec 2022 jusqu'à 05 Dec 2022
Éruptions solaires

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
03 Dec 2022128016
04 Dec 2022131012
05 Dec 2022133007

Bulletin

The solar flaring activity was at low levels. The largest flare was a C3.1 flare recorded at the northeast limb, associated with a new region (N16E85). Catania sunspot group 8 (NOAA AR 3153) is the largest region on disk but produced only low-level C-class flares in the last day. Catania sunspot group 11 (NOAA AR 3156) has now rotated onto disk and continues to produce C-class flares. Catania sunspot groups 7 and 9 (NOAA ARs 3154 and 3155) were inactive. Catania sunspot group 6 (NOAA AR 3152) decayed into a plage region. Solar flaring activity is expected to be at low levels, with C-class flares likely and a chance for M-class flares.

No Earth directed CMEs were detected in the available coronagraph imagery.

In the past 24 hours the greater than 10 MeV proton flux was below the minor-storm warning threshold and is expected to remain so. The greater than 2 MeV electron flux exceeded the 1000 pfu threshold during the last 24 hours. The electron flux is expected to continue to exceed this threshold over the next day. The 24h electron fluence was at moderate levels. The 24h electron fluence is expected to be at moderate to high levels in the next 24 hours.

The solar wind speed showed a gradually decreasing trend, decreasing from 740 km/s to values around 570 km/s. The interplanetary magnetic field magnitude ranged between 2 and 6 nT. The magnetic field orientation was predominantly in the positive sector (field directed away from the Sun). The solar wind speed is expected to continue to gradually decrease over the next 24 hours, as the influence of the high-speed stream wanes.

Geomagnetic conditions reached active levels (NOAA KP 2-3 and Local K Dourbes 2-4). Geomagnetic conditions are expected to be at unsettled levels over the next day, with isolated active periods possible particularly on Dec 03.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 088, sur la base de 05 stations.

Indices solaires pour 02 Dec 2022

Nombre de Wolf, observé par Catania085
Flux solaire à 10 cm124
AK Chambon La Forêt026
AK Wingst016
Ap estimé017
Nombre international de taches solaires estimé078 - Basé sur 11 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