Affichage des archives de dimanche, 12 juin 2022

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2022 Jun 12 1239 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 12 Jun 2022 jusqu'à 14 Jun 2022
Éruptions solaires

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

Géomagnétisme

Quiet (A<20 and K<4)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
12 Jun 2022115013
13 Jun 2022116013
14 Jun 2022117007

Bulletin

Solar activity was low with a couple of low C flares. All those flares were from NOAA active region 3030 in the northeast. The most significant one was a long duration C1.8 flare peaking at around 8:38UT. NOAA active region 3029 has decayed into plage and footpoint spreading and decay was observed in the new region NOAA 3031. The larger bipolar region NOAA 3030 remains the most significant region on disc. Flaring at C level is expected with still a chance for an isolated M flare.

No new Earth directed CMEs have been recorded in coronagraph data.

The greater than 10 MeV proton flux was at background levels and is expected to remain so. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold. The 24h electron fluence was at normal levels and is expected to be at low to normal levels.

An equatorial positive polarity coronal hole is transiting the central meridian. It is expected to influence Solar wind near Earth from June 15 onwards.

Slow solar wind conditions were observed. Though after 8UT solar wind speed has seen an increase to around 450 km/s. The interplanetary magnetic field also became enhanced with a magnitude now reaching 15 nT. The north-south component was variable with Bz peaking down to -11nT. The phi angle now indicates connection with a positive sector (magnetic field away from the Sun). Essentially slow solar wind conditions are expected over the next days. An increase in solar wind conditions is expected by 15 June under the influence of the high speed stream from a positive polarity coronal hole.

Geomagnetic conditions were quiet to unsettled (NOAA Kp 1-2 and local K Belgium 0-3). Quiet to unsettled geomagnetic conditions are expected over the next days.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 058, sur la base de 26 stations.

Indices solaires pour 11 Jun 2022

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm112
AK Chambon La Forêt///
AK Wingst011
Ap estimé010
Nombre international de taches solaires estimé040 - Basé sur 28 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 géomagnétique21/01/2026Kp7+ (G3)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
décembre 2025124 +32.2
janvier 2026110 -14
30 derniers jours114.8 +6.7

A ce jour dans l'histoire*

Éruptions solaires
12024M3.45
21999M2.14
32024M2.11
42024M2.07
52015M2.03
DstG
11957-235G4
22004-130G3
32005-97G2
42000-91G1
52012-70G1
*depuis 1994

Les réseaux sociaux