Affichage des archives de dimanche, 13 juin 2021

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2021 Jun 13 1231 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 13 Jun 2021 jusqu'à 15 Jun 2021
Éruptions solaires

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

Géomagnétisme

Quiet (A<20 and K<4)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
13 Jun 2021078009
14 Jun 2021076008
15 Jun 2021076010

Bulletin

There are presently only two sunspot groups observed on the visible side of the Sun, Catania sunspot group 2 and 6 (NOAA AR 2829 and 2832, respectively). Solar flaring activity is low, with only one B-class flare reported, and we expect it will stay so in the coming hours. Available observations (limited due to system maintenance) do not indicate possible presence of the Earth directed CMEs. The proton flux levels remained at background values. The greater than 2MeV electron flux is bellow the 1000 pfu threshold, and we expect it will remain so in the next 24 hours. The 24h electron fluence is at normal levels and we expect it will stay so in the coming 24 hours.

The in situ observations show the simultaneous increase of the solar wind speed, temperature and the change of the phi angle to positive value, at about 15:00 UT on June 12. The change of these solar wind characteristics was preceded by the small increase and the drop of the solar wind density. All this indicate arrival of the solar wind from the positive polarity coronal hole. However, only small equatorial unipolar region of positive polarity was observed at the central meridian on June 08 and June 09, and no prominent positive polarity coronal holes were observed. Presently the solar wind speed is about 460 km/s and the interplanetary magnetic field magnitude is about 4 nT. The solar wind originating from the large extension of the southern polar coronal hole can be expected at Earth in the early morning of June 15. During last 24 hours the geomagnetic conditions were at the quiet to unsettled We expect such geomagnetic conditions to persist in the coming hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 017, sur la base de 22 stations.

Indices solaires pour 12 Jun 2021

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm078
AK Chambon La Forêt016
AK Wingst015
Ap estimé013
Nombre international de taches solaires estimé007 - Basé sur 30 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