Affichage des archives de lundi, 27 septembre 2021

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2021 Sep 27 1231 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 27 Sep 2021 jusqu'à 29 Sep 2021
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
27 Sep 2021086007
28 Sep 2021086007
29 Sep 2021086007

Bulletin

Four active regions (ARs) present on the visible solar disk. No flares above the B-class level in the past 24 hours. Over the next 24 hours, C-class flares can be expected, in particular from NOAA AR 2871 which has a beta-gamma magnetic field configuration (the other 3 ARs have a beta magnetic field configuration).

No Earth directed CMEs have been observed in coronagraph data in the last 24 hours.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay there in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold. Over the next 24 hours, it is expected to remain below the threshold. The electron fluence was at normal levels over the past 24 hours, and is expected to remain so for the next 24 hours.

Over the past 24 hours the solar wind speed has been around 400 km/s. The total magnetic field strength had reached 11 nT, while its Bz component reached -6 nT. This slightly elevated magnetic field, together with low temperature plasma, could mark the expected arrival of the ICMEs from 23 and 24 September. Due to the low speeds and mostly positive Bz, the effect is very mild, the situation may change in the coming hours since more than one ICME was expected.

Geomagnetic conditions were quiet to unsettled (NOAA Kp and K Dourbes 1-3) over the past 24 hours. Active periods can be expected over the next 24 hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 049, sur la base de 10 stations.

Indices solaires pour 26 Sep 2021

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm086
AK Chambon La Forêt006
AK Wingst002
Ap estimé001
Nombre international de taches solaires estimé048 - Basé sur 26 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

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