Affichage des archives de jeudi, 9 février 2023

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2023 Feb 09 1236 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 09 Feb 2023 jusqu'à 11 Feb 2023
Éruptions solaires

M-class flares expected (probability >=50%)

Géomagnétisme

Quiet (A<20 and K<4)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
09 Feb 2023205013
10 Feb 2023205006
11 Feb 2023200005

Bulletin

The level of the solar flaring activity has stayed moderate over the past 24 hours. A total of 17 flares have been reported, of which 7 were M-class flares and 10 were C-class flares. All of the M-class flaring activity originated from NOAA AR3213 and NOAA AR3217. NOAA AR 3213 has now fully crossed the central meridian and has evolved into a beta-gamma-delta photospheric magnetic field configuration. NOAA AR3217 just rotated onto the visible side of the solar disk. The strongest flare reported was a M3.1 flare originating from NOAA AR3213 with peak time 03:10UT on February 9. We expect solar flaring activity to remain at moderate levels over the next 24 hours, with M-class flares expected and with a small possibility of X-class flares.

During the last 24 hours there were no potentially Earth-directed coronal mass ejections detected in the available coronagraph observations.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours. The greater than 2 MeV electron flux reached the 1000 pfu threshold for a short period over the past 24 hours. It is expected to remain below the 1000 pfu threshold over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so over the next 24 hours.

The solar wind parameters of the last 24 hours still reflect conditions of the high speed stream that arrived on the 6th of February. The solar wind speed has been gradually declining from about 590 km/s to 520 km/s. The magnitude of the interplanetary magnetic field was around 5nT. We expect to see a continuation of the decline in the solar wind speed as we are returning towards slow solar wind conditions in the next 24 hours.

During the last 24 hours, the geomagnetic conditions were unsettled (K-Bel=2-4 NOAA-Kp=2-4). Geomagnetic conditions are expected to be quiet to unsettled in the next days.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 155, sur la base de 13 stations.

Indices solaires pour 08 Feb 2023

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm192
AK Chambon La Forêt028
AK Wingst018
Ap estimé020
Nombre international de taches solaires estimé140 - Basé sur 23 stations

Résumé des événements marquants

JourCommencerMaxFinLocForceOP10cmCatania/NOAATypes de sursaut radio
08024502530257----M2.0--/3213
08152816031626N31W05M1.62N--/3213III/2
08195620122046S09E72M1.51N--/3217
08210321132121N30W10M1.71F--/3213III/1VI/1
09024503100328S02E70M3.01F--/3213
09071107170721S02E70M1.1SF--/3217III/2
09084909070924----M2.8--/----IV/1III/1

Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive

Toutes les heures sont indiquées en UTC

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