Affichage des archives de jeudi, 21 décembre 2023

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2023 Dec 21 1256 UTC

Prévisions SIDC

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
21 Dec 2023205006
22 Dec 2023205018
23 Dec 2023204022

Régions solaires actives et éruptions solaires

The solar flaring activity was at moderate level during the last 24 hours, with several C-class flares and a M-class flare. The strongest flare was GOES M4.2 flare from NOAA AR 3519 which peaked at 05:38 UTC on Dec 21. During the flare, the source region (AR 3519) of the flare had beta configuration of its photospheric magnetic field. The solar flaring activity is expected to be at low to moderate levels over the next 24 hours with few C-class flares, possibly M-class flares and a low chance for isolated X-class flares.

Éjection de masse coronale

No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph observations during last 24 hour.

Trous coronaux

A negative polarity coronal hole crossed the central meridian on Dec 20 and a high-speed stream from this coronal hole may arrive to Earth from December 22.

Vent solaire

Solar wind conditions have transitioned from fast to slow solar wind. The solar wind speed ranged between 350 km/s and 490 km/s. The North- South component (Bz) ranged between -4 and 3 nT. The interplanetary magnetic field ranged from 1 nT to 5 nT. Slow solar wind conditions are expected to continue over the next 24 hours unless the high speed streams from the negative polarity coronal hole, which started to cross the central meridian on Dec 18, impact the Earth.

Géomagnétisme

Geomagnetic conditions were globally and locally at quiet to unsettled conditions (NOAA Kp and K BEL 1 to 3) over the past 24 hours. It is expected to remain so unless the high speed streams from the negative polarity coronal hole, which started to cross the central meridian on Dec 18, impact the Earth.

Niveaux de flux de protons

The greater than 10 MeV proton flux was below the threshold level over the past 24 hours and is expected to remain so for the next 24 hours.

Flux d'électrons sur l'orbite géostationnaire

The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was just below the threshold level in the last 24 hours. It increased probably due to enhanced solar wind conditions but remained just below the 1000 pfu alert threshold level. It may increase even further and cross the threshold during the next 24 hours. The 24h electron fluence was at normal level and is expected to remain so.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 147, sur la base de 03 stations.

Indices solaires pour 20 Dec 2023

Nombre de Wolf, observé par Catania231
Flux solaire à 10 cm195
AK Chambon La Forêt014
AK Wingst011
Ap estimé012
Nombre international de taches solaires estimé160 - Basé sur 14 stations

Résumé des événements marquants

JourCommencerMaxFinLocForceOP10cmCatania/NOAATypes de sursaut radio
21051905380549S12W61M4.21N89/3519III/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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