Affichage des archives de dimanche, 4 mars 2018

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2018 Mar 04 1330 UTC

Prévisions SIDC

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 cm	Ap
04 Mar 2018	067	007
05 Mar 2018	067	008
06 Mar 2018	066	007

Bulletin

Solar activity is very low with only one B-class flare reported during last 24 hours. Catania sunspot group 73 (NOAA AR 2007) has rotated behind the west solar limb and there are presently no numbered active regions on the visible side of the solar disc. We expect low solar activity to continue in the coming hours with very low probability of flaring, even on the B-class level. Coronagraph images do not show signatures of the Earth directed CMEs, and the solar protons remained at the background level.

The solar wind speed is presently about 370 km/s and the interplanetary magnetic field magnitude is 3 nT. The increase of the solar wind speed (up to 460 km/s), interplanetary magnetic field (up to 10 nT) and temperature, simultaneously with decrease of density observed during last 24 hours are probably associated with the equatorial coronal hole, which reached central meridian in the morning of February 26. The geomagnetic conditions are presently quiet and we expect quiet to unsettled geomagnetic conditions in the coming hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 24 stations.

Indices solaires pour 03 Mar 2018

Nombre de Wolf, observé par Catania	///
Flux solaire à 10 cm	068
AK Chambon La Forêt	013
AK Wingst	006
Ap estimé	006
Nombre international de taches solaires estimé	000 - Basé sur 24 stations

Résumé des événements marquants

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

Toutes les heures sont indiquées en UTC

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