Affichage des archives de lundi, 12 février 2018

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2018 Feb 12 1304 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 12 Feb 2018 jusqu'à 14 Feb 2018
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
12 Feb 2018077012
13 Feb 2018078012
14 Feb 2018077005

Bulletin

Over the past 24 hours solar activity has been low. The largest flare was a C1.5 class flare. Active Region (AR) 2699 (Mcintosh class:Dai; Mag. type:Beta) has been most active, showing considerable flux emergence and cancellation, producing the C1.5-class flare, which peaked at 01:35 UT this morning (12-feb-2018). The greater than 10MeV proton flux remained at background levels over the past 24 hours. Observations of coronal dimmings and EUV waves from EUV imagery yesterday at 20:40 UT (11-Feb-2018) and today at 01:41 UT suggests AR 2699 produced a couple of eruptions. Coronagraph imagery is currently unavailable to estimate the extent of any associated CMEs, and estimate a possible arrival time, but the source region is located near disk centre and any associated eruption may interact with the Earth. AR 2699 is expected to produce further flares and eruptions. The solar wind speed has increased from around 300 to 325 km/s over the past 24 hours. The total magnetic field strength has remained around 5 nT. The Bz component was largely positive, fluctuating between -5 and +5 nT. Geomagnetic conditions ranged between Kp index 0-2 (NOAA) and local K index 0-3 (Dourbes) over the past 24 hours. A small positive polarity coronal hole passed the central meridian a couple of days ago and may enhance solar wind speeds over the coming days. Evidence of a small eruption that occurred near disk centre this morning may indicate an eruption will enhance geomagnetic conditions in a few days. Geomagnetic conditions are expected to be quiet to unsettled.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 027, sur la base de 19 stations.

Indices solaires pour 11 Feb 2018

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm078
AK Chambon La Forêt005
AK Wingst002
Ap estimé001
Nombre international de taches solaires estimé030 - Basé sur 18 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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