Affichage des archives de lundi, 29 mai 2017

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2017 May 29 1257 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 29 May 2017 jusqu'à 31 May 2017
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 cmAp
29 May 2017077006
30 May 2017074007
31 May 2017071007

Bulletin

The only region on disk (NOAA 2659, Catania group 27) produced several B flares and a couple of C flares. The strongest was a C3.3 flare peaking at 19:28UT. The region was seen to be stable or in decay and it will reach the Western limb in the next 24 hours. The region is expected to produce more B flares over the next 24 hours with a possibility for an isolated C flare, before turning over the limb. No Earth directed CMEs have been observed in coronagraph data. The proton flux levels are at background values and are expected to remain so.

Solar wind conditions showed the wake of the May 23 CME. Solar wind speed remained at levels between 340-400km/s. Total magnetic field remained at elevated levels in the 10-17 nT range with Bz turning Northward and remaining so for most of the period. Just before the end of the period Bz turned Southward again to -12nT currently. The magnetic field phi angle was indicative of magnetic field rotation due to the CME passage. A further decline of solar wind parameters should occur over the next 24 hours. Geomagnetic conditions remained at quiet to active levels (both local K Dourbes and NOAA Kp 0-4) due to the positive Bz orientation. Geomagnetic conditions are expected to be at quiet to active levels under the waning influence of the CME passage, although some minor storm levels are initially still possible, should Bz remain consistently negative over the next hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 015, sur la base de 27 stations.

Indices solaires pour 28 May 2017

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm079
AK Chambon La Forêt025
AK Wingst034
Ap estimé040
Nombre international de taches solaires estimé021 - Basé sur 32 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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