Affichage des archives de dimanche, 17 septembre 2017

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2017 Sep 17 1234 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 17 Sep 2017 jusqu'à 19 Sep 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
17 Sep 2017070007
18 Sep 2017069007
19 Sep 2017068007

Bulletin

The only sunspot group presently observed on the solar disk, Catania number 55 (NOAA AR 2680), is unlikely to produce flaring activity above the B-class level. No flares were reported in the past 24 hours. Newly arrived coronagraph observations show two very faint and slow partial halo CMEs (with angular width of about 180 degrees), first time observed in the SOHO/LASCO C2 field of view at 19:48 UT on September 15 and at 12:24 on September 16. The source region of both CMEs was the Catania sunspot group 46 (NOAA AR 2673) which is at the back side of the Sun as seen from the Earth. Therefore these two CMEs will not arrive to the Earth. The solar protons remained at background level in the past 24 hours.

The Earth remains to be inside the fast solar wind stream associated with a low-latitude extension of the northern polar coronal hole which reached central meridian on September 09. The solar wind speed is slowly decreasing and it presently amounts about 670 km/s. The interplanetary magnetic field magnitude is 6 nT. Due to the influence of the fast flow active geomagnetic conditions were reported in the last 24 hours (both NOAA and local station at Dourbes reported interval of Kp=4 and K=4, respectively). Presently geomagnetic conditions are quiet, however the solar wind speed is still quite high and longer intervals of southward Bz might induce unsettled to active conditions in the coming hours.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 015, sur la base de 21 stations.

Indices solaires pour 16 Sep 2017

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm072
AK Chambon La Forêt034
AK Wingst025
Ap estimé029
Nombre international de taches solaires estimé014 - Basé sur 25 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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