Affichage des archives de dimanche, 23 juillet 2017

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2017 Jul 23 1234 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
23 Jul 2017	070	016
24 Jul 2017	070	017
25 Jul 2017	070	007

Bulletin

The only flare of the period was a B1.5 flare peaking at 7:37UT from a region turning onto the disk in the East. With no spotted regions on disk, X-ray flux is expected to remain below C level over the next days. SoHO/LASCO C2 images show a full halo CME from 4:36UT onwards. STEREO A EUVI 195 clearly shows the event from around 3:15UT originating from the backside (in relation to Earth) of the Sun. The CME will thus not influence Earth. Another CME with limited angular width of around 100 degrees directed towards the NorthWest was recorded slightly earlier from around 01:36UT onwards in SoHO/LASCO C2 images. This event is also judged to have originated from the backside of the Sun and hence will not influence Earth. No Earth directed CMEs have been observed in coronagraph data. Solar proton fluxes are at background values and are expected to remain so.

Solar wind showed the continuing influence of the coronal hole high speed stream. Solar wind speed started and ended the reporting period around 550 km/s but reached 600 km/s during the period. Total magnetic field was around the 5-7nT range but increased towards to over 9nT by the end of the period. Bz was variable with peaks down to -7nT. Over the next 2 days we should see a return to nominal Solar wind conditions. Geomagnetic conditions were quiet to unsettled (local K Dourbes 1-3, NOAA Kp 2-3). Quiet to unsettled geomagnetic conditions are expected over the next days as high speed stream effects diminish.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 22 stations.

Indices solaires pour 22 Jul 2017

Nombre de Wolf, observé par Catania	///
Flux solaire à 10 cm	070
AK Chambon La Forêt	022
AK Wingst	016
Ap estimé	017
Nombre international de taches solaires estimé	000 - Basé sur 26 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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