Affichage des archives de mardi, 3 janvier 2017

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2017 Jan 03 1230 UTC

Prévisions SIDC

Éruptions solaires

Quiet conditions (<50% probability of C-class flares)

Géomagnétisme

Active conditions expected (A>=20 or K=4)

Moniteur de Flux de Proton

Quiet

	Flux de 10 cm	Ap
03 Jan 2017	074	016
04 Jan 2017	074	031
05 Jan 2017	074	040

Bulletin

Solar X-ray flux has remained at background levels. The minor sunspot formations appearing yesterday have already decayed (Catania 75) or are in decay (Catania 74). No solar flares are expected in the next days. No Earth directed CME's have been recorded in coronagraph data. Solar proton flux values are at background levels and expected to remain so.

Solar wind conditions showed the expected interaction region and sector boundary crossing ahead of the negative polarity coronal hole high speed stream. Density increased steadily from 0:00UT to around 6:45UT when the magnetic field phi angle switched into the negative sector and solar wind speed (as well as temperature) started to increase from the 350-400 km/s range to the 450-500 km/s range. Over this period total magnetic field became elevated peaking around 12nT. Bz was mostly variable with the exception of a 1.5 hour negative excursion to -8.5 nT associated also with a switch back into the positive polarity sector. Solar wind speed is expected to further increase over the next days as the bulk of the high speed stream will become effective with speeds close to 700 km/s. Magnetic field values have currently somewhat recovered but could see some further enhancement over the next days. Geomagnetic conditions were quiet to active (local K Dourbes 0-4 and NOAA Kp 1-4) and are expected to remain unsettled to active with possibly minor storm levels over the next days under the influence of the core of the high speed stream.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 007, sur la base de 20 stations.

Indices solaires pour 02 Jan 2017

Nombre de Wolf, observé par Catania	023
Flux solaire à 10 cm	073
AK Chambon La Forêt	008
AK Wingst	006
Ap estimé	006
Nombre international de taches solaires estimé	000 - Basé sur 22 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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