Affichage des archives de dimanche, 24 juin 2018

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2018 Jun 24 1242 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 24 Jun 2018 jusqu'à 26 Jun 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
24 Jun 2018077012
25 Jun 2018077008
26 Jun 2018075005

Bulletin

The solar activity has been quiet over the past 24 hours. Catania sunspot group 86 & 88 (NOAA active region 2713 and 2715) produced few B-class flares. The magnetic complexity of Catania sunspot group 86 (NOAA active region 2715) has slightly increased (from beta to beta-delta Hale class), therefor it has a high chance of producing C-class flare with potentially, but less likely, a M-class flare.

No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.

The Earth remained under the influence of the solar wind associated with the north pole coronal hole that has passed the central meridian on the June 20. The wind speed values reached 510 km/s on June 23 around 23:30 UT, and is currently around 490 km/s. The interplanetary magnetic field has slowly converged toward its nominal condition. Currently the total magnetic field strength below 5 nT and the southward component fluctuating between -3 and +2 nT. Solar wind conditions are expected to return to the slow regime within the next two days.

The geomagnetic conditions have been unsettled to active over the past 24 hours due to the ongoing enhancement of the solar wind with K-index (Dourbes) and Kp-index (NOAA) ranging between 2 and 4. Unsettled geomagnetic conditions are expected with possible short active periods for the next day.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 024, sur la base de 22 stations.

Indices solaires pour 23 Jun 2018

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm077
AK Chambon La Forêt026
AK Wingst///
Ap estimé020
Nombre international de taches solaires estimé040 - Basé sur 28 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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