Affichage des archives de mardi, 28 juin 2022

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2022 Jun 28 1254 UTC

Prévisions SIDC

Éruptions solaires

C-class flares expected, (probability >=50%)

Géomagnétisme

Quiet (A<20 and K<4)

Moniteur de Flux de Proton

Quiet

	Flux de 10 cm	Ap
28 Jun 2022	098	008
29 Jun 2022	100	008
30 Jun 2022	101	004

Bulletin

Solar flaring activity over the past 24 hours reached low levels with a single C-class flare - an impulsive C1.4-class flare with peak time 18:43 UTC on June 27th from NOAA AR 3040 (beta), which has grown slightly and crossed the central meridian. Active region NOAA 3038 (beta) has rotated behind the northwest limb and a new active region NOAA AR 3041 (beta) has appeared on the disc in the north-west quadrant. It has remained inactive. A few other simple unnumbered active regions are visible on the solar disc, but have been inactive as well. The X-ray flaring activity over the next 24 hours is expected to be at very low to low levels with chances for isolated C-class flaring.

No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery over the past 24 hours.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was mostly above the 1000 pfu threshold and is expected to remain so over the next 24 hours. The 24h electron fluence was at moderate levels and is expected to remain so over the next 24 hours.

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) were under the waning influence of a high speed stream. The solar wind velocity has fluctuated in between 580 km/s and 480 km/s at present. The interplanetary magnetic field was weak with a maximal value of 7 nT and a minimum Bz of -5 nT. The B field remained predominantly in the negative sector. The solar wind parameters are continue to return towards background slow solar wind conditions over the next 24 hours.

The geomagnetic conditions over the past 24 hours were mostly quiet with isolated unsettled periods. Mostly quiet geomagnetic conditions are expected over the next 24 hours with isolated unsettled periods and remaining minor chances for an isolated active period.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 073, sur la base de 14 stations.

Indices solaires pour 27 Jun 2022

Nombre de Wolf, observé par Catania	058
Flux solaire à 10 cm	098
AK Chambon La Forêt	012
AK Wingst	010
Ap estimé	014
Nombre international de taches solaires estimé	056 - Basé sur 27 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

<< Aller à l'aperçu quotidien