Affichage des archives de dimanche, 31 juillet 2022

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2022 Jul 31 1231 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 31 Jul 2022 jusqu'à 02 Aug 2022
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 cmAp
31 Jul 2022092019
01 Aug 2022092025
02 Aug 2022092007

Bulletin

X-ray flux remained below C class level. The unipolar NOAA active region 3062 remained stable as it is approaching the west limb while the bipolar NOAA active region 3068 has somewhat consolidated. Flaring at C level is not very likely but remains possible over the next days.

No Earth directed CMEs have been identified in coronagraph data.

The greater than 10 MeV proton flux was at background levels and is expected to remain so. The greater than 2 MeV electron flux just briefly touched the 1000 pfu alert threshold. The 24h electron fluence was at normal levels and is expected to be at normal levels.

An extension of the (negative polarity) south polar coronal hole has started to cross the central meridian. It may influence near-Earth Solar wind conditions around July 3.

Essentially slow Solar wind conditions were observed. Solar wind speed was in the 320-390km/s range. The interplanetary magnetic field has become enhanced though, reaching 13nT currently with a variable north-south component. This could possibly be associated to the compression region ahead of the (later than) expected high speed stream. The interplanetary magnetic field is still connected to a negative sector (field towards the Sun). We are still expecting today a switch into the positive sector (field away from the Sun), followed by an increase in Solar wind speed associated to the high speed stream from the isolated coronal hole that crossed the central meridian on July 26. As this feature is later than expected, the wind speed is not expected to reach far over 500 km/s.

Geomagnetic conditions were quiet to unsettled (NOAA Kp and local K Dourbes 1-3). Active conditions are expected over the next days associated to the interaction region and high speed stream from the isolated coronal hole that crossed the central meridian on July 26.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 036, sur la base de 21 stations.

Indices solaires pour 30 Jul 2022

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm091
AK Chambon La Forêt012
AK Wingst010
Ap estimé008
Nombre international de taches solaires estimé046 - 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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