Affichage des archives de lundi, 18 septembre 2023

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2023 Sep 18 1231 UTC

Prévisions SIDC

Éruptions solaires

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

Géomagnétisme

Moderate (ISES: Major) magstorm expected (A>=50 or K=6)

Moniteur de Flux de Proton

Quiet

Flux de 10 cmAp
18 Sep 2023138011
19 Sep 2023138037
20 Sep 2023138007

Régions solaires actives et éruptions solaires

There are six active regions visible on the disk. Only minor C-class flaring was observed in the last 24 hours. The active regions have simple alpha or beta magnetic field configuration. More C-class flaring is expected.

Éjection de masse coronale

A partial halo CME was detected by LASCO/C2 at 13:25 UTC on 17 September. The source region of the CME is close to the SW limb, there are low chances of seeing a glancing blow at the Earth, or a shock at most, on 21 September.

Trous coronaux

The fast solar wind from two small coronal holes may affect the Earth in the next 24-48 hours. One of them has positive polarity and is located in the southern hemisphere (close to the equator), the second one has negative polarity and is located in the northern hemisphere.

Vent solaire

The solar wind data at Earth shows the arrival of an ICME, corresponding to the CME on 14 September. The interplanetary magnetic field reached 11 nT with Bz down to -7 nT and solar wind speeds around 430 km/s. Although the effects of this ICME are anticipated to diminish within the next 24 hours, another ICME event, corresponding to the CME from 16 September, is predicted to impact Earth on 19 September, potentially with greater intensity.

Géomagnétisme

During the last 24 hours the geomagnetic conditions have reached minor storm levels globally (Kp 5) and unsettled locally (K_Bel 3), due to the ICME arrival (from the CME on 14 September). Moderate storm levels (and up to major storm levels) can be expected when the ICME corresponding to the 16 September CME arrives to the Earth in about 24 hours.

Niveaux de flux de protons

Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next 24 hours.

Flux d'électrons sur l'orbite géostationnaire

The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain so in t

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 125, sur la base de 14 stations.

Indices solaires pour 17 Sep 2023

Nombre de Wolf, observé par Catania///
Flux solaire à 10 cm145
AK Chambon La Forêt029
AK Wingst016
Ap estimé017
Nombre international de taches solaires estimé097 - Basé sur 17 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

<< Aller à l'aperçu quotidien

Dernières nouvelles

Aidez SpaceWeatherLive.com !

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Abonnements
Donations
Aidez SpaceWeatherLive.com ! Faites un don
Soutenir SpaceWeatherLive avec nos produits dérivés
Découvrez nos produits dérivés

La Météo Spatiale en faits

Dernière classe X08/12/2025X1.1
Dernière classe M27/12/2025M5.1
Dernier orage géomagnétique22/12/2025Kp5 (G1)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
novembre 202591.8 -22.8
décembre 2025115.5 +23.7
30 derniers jours113.8 +28

A ce jour dans l'histoire*

Éruptions solaires
12001X4.99
22001M6.83
31999M6.5
42024M4.5
51998M4.47
DstG
11992-96G2
21960-85G1
31991-74G1
41959-60G1
51985-59G1
*depuis 1994

Les réseaux sociaux