Affichage des archives de lundi, 19 août 2024
Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC
Publié: 2024 Aug 19 1231 UTC
Prévisions SIDC
Éruptions solaires
M-class flares expected (probability >=50%)
Géomagnétisme
Quiet (A<20 and K<4)
Moniteur de Flux de Proton
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 19 Aug 2024 | 233 | 002 |
| 20 Aug 2024 | 233 | 007 |
| 21 Aug 2024 | 233 | 007 |
Régions solaires actives et éruptions solaires
Solar flaring activity was moderate over the past 24 hours. The largest flare was a M1.3-flare, with peak time 09:36 UTC on August 19, from NOAA AR 3785 (beta). There are currently 10 numbered active regions on the visible disk. NOAA AR 3784 is the most complex AR (beta-gamma-delta). The solar flaring activity is expected to be at moderate levels over the coming day with C-class flares expected and M-class flares probable and a low chance of X-class flares.
Éjection de masse coronale
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
Trous coronaux
A positive polarity low-latitude coronal hole crossed the central meridian. A high-speed stream from this coronal hole may enhance the solar wind environment near Earth on August 22.
Vent solaire
The solar wind at the Earth is slow, with speeds around 400 km/s and interplanetary magnetic field around 7nT, with the Bz reaching a minimum value of -5 nT. Slow solar wind conditions are expected to continue in the next 24h.
Géomagnétisme
Geomagnetic conditions were globally and locally quiet to active (Kp 4- and K Bel 4). Quiet conditions are expected in the next 24 hours.
Niveaux de flux de protons
Over the past 24 hours the greater than 10 MeV GOES proton flux was at background levels and is expected to remain so over the next days.
Flux d'électrons sur l'orbite géostationnaire
The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, and is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 227, sur la base de 14 stations.Indices solaires pour 18 Aug 2024
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 231 |
| AK Chambon La Forêt | 016 |
| AK Wingst | 016 |
| Ap estimé | 016 |
| Nombre international de taches solaires estimé | 209 - Basé sur 12 stations |
Résumé des événements marquants
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 18 | 2052 | 2107 | 2122 | ---- | M1.3 | --/3796 | |||
| 18 | 2346 | 0013 | S04E70 | M1.4 | SF | --/3796 | |||
| 19 | 0928 | 0936 | 0940 | S14W57 | M1.3 | SF | 50/3785 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
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La Météo Spatiale en faits
| Dernière classe X | 08/12/2025 | X1.1 |
| Dernière classe M | 31/12/2025 | M7.2 |
| Dernier orage géomagnétique | 22/12/2025 | Kp5 (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| novembre 2025 | 91.8 -22.8 |
| 30 derniers jours | 116.4 +22.7 |