Publié: 2024 Sep 29 1232 UTC
M-class flares expected (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 29 Sep 2024 | 195 | 019 |
| 30 Sep 2024 | 197 | 017 |
| 01 Oct 2024 | 199 | 007 |
Solar flaring activity was low over the past 24 hours. A total of 9 numbered sunspot groups were identified on the disk over the past 24 hours. The largest flare is ongoing (currently around C6), from a returning region rotating into view from the east limb. SIDC Sunspot Group 244 (NOAA Active Region 3836) currently located at S12E05 has a Beta-Gamma magnetic configuration and was stable over the past 24 hours. Solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares likely and a small chance for X-class flares.
No Earth directed CMEs were observed in the past 24 hours.
SIDC Coronal Hole 65, a small negative polarity equatorial coronal hole, crossed central meridian on 26 September, a HSS may be expected at the Earth in the next 24 hours.
The Earth is inside a slow solar wind stream, with speeds around 350 km/s and an interplanetary magnetic field of about 5 nT. A mild high speed solar wind stream may arrive in the next 24 hours.
The geomagnetic conditions over the past 24 hours were quiet to unsettled both locally and globally (K_Bel and Kp up to 3). Active conditions can be expected for the next 24 hours.
Over the past 24 hours, the greater than 10 MeV GOES proton flux has been at nominal levels, and is expected to remain so over the next 24 hours.
The greater than 2 MeV electron flux as measured by GOES 16 and 18 was below the 1000 pfu threshold in the past 24 hours. Similar conditions can be expected for 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 : 164, sur la base de 13 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 195 |
| AK Chambon La Forêt | 015 |
| AK Wingst | 008 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 164 - Basé sur 22 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
De nombreuses personnes consultent SpaceWeatherLive pour suivre l'activité solaire ou observer les aurores boréales, mais l'augmentation du trafic engendre des coûts plus élevés pour maintenir les serveurs en ligne. Si vous appréciez SpaceWeatherLive et souhaitez soutenir le projet, vous pouvez vous abonner pour un site sans publicité ou faire un don. Grâce à votre aide, SpaceWeatherLive restera accessible !
| Dernière classe X | 04/02/2026 | X4.21 |
| Dernière classe M | 25/02/2026 | M2.4 |
| Dernier orage géomagnétique | 03/03/2026 | Kp5 (G1) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (4%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| février 2026 | 78.2 -34.3 |
| mars 2026 | 74.4 -3.8 |
| 30 derniers jours | 52.8 -75.1 |