Publié: 2021 May 28 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 28 May 2021 | 082 | 009 |
| 29 May 2021 | 080 | 008 |
| 30 May 2021 | 080 | 004 |
The Sun has released two C flares during the past 24 hours. The brightest flare was a C7.6 flare produced by beta-gamma region NOAA 2824, peaking at 23:15 UT on May 27. The chance for a C flare in the next 24 hours is estimated at 80%, while the chance for an M flare is estimated at 15%.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.
The solar wind speed as registered by DSCOVR varied between about 390 km/s and 455 km/s in the past 24 hours, with current values around 440 km/s. The Interplanetary Magnetic Field (IMF) was oriented away from the Sun and its magnitude varied between about 5 and 10 nT. Bz was never below -5 nT for extended intervals. Solar wind conditions are expected to gradually decline on May 28-29.
Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 0 and 3) were registered in the past 24 hours. Active geomagnetic intervals (K Dourbes = 4) are possible on May 28 and 29, with a slight chance for minor storm geomagnetic levels (K Dourbes = 5) on May 28. Quiet to unsettled levels (K Dourbes < 4) are expected on May 30.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 029, sur la base de 23 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 083 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 018 |
| Ap estimé | 019 |
| Nombre international de taches solaires estimé | 039 - Basé sur 29 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 | 16/02/2026 | M2.4 |
| Dernier orage géomagnétique | 16/02/2026 | Kp6 (G2) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| février 2026 | 100.6 -12 |
| 30 derniers jours | 117.7 +9.9 |