Publié: 2021 Sep 24 1343 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 24 Sep 2021 | 090 | 013 |
| 25 Sep 2021 | 090 | 010 |
| 26 Sep 2021 | 089 | 012 |
Multiple regions present on the sun with most magnetically complex the Catania 45/NOAA 2871, source of a M1.8 class flare. Over the next 24 hours, C-class flares can be expected with a slight possibility of further M class.
A CME associated with the M2.9 class flare on Sep 23 04:27UT may arrive from Sep 26 22:57UT.
The greater than 10 MeV proton flux was at background 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 remained below the 1000 pfu alert threshold. Over the next 24 hours, it is expected to increase towards the threshold. The 24h electron fluence was at nominal levels over the past 24 hours. Over the next 24 hours they are expected to remain at those levels, increasing towards moderate levels.
Over the past 24 hours the solar wind speed increased, reaching from 510 km/s. The total magnetic field strength had values between 1 and 9 nT, while its Bz component varied between -6 and 7nT. The interplanetary magnetic field phi angle has predominantly been on the negative sector (directed towards the the Sun). We seem to be under the influence of the high speed stream associated with the negative coronal hole, crossing central meridian Sep 21 and the CME 19 seemed to have an impact about Sep 23 12:00UT. An extension of the northern positive coronal hole is presently at central meridian. Solar wind parameters are expected to remain ehanced.
Geomagnetic conditions were at quiet to unsettled levels, (NOAA Kp 1-2 and K Dourbes 0-2) over the past 24 hours. Unsettled conditions with possibility of active events can be expected over the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 061, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 090 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 010 |
| Ap estimé | 011 |
| Nombre international de taches solaires estimé | 068 - Basé sur 20 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 23 | 1523 | 1528 | 1539 | S30E15 | M1.8 | 1N | 45/2871 | III/2 |
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 | X4.3 |
| Dernière classe M | 09/02/2026 | M2.8 |
| Dernier orage géomagnétique | 05/02/2026 | Kp5+ (G1) |
| 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 | 132.1 +19.5 |
| 30 derniers jours | 128.6 +27.4 |