Publié: 2021 Aug 21 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 21 Aug 2021 | 077 | 007 |
| 22 Aug 2021 | 079 | 007 |
| 23 Aug 2021 | 081 | 007 |
One numbered active region is visible on the solar disk: NOAA 2858 (beta magnetic field configuration). There is a region that rotated over the east limb (unnumbered still) that produced 3 C-class flares in the past 24 hours, the strongest being a C3.0 flare peaking at 15:57 UT on 20 August. There is another region rotating into view in the southern hemisphere. More C-class flares can be expected, M-class flares are possible.
The AR rotating into view from the southern hemisphere produced a wide eastward CME first seen by LASCO C2 at 06:12 UT on 20 August. given the position of the source region behind the limb, this CME is not expected to affect the Earth. No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery.
The southern extension of the north polar coronal hole has crossed central meridian today, a related high speed stream may arrive to the Earth in about 3 days.
The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, while the 24h electron fluence was at normal levels over the past 24 hours. Over the next 24 hours they are expected to remain at those levels.
Over the past 24 hours the solar wind speed has been around 350 km/s. The total magnetic field strength varied between 2 and 8 nT, with positive polarity (directed away from the Sun). Similar slow solar wind conditions are expected for the next 24 hours.
Geomagnetic conditions were at quiet to unsettled levels (NOAA Kp 0-2 and K Dourbes 0-3) over the past 24 hours. Similar conditions are expected over the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 015, sur la base de 16 stations.
| Nombre de Wolf, observé par Catania | 015 |
| Flux solaire à 10 cm | 078 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 006 |
| Ap estimé | 006 |
| Nombre international de taches solaires estimé | 013 - Basé sur 27 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 |