Publié: 2020 Feb 28 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 28 Feb 2020 | 072 | 010 |
| 29 Feb 2020 | 072 | 006 |
| 01 Mar 2020 | 071 | 010 |
Solar activity was at very low levels. The Sun is still spotless. A small active region close to the east limb at latitude S10 seems spotless, whereas another small region at latitude N25 is still at the east limb as seen in SDO/AIA imagery. No earth-directed coronal mass ejections (CMEs) have been observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values. A small and irregularly shaped equatorial negative polarity coronal hole (CH) is present on the solar disk.
Solar activity is expected to remain at very low levels.
Solar wind conditions were at background levels. Solar wind speed declined from about 380 km/s at the beginning of the period to 330 km/s by 06:30UT, then increasing again to its current value around 350 km/s(ACE). Bz undulated between -4 and +4 nT. The direction of the interplanetary magnetic field (phi angle) was mainly towards the Sun until around 06:30UT, when it switched towards predominantly a positive sector (away from the Sun). Geomagnetic conditions were at quiet levels, with an unsettled episode (09-12UT) recorded at Dourbes.
Geomagnetic activity is expected to be mostly at quiet levels, with an isolated unsettled interval remaining possible. Late on 29 February or during 01 March, geomagnetic conditions may become unsettled with a chance on an active episode following the expected arrival of a wind stream associated with the negative polarity CH.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 20 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 071 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 003 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 000 - Basé sur 23 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 | 94.2 -18.4 |
| 30 derniers jours | 108.9 -4.7 |