Publié: 2016 Mar 02 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 02 Mar 2016 | 097 | 008 |
| 03 Mar 2016 | 096 | 008 |
| 04 Mar 2016 | 094 | 008 |
The strongest flare reported in the last 24 hours was the B3.4 flare (peaked at 17:57 UT on March 1), which originated from the Catania sunspot group 27 (NOAA 2506). Although the probability for the C-class flares is low (about 20%) they are still possible, in particular from the unnamed active region which just rotated from the behind of the East solar limb. The prominence eruption was observed at about 08:00 UT on March 1, with the source region close to the East solar limb. The prominence eruption was associated with rather slow CME (speed reported by the CACTUS software is about 500 km/s) with angular width of about 115 degrees. No Earth directed CMEs were observed in the last 24 hours. The solar wind speed has increased and its current value is about 450 km/s, the interplanetary magnetic field magnitude is about 10 nT. The small equatorial corona hole has reached the central meridian this morning. The associated fast solar wind can be expected on Marc 5. The geomagnetic conditions are quiet to unsettled. Currently the Bz component of the interplanetary magnetic field is positive however if the Bz component turns negative we can expect unsettled to active conditions in the coming hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 069, sur la base de 18 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 097 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 010 |
| Ap estimé | 009 |
| Nombre international de taches solaires estimé | 063 - Basé sur 15 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 |