Publié: 2017 Apr 05 1230 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 05 Apr 2017 | 091 | 004 |
| 06 Apr 2017 | 089 | 005 |
| 07 Apr 2017 | 087 | 005 |
Solar activity was at low levels during the period. Flaring activity decreased as NOAA 2644 rounded the west limb. NOAA 2645 produced most of the flaring, including a C4.9 event peaking at 23:42UT, the strongest event of the period. This region still has a complex magnetic trailing portion. The 10.7cm radio flux dropped from 108 sfu on 3 April to 94 sfu on 4 April. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10MeV proton flux was at nominal levels.
Mostly C-class flaring is expected, with a chance on an isolated M-class flare. A major flare from NOAA 2645 may drive the proton levels above event threshold.
During the first half of the period, solar wind speed was somewhat enhanced with speeds around 470 km/s. This may be the brief and weak influence of the moderate speed stream from the positive equatorial coronal hole (CH). Solar wind speed was near 410 km/s during the second half of the period. Bz was mostly positive, fluctuating between +13 and -6 nT. Total magnetic field strength B was in a generally declining trend, from 16 to 5 nT. The direction of the interplanetary magnetic field was variable, pointing towards the Sun by the end of the period.
The geomagnetic field was at quiet to unsettled levels, and is expected to remain so. There's a small chance on an active episode.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 054, sur la base de 21 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 094 |
| AK Chambon La Forêt | 018 |
| AK Wingst | 016 |
| Ap estimé | 018 |
| Nombre international de taches solaires estimé | 079 - Basé sur 33 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 | X4.3 |
| Dernière classe M | 12/02/2026 | M1.4 |
| 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 | 121.7 +9.1 |
| 30 derniers jours | 131.5 +34.7 |