Publié: 2023 Feb 02 1230 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 02 Feb 2023 | 134 | 011 |
| 03 Feb 2023 | 132 | 013 |
| 04 Feb 2023 | 130 | 007 |
There are six active regions visible on the solar disc, all of them with simple alpha or beta magnetic field configuration. Solar flaring activity was at low levels over the past 24 hours, with several C-class flares detected. The strongest one was a C5.8 flare from NOAA AR 3204, peaking at 22:48 UTC on 1 February. This active region is rotating out of view over the west limb. Further C class flaring is expected.
No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery over the past 24 hours. LASCO C2 data is not available since 28 January. STEREO-COR2 data shows a wide CME at 09:38 UT on 1 February after a data gap, this CME is erupting from the NW limb and not expected to affect the Earth.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux has been below the 1000 pfu threshold and is expected to remain so. The 24h electron fluence was at normal levels and is expected to remain so over the next 24 hours.
There was a weak forward shock in the L1 solar wind data at 15:40 UTC on 1 February. The solar wind speed jumped from 348 to 369 km/s, the magnetic field went from 4 to 6 nT after the shock, and reached 11 nT later (with Bz briefly down to -10 nT). The driver of the shock was probably the mild high speed solar wind stream expected to arrive, reaching solar wind speeds about 100 km/s faster than before the shock. The interplanetary magnetic field has a negative polarity on the ecliptic plane (towards the Sun). Slightly disturbed solar wind conditions can be expected for the next 24 hours.
Geomagnetic conditions reached active levels both locally and at planetary levels (K_Dourbes and Kp up to 4). Mostly unsettled conditions expected for the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 069, sur la base de 08 stations.
| Nombre de Wolf, observé par Catania | 094 |
| Flux solaire à 10 cm | 134 |
| AK Chambon La Forêt | 018 |
| AK Wingst | 006 |
| Ap estimé | 006 |
| Nombre international de taches solaires estimé | 073 - Basé sur 25 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 | 11/02/2026 | M1.3 |
| 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 | 130.2 +30.2 |