Publié: 2023 Jan 07 1235 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 07 Jan 2023 | 172 | 002 |
| 08 Jan 2023 | 174 | 003 |
| 09 Jan 2023 | 175 | 003 |
Solar flaring activity reached moderate levels. NOAA Active Region (AR) 3182 produced an M1.6 flare, peaking at 00:52 UTC January 07 as well as multiple C-class flares. Further C-class flares were produced by NOAA AR 3183 including a C5 and C6 flare at 20:27 and 18:53 UTC on January 06, respectively. NOAA AR 3182 and 3181 exhibited further sunspot growth. NOAA AR 3180 and 3177 decayed slightly. Solar flaring activity is expected to be moderate over the next 24 hours with a high probability of C-class flares, M flares likely and a chance for further X-class flares.
No Earth directed CMEs have been observed in the coronagraph data.
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 was below the 1000 pfu threshold. It is expected remain below the 1000 pfu threshold over the next 24 hours. The electron fluence was at normal levels and is expected to be at normal levels over the next days.
The magnitude of the interplanetary magnetic field gradually decreased, with values between 3 and 11 nT. The orientation of the magnetic field was predominantly in the negative sector (field directed towards the Sun) with a variable north-south component (Bz ranging between -7 to 9 nT). The solar wind speed values gradually ranged between 400 and 520 km/s. January 07-08 we expect a gradual return to slow solar wind regime.
Geomagnetic conditions were quiet to unsettled (NOAA Kp =3 and local K-Dourbes =2). Quiet to unsettled conditions are expected over the next days.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 134, sur la base de 13 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 172 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 004 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 135 - Basé sur 19 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 07 | 0040 | 0052 | 0102 | S18E56 | M1.6 | SF | 38/3182 | VI/2 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Dernière classe X | 18/01/2026 | X1.9 |
| Dernière classe M | 19/01/2026 | M1.2 |
| Dernier orage géomagnétique | 19/01/2026 | Kp9- (G4) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| janvier 2026 | 103.8 -20.2 |
| 30 derniers jours | 109 +1.5 |