Publié: 2021 Dec 31 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 31 Dec 2021 | 100 | 004 |
| 01 Jan 2022 | 098 | 010 |
| 02 Jan 2022 | 096 | 021 |
NOAA region 2918 (Catania group 96) produced a few more C flares while in decay. The largest was a C9.8 flare peaking at 6:56UT. The most significant region on disc remains NOAA region 2916 which continues to have mixed polarity fields in the trailing part. It nevertheless remained quiet and stable. The two unipolar regions on disc (NOAA 2917 and 2919) remained unipolar while a new region is starting to emerge around S15E32. Flaring at C level remains likely with only a limited chance for flaring to reach M class levels.
No Earth directed CMEs have been observed in 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 2MeV electron flux remained under the 1000 pfu threshold. The 24h electron fluence was at normal levels and is expected to be at normal levels over the next 24 hours. Electron fluxes could start building up again in the next days with the expected elevated Solar wind speeds.
Solar wind remained only slightly elevated but showed an overall return to slow Solar wind conditions. Solar wind speed decreased from around 500km/s to 430km/s. The magnetic field magnitude hovered around a nominal 4nT value. The magnetic field phi angle indicated connection to a positive polarity sector. A further decrease to slow Solar wind conditions is expected over the next 24 hours. This is expected to be followed by a renewed increase starting around midnight 1-2 January related to another equatorial positive polarity coronal hole that crossed the central meridian December 29-30.
Geomagnetic conditions were mostly quiet (NOAA Kp 0-2) with only an isolated period of unsettled conditions locally (local K Belgium reaching 3 early in the period). Geomagnetic conditions are expected to be quiet over the next 24 hours before reaching unsettled conditions and potentially active levels in response to the elevated Solar wind conditions by early January 2.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 060, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 102 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 010 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 072 - Basé sur 14 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
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 | 21/01/2026 | M3.4 |
| Dernier orage géomagnétique | 22/01/2026 | Kp5+ (G1) |
| 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 | 119.4 -4.6 |
| 30 derniers jours | 121.8 +8.9 |