Publié: 2023 Nov 14 1235 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 14 Nov 2023 | 134 | 016 |
| 15 Nov 2023 | 130 | 007 |
| 16 Nov 2023 | 124 | 007 |
There are six active regions visible on the disk. Flaring activity has been low, with only minor C-class flaring in the last 24 hours. The strongest one was a C2.9 flare from NOAA AR 3477 (beta magnetic field configuration), peaking at 20:50 UTC on 13 November. NOAA AR 3483 has a beta-gamma magnetic field configuration while the other regions have simpler beta magnetic field configuration. Most of these active regions are rotation out of view over the west limb. More C-class flares are expected.
No Earth directed CMEs were observed in the last 24 hours.
In the last 24 hours, the Earth was under the influence of an ICME corresponding probably to an early arrival of the CME from 10 November. The ICME arrived around 16:20 UTC on 13 November with an interplanetary magnetic field reaching 15 nT (with positive Bz) and solar wind speed around 450 km/s. Similar disturbed conditions can be expected for the next 24 hours.
During the last 24 hours the geomagnetic conditions were quiet to unsettled (NOAA KP 3, K_Bel 3). Since Bz was positive within the ICME so far, its geomagnetic impact was minor. Similar conditions can be expected in the next 24 hours, with possible active and minor storm periods if Bz turns negative.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next 24 hours.
The greater than 2 MeV electron flux was below the 1000 pfu threshold, as measured by GOES 16. It is expected to remain so in the next 24 hours. The 24 hour electron fluence was at moderate levels, it is expected to stay at those levels for the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 060, sur la base de 10 stations.
| Nombre de Wolf, observé par Catania | 080 |
| Flux solaire à 10 cm | 134 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 018 |
| Ap estimé | 018 |
| Nombre international de taches solaires estimé | 074 - 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
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 | M1.4 |
| 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 | 129.4 +16.8 |
| 30 derniers jours | 129.3 +29.3 |