Publié: 2021 Sep 28 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 28 Sep 2021 | 086 | 007 |
| 29 Sep 2021 | 086 | 007 |
| 30 Sep 2021 | 086 | 014 |
Two active regions (ARs) present on the visible solar disk. NOAA AR 2871 (beta-gamma magnetic field configuration) produced a C1.6 flare peaking at 06:34 UT. Over the next 24 hours, more C-class flares can be expected.
The C-class flare mentioned above was related to a CME (and dimmings, type II radio bursts and an EUV wave), mostly directed towards the west, but with an Earth directed component. The CME was first seen in STEREO/COR2 at 06:52 UT (during a gap in LASCO data). Its speed is calculated to be 1050 km/s, with an expected arrival time to the Earth (glancing blow) around 16:00 UT on 30 September.
The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay there in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, it may increase over the next 24 hours. The electron fluence was at normal levels over the past 24 hours, it may increase over the next 24 hours.
Early on 27 September we have seen the (weak) effects of an ICME arrival to the Earth, related to the CMEs that erupted on 23 September. Later on 27 September, we saw the arrival of a high speed stream from the low latitudinal extension of the northern polar coronal hole (positive polarity). Solar wind speeds have reached 540 km/s with magnetic fields up to 15 nT (with Bz mostly positive). Elevated solar wind speeds with lower magnetic field magnitudes can be expected for the next 24 hours.
Geomagnetic conditions were quiet to unsettled (NOAA Kp and K Dourbes 1-3) over the past 24 hours, similar conditions can be expected for the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 056, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | 054 |
| Flux solaire à 10 cm | /// |
| AK Chambon La Forêt | 011 |
| AK Wingst | 008 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 044 - Basé sur 22 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 | 08/12/2025 | X1.1 |
| Dernière classe M | 14/01/2026 | M1.6 |
| Dernier orage géomagnétique | 11/01/2026 | 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 | 91.4 -32.6 |
| 30 derniers jours | 97.3 -8.4 |