Publié: 2022 Aug 22 1248 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 22 Aug 2022 | 096 | 018 |
| 23 Aug 2022 | 097 | 016 |
| 24 Aug 2022 | 110 | 011 |
Solar flaring activity was at low levels over the past 24 hours. There are five active regions present on the visible solar disk, with a newly emerged region located on NE. Two returning active region are about to rotate in the visible part of the disk on SE. NOAA AR 3085 has been the most energetic, exhibiting growth and producing the largest flare of the period, a C2.4-class flare, peaking at 21 August 23:47 UTC. Flaring activity is expected remain mainly at low levels over the next 24 hours, with a small chance of M-class flares.
No Earth directed Coronal Mass Ejections (CMEs) were detected in the available coronagraphic imagery over the past 24 hours.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours. The proton flux is expected to remain at nominal levels for the next 24 hours. The greater than 2MeV electron flux was about the 1000 pfu threshold over the past 24 hours. It is expected remain about about threshold over the next 24 hours. The 24h electron fluence was at moderate levels over the past 24 hours. It is expected be at nominal to moderate levels over the next 24 hours.
The solar wind parameters reflect high speed streams (HSS) and ICME influences over the past days. Over the past 24 hours, the solar wind magnetic field values were quite stable, fluctuating between 5 and 8 nT, while Bz had values between -7 and 6nT. The solar wind speed was fairly stable at around 570 km/s, with variations. The interplanetary magnetic field phi angle was on the negative sector (towards the Sun). Over the next 24 hours, we are expecting the impact of those effects to persist.
Active conditions were recorded at 21 August 15:00-19:00 UTC (NOAA Kp and/or K Dourbes 4) over the past 24 hours. Unsettled to active conditions can be expected over the past 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 076, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 097 |
| AK Chambon La Forêt | 022 |
| AK Wingst | 017 |
| Ap estimé | 017 |
| Nombre international de taches solaires estimé | 061 - Basé sur 27 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 | 117.9 -6.1 |
| 30 derniers jours | 121.2 +12.1 |