Publié: 2022 Oct 26 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 26 Oct 2022 | 117 | 002 |
| 27 Oct 2022 | 120 | 010 |
| 28 Oct 2022 | 122 | 007 |
Solar flaring activity was at low levels and infrequent, with two C-class flares detected over the last 24 hours. NOAA Active Region (AR) 3133 (magnetic type Beta) produced both C-class flares and is expected to produce more in the next 24 hours. NOAA AR 3131 (Catania group 73, magnetic type Beta) is also capable of producing C-class flaring activity during the coming 24 hours.
Two front-sided Coronal Mass Ejections (CME) were observed by satellite coronographs, however, none of them are estimated to be geo-effective.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
An equatorial coronal hole of positive polarity started crossing the central meridian today. An associated high speed stream in in-situ solar wind measurements is expected for 29 Oct.
The Solar Wind (SW) conditions returned to a slow wind regime during the last 24 hours. The SW speed dropped from 430 to 240 km/s, while the total magnetic field (Bt) remained bellow 5 nT, and its North-South (Bz) component ranged between -4 and 4 nT in the last 24 hours. The interplanetary magnetic field phi angle was most of the time directed towards the Sun over the last 24 hours. A High Speed Stream (HSS) is expected to arrive tomorrow and cause a significant effect to the SW conditions.
Geomagnetic conditions were quiet both globally and locally (NOAA Kp and K Belgium 0-2) over the last 24 hours. The are expected to increase to active conditions in the next 24 hours, since a HSS is expected to arrive some time tomorrow.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 072, sur la base de 16 stations.
| Nombre de Wolf, observé par Catania | 090 |
| Flux solaire à 10 cm | 116 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 003 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 073 - Basé sur 25 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 | 01/02/2026 | X1.0 |
| Dernière classe M | 01/02/2026 | M1.8 |
| Dernier orage géomagnétique | 28/01/2026 | 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 |
| 30 derniers jours | 119.2 +2.7 |