Publié: 2021 Nov 29 1238 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 29 Nov 2021 | 093 | 015 |
| 30 Nov 2021 | 094 | 005 |
| 01 Dec 2021 | 094 | 010 |
Solar activity was at very low levels over the past 24 hours. There are three Active Regions (AR) visible on the Sun. NOAA AR 2899 has now rotated over the west limb, while a new simple region (NOAA AR 2901, alpha magnetic field configuration) has emerged in the North East quadrant. NOAA AR 2898 and 2900 are the largest regions on disk, both with beta magnetic field configuration. There is estimated to be a 50 percent probability of C-class flares in the next 24 hours.
There was a filament eruption observed in the southern hemisphere, visible from 06UT Nov 29. The bulk of the eruption appears to be directed to the south of the Sun-Earth line but a full analysis will be made when coronagraph data become available. No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu alert threshold in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.
The magnetic field was enhanced at the start of the period, due to the ongoing passage of the ICME that arrived on Nov 27. The magnetic field gradually decreased from 12 to 5 nT over the past 24 hours. Bz varied between -7 and 9 nT, with an extended period of negative Bz between 16UT Nov 28 and 05UT Nov 29. The solar wind speed remained low, oscillating around 390 km/s.
Geomagnetic conditions were at quiet to active levels (NOAA Kp and K-BEL recorded values of 1-4). Geomagnetic conditions are expected to be quiet to unsettled on Nov 29 and Nov 30.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 039, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 092 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 011 |
| Ap estimé | 010 |
| Nombre international de taches solaires estimé | 044 - Basé sur 13 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
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