Publié: 2020 Dec 03 1241 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 03 Dec 2020 | 105 | 007 |
| 04 Dec 2020 | 102 | 032 |
| 05 Dec 2020 | 098 | 011 |
Solar activity was low with the largest flare of the period a C1.7 flare peaking at 1:56UT from NOAA AR 2786. There are 3 regions on disk. The largest is NOAA AR 2786, which although large now has a simple alpha configuration. Region NOAA AR 2790 is of beta configuration but was inactive. Further C flares are probable with only a small chance of an isolated M flare.
There were no new observations of Earth-directed Coronal Mass Ejections.
The greater than 10MeV proton flux remained enhanced (max 5 pfu), with a general decaying trend. The greater than 2MeV electron flux did briefly exceed the 1000 pfu alert threshold during the diurnal maximum. The 24h electron fluence was at moderate levels and is expected to be at normal to moderate levels over the next 24 hours. An increase in levels is still possible over the next days following the recent Solar wind enhancements, and with the possible CME glancing blow.
Solar wind conditions became nominal with Solar wind speed further decreasing to 360 km/s. The interplanetary magnetic field magnitude was around a nominal 5nT with a variable and unremarkable North-South orientation. The phi angle was mostly in the negative sector (towards the Sun). There were no signs of possible perturbations associated to the November 29 CME and this is now not expected anymore. Essentially nominal Solar wind conditions are expected with a slight chance for perturbations from the morning of December 4 onwards associated to the December 1 CME.
Geomagnetic conditions were quiet (local K Dourbes 0-2 and NOAA Kp 0-1). Geomagnetic conditions could possibly become active or show minor geomagnetic storm conditions should a glancing blow from the December 1 CME occur.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 039, sur la base de 07 stations.
| Nombre de Wolf, observé par Catania | 050 |
| Flux solaire à 10 cm | 105 |
| AK Chambon La Forêt | 004 |
| AK Wingst | 003 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 043 - Basé sur 12 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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