Publié: 2021 Sep 01 1236 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 01 Sep 2021 | 085 | 007 |
| 02 Sep 2021 | 085 | 025 |
| 03 Sep 2021 | 085 | 007 |
Apart from a single C1.2 flare from Catania group 32 (NOAA 2860), X-ray flux remained below C level. Catania group 32 (NOAA 2860) shrunk and reduced in complexity (now Beta type of its photospheric magnetic field). It remains a likely source for C class flaring with only a small chance for M class flare remaining. The new region rotating onto the disc in the North East appears to be spotless.
There were no new Earth directed CMEs observed in available coronagraph data.
The greater than 10 MeV proton flux was at background levels and we expect it will remain so in the next 24 hours. The greater than 2 MeV electron flux reached again above the 1000 pfu threshold during its diurnal maximum both yesterday and today. The 24h electron fluence is at moderate levels and we expect it to follow slowly decaying trend.
A negative polarity coronal hole in the southern hemisphere is about to start crossing the central meridian. It is expected to influence Solar wind conditions near Earth on September 5.
Solar wind is in a slow Solar wind regime with no obvious signs of arrival of the August 26 CME. Solar wind speed was mostly in the 310-350 km/s range. Interplanetary magnetic field was below or around 5nT with an unremarkable Bz component. The orientation of the Interplanetary magnetic field was mostly towards the Sun. Solar wind is likely to become enhanced again with an expected arrival of the August 28 CME tomorrow before noon.
Geomagnetic conditions have been quiet (NOAA Kp 0-2 and local K Dourbes 1-2 ). Active conditions are possible over the next 24-48 hours with the possible August 28 CME arrival.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 036, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | 033 |
| Flux solaire à 10 cm | 084 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 008 |
| Ap estimé | 007 |
| Nombre international de taches solaires estimé | 040 - Basé sur 35 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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