Publié: 2021 Feb 04 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 04 Feb 2021 | 074 | 007 |
| 05 Feb 2021 | 074 | 007 |
| 06 Feb 2021 | 074 | 007 |
Solar activity was at low levels over the past 24 hours. The only active region on the visible Sun, NOAA AR 2801 has reduced its size, number of sunspots and simplified its magnetic configuration from beta to alpha. Solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraphic imagery.
An equatorial positive polarity coronal hole traversed central meridian yesterday, its associated high speed solar wind is expected to arrive to the Earth on 7 February.
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 threshold during the past 24 hours. The electron flux is expected to go above this alert level for the next period. The 24h electron fluence was mostly at normal levels, it is expected to increase in the next 24 h.
Over the past 24 hours, the solar wind speed ranged between 475 and 550 km/s. The total magnetic field strength fluctuated between 4 and 8 nT. Bz had a minimum value of -6 nT. The interplanetary magnetic field was directed towards the Sun (negative polarity). The Earth is under the influence of the high-speed solar wind stream associated with the elongated negative polarity coronal hole that began to cross the central meridian on Jan 28. The solar wind speed is expected to decrease over the next 24 hours.
Geomagnetic conditions reached active levels (NOAA Kp recorded values between 1-4, local k Dourbes between 1-4). Geomagnetic conditions are expected to be mostly quiet to unsettled, with possible active periods, in the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | 022 |
| Flux solaire à 10 cm | 074 |
| AK Chambon La Forêt | 021 |
| AK Wingst | /// |
| Ap estimé | 013 |
| Nombre international de taches solaires estimé | 006 - Basé sur 18 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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