Publié: 2020 Aug 12 1233 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 12 Aug 2020 | 075 | 005 |
| 13 Aug 2020 | 075 | 007 |
| 14 Aug 2020 | 075 | 007 |
The solar activity was quiet over the past 24 hours. The sunspot (NOAA-AR 2770) continued to produce small B-class flares. The X-ray flux remained, however, below C-class level. An new region showing some activity is currently turning around the East limb (at about 30 degree latitude South). The solar activity is expected to remain at low levels with a very small chance of occurring a C-class flare from the Region NOAA-AR 2770 and eventually from the new region.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery in the last 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux reached high levels over the past 24 hours and may reach high levels over the next 24 hours.
The Earth continued to be under the influence of the slow solar wind streams. The solar wind parameters (DSCOVR) show nominal values with the solar wind speed around 300 km/s, the total interplanetary magnetic field below 5 nT, and the Bz magnetic field components fluctuating between -4.2 nT and +3.4 nT. The solar wind conditions are expected to remain mostly nominal for the next days.
Geomagnetic conditions were quiet, and quiet conditions are expected for the next following day.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 017, sur la base de 29 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 074 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 004 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 012 - Basé sur 33 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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