Publié: 2019 Feb 25 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 25 Feb 2019 | 071 | 001 |
| 26 Feb 2019 | 070 | 012 |
| 27 Feb 2019 | 071 | 010 |
Over the past 24 hours solar activity has been low. No significant flares have been recorded. No Active Regions (AR) or filament channels are present on the solar disk. The greater-than 10 MeV proton flux was at nominal values. A negative polarity equatorial coronal hole (CH) has reached W30S15.
Solar activity is expected to remain at low levels.
The solar wind speed has fluctuated between 310 and 340 km/s (DSCOVR) over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT (DSCOVR). The Bz component fluctuated around 0 nT, ranging between -4 and +4 nT. Geomagnetic conditions ranged between Kp index 0-1 (NOAA) and local K index 0-3 (Dourbes) over the past 24 hours. A positive polar coronal hole is currently positioned near W30S15 in the Western hemisphere of the Sun and the associated co-rotating interaction region and high-speed stream (HSS) may enhance solar wind speeds over the next couple of days and as a consequence increase geomagnetic activity levels to active conditions.
Geomagnetic conditions are expected to be quiet to unsettled.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 30 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 071 |
| AK Chambon La Forêt | 003 |
| AK Wingst | 001 |
| Ap estimé | 001 |
| Nombre international de taches solaires estimé | 000 - Basé sur 32 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
Toutes les heures sont indiquées en UTC
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