Publié: 2016 Aug 20 1337 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 20 Aug 2016 | 081 | 005 |
| 21 Aug 2016 | 079 | 005 |
| 22 Aug 2016 | 077 | 012 |
Solar activity was very low in the past 24 hours. A B4.4 flare was observed today 20-Aug-2016 coming from the active region AR NOAA 2578 (peaking at 06:00 UT). Two additional active regions are presently observed on the visible side of the solar disc. Their photospheric magnetic field configuration is simple (alpha configuration). There is a transequatorial coronal hole observed presently on the visible solar disc which may become geoeffective in 3-4 days. No Earth-directed CME has been observed. Solar proton flux intensity is expected to lie within the background levels. Solar activity is expected to be low with small probability for B-class flares. The variations of the solar wind parameters were weak. Solar wind speed remained below 400 km/s during the last 24 hours. The magnitude of the Interplanetary Magnetic Field (Bt) elevated till 8 nT this morning (20-Aug-2016) and then it smoothly decreased till 5 nT. The Bz component demonstrated one variation within the interval 7nT : -4 nT and afterwards remained neutral. Geomagnetic conditions have been very quiet in the past 24 hours (K Dourbes between 1 and 3; NOAA Kp between 1 and 2). Geomagnetic activity is expected to continue at very low levels today (20-08-2016) and tomorrow (21-08-2016). Active to minor geomagnetic storm conditions (K Dourbes = 3-4) are possible later as a possible response to the transequatorial negative polarity coronal hole.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 019, sur la base de 16 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 081 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 006 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 050 - Basé sur 23 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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