Publié: 2017 Dec 16 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 16 Dec 2017 | 072 | 015 |
| 17 Dec 2017 | 072 | 019 |
| 18 Dec 2017 | 072 | 007 |
The Sun produced no C flares in the past 24 hours. The chance for a C flare in the next 24 hours is estimated at 5%. A filament eruption near 25S 40E was observed in GONG H-alpha and SDO/AIA 304 A images around 12h UT on December 15. An associated CME was detected by CACTUS in LASCO C2 images at 12:12 UT, with an estimated low speed of 284 km/s using COR2 A J-maps. This CME may arrive at Earth (probability: 20%), in which case it should arrive early on December 20 according to the drag based model. The greater than 10 MeV proton flux was at nominal levels. Solar wind speed measured by DSCOVR suddenly increased from about 345 to 370 km/s around 21:30 UT on December 15. Afterwards, it gradually decreased to current values around 340 km/s. The Interplanetary Magnetic Field (IMF) was mainly directed away from the Sun and its magnitude ranged between about 0.5 and 7 nT. Bz was never below -5 nT. Quiet geomagnetic conditions (K Dourbes between 0 and 2; NOAA Kp between 0 and 2) were registered in the past 24 hours. Active conditions (K Dourbes = 4) are possible on December 16 and 17, with a slight chance for minor geomagnetic storm intervals (K Dourbes = 5), due to the expected arrival of a high speed stream from a recurrent positive equatorial coronal hole. Quiet to unsettled conditions (K Dourbes < 4) are expected on December 18.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 16 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 072 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 003 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 000 - Basé sur 17 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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