Publié: 2016 Jan 24 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 24 Jan 2016 | 100 | 008 |
| 25 Jan 2016 | 104 | 006 |
| 26 Jan 2016 | 108 | 022 |
A single C-class flare was observed during the period. This long duration C1 flare was produced by NOAA 2488 and peaked at 04:55UT. The faculae field preceding old active region NOAA 2481 has started to round the southeast limb. This region was the source of some flaring activity and coronal mass ejections (CMEs) during its transit over the Sun's backside. The filament near NOAA 2487 has stretched to about 40 degrees in length and is transiting the central meridian. No earth-directed CMEs were observed.
There remains a good chance on a C-class flare.
Earth exited the high speed stream of the southern polar coronal hole (CH) late on 23 January. Solar wind speed declined from initial values between 550-600 km/s to values between 410-470 km/s by the end of the period. Bz varied between -5 nT and +5 nT, while the interplanetary magnetic field was mostly directed towards the Sun. Quiet to unsettled geomagnetic conditions were observed.
Mostly quiet to unsettled geomagnetic conditions are expected. Starting late on 25 or on 26 January, chances on an active episode may increase following the expected arrival of the high speed stream from the (positive) northern polar CH extension.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 044, sur la base de 07 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 099 |
| AK Chambon La Forêt | 020 |
| AK Wingst | 011 |
| Ap estimé | 011 |
| Nombre international de taches solaires estimé | 057 - Basé sur 20 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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