Publié: 2015 May 15 1230 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 15 May 2015 | 140 | 011 |
| 16 May 2015 | 138 | 012 |
| 17 May 2015 | 136 | 018 |
NOAA 2339 and 2342 were the only sunspot regions actively producing low-level C-class flares. NOAA 2339 was the source of the strongest flare of the period, a C4.8 peaking at 17:53UT. Some opposite polarity flux has emerged in its trailing section. NOAA 2342 produced two C2 flares peaking resp. at 14:08UT and 00:11UT, related to eruptive phases of the group filament. An active region is rounding the southeast solar limb and was responsible for a C1 flare (06:50UT). No earth-directed coronal mass ejections (CMEs) have been observed.
Further C-class flaring is expected, with a chance on an M-class flare.
Solar wind speed declined from its initial value near 700 km/s to its current 530 km/s as Earth is gradually exiting the high speed stream (HSS) from the recurrent negative polarity coronal hole (CH). Bz oscillated mostly between -4 and +4 nT. Quiet to unsettled geomagnetic conditions were observed. A recurrent positive polarity CH is transiting the central meridian.
The arrival of the 13 May CME is expected late 17 - early 18 May, slightly preceding or nearly coinciding with the expected arrival of the HSS from the aforementioned positive CH. Until then, quiet to unsettled geomagnetic conditions are expected, with a chance on an active episode.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 090, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 145 |
| AK Chambon La Forêt | 017 |
| AK Wingst | 010 |
| Ap estimé | 011 |
| Nombre international de taches solaires estimé | 119 - Basé sur 25 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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