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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2015 Apr 26 1230 UTC

SIDC Předpověď

Sluneční erupce

Eruptive (C-class flares expected, probability >=50%)

Geomagnetismus

Quiet (A<20 and K<4)

Sluneční protony

Quiet

	10cm tok	Ap
26 Apr 2015	123	008
27 Apr 2015	121	015
28 Apr 2015	119	007

Bulletin

Solar flaring activity was low with just two C flares occurring over the period. The largest was a long duration event from over the western limb, peaking at 18:49UT at C1.9 magnitude. It was associated with an eruption and CME, which appears to be not directed to Earth. Another C1.0 flare from Catania group 37 (NOAA region 2331) peaked just before the end of the period at 11:49UT. Flaring at C level is expected over the next days. An asymmetric full halo CME was also visible in SoHO/LASCO coronagraph data from 14:48UT onwards in the C2 field of view. No related on disc activity could be associated, and the event is believed to be backsided and hence not geoeffective. Solar wind was at nominal levels with speeds in the 290-330 km/s range and total magnetic field in the 2.1-4.6 nT range. Bz was variable though initially mostly positive. Phi angle was stable in the outward sector. Geomagnetic conditions were quiet to unsettled (NOAA Kp 0-1, local K Dourbes 0-3). Nominal solar wind conditions with associated quiet to unsettled geomagnetic conditions are expected to continue over the next days. Some possible sector boundary crossings could slightly enhance solar wind conditions.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 042, na základě 11 stanic.

Solární indexy za 25 Apr 2015

Wolfovo číslo Catania	///
10cm sluneční tok	126
AK Chambon La Forêt	003
AK Wingst	002
Odhadovaný Ap	001
Odhadovaný mezinárodní počet slunečních skvrn	051 - Na základě 16 stanic

Souhrn významných událostí

Poskytuje Centrum pro analýzu dat o solárních vlivech© - SIDC - Zpracováno SpaceWeatherLive

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