Prohlížíte si archiv pátek 27. března 2015

Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2015 Mar 27 1455 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
27 Mar 2015	136	011
28 Mar 2015	133	008
29 Mar 2015	130	008

Bulletin

Only weak C-class flares were reported during last 24 hours, despite the presence of the complex beta-gamma-delta active region (NOAA AR 2305) on the solar disc. The strongest reported flare C1.4 (peaking at 19:21 UT) on March 26 also originated from the Catania sunspot group 13(NOAA AR 2305) which started to decay and it currently has beta-gamma configuration of its photospehric magnetic field. We expect C-class flares in the coming hours. No Earth directed CMEs were observed during last 24 hours. The Earth is currently inside a slow solar wind with the speed of about 410 km/s, and the interplanetary magnetic field is stable with the magnitude of about 6nT. The sudden change of the magnetic field phi angle, at about 14:30 UT on March 26 and its stable value since then, indicates crossing of the sector boundary. The southern polar coronal hole is strongly extended towards solar equator, up to about S35, and this part of the coronal hole has reached the central meridian early today. The associated fast flow might be expected at the Earth on March 30. The geomagnetic conditions are quiet and expected to remain so in the coming hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 075, na základě 12 stanic.

Solární indexy za 26 Mar 2015

Wolfovo číslo Catania	///
10cm sluneční tok	136
AK Chambon La Forêt	019
AK Wingst	012
Odhadovaný Ap	011
Odhadovaný mezinárodní počet slunečních skvrn	077 - Na základě 15 stanic

Souhrn významných událostí

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

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