Prohlížíte si archiv středa 23. května 2018

Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2018 May 23 1255 UTC

SIDC Předpověď

Sluneční erupce

Quiet conditions (<50% probability of C-class flares)

Geomagnetismus

Active conditions expected (A>=20 or K=4)

Sluneční protony

Quiet

	10cm tok	Ap
23 May 2018	072	015
24 May 2018	073	008
25 May 2018	074	007

Bulletin

Solar activity increased during the period due to a new region rotating around the East limb in the Northern hemisphere. This new region produced thirteen B-class flares among them the largest B8.9 flare peaking at 14:59 UT yesterday. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. Solar activity is expected to be at low levels with a significant chance for C-class flare. Solar wind speed gradually increased as expected from around 320 km/s to around 490 km/s during the period under the influence of positive polarity extension of the northern polar coronal hole. Total magnetic field varied from 2 to 12 nT, while Bz component varied from +10 to -9 nT. Geomagnetic conditions were mostly quiet until 06:00 UT today, then both local index (Dourbes) and planetary (NOAA) reached the value K = 3 due to the enhanced solar wind speed. Mainly unsettled and active geomgnetic conditions can be expected today and tomorrow.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 027, na základě 14 stanic.

Solární indexy za 22 May 2018

Wolfovo číslo Catania	013
10cm sluneční tok	071
AK Chambon La Forêt	013
AK Wingst	007
Odhadovaný Ap	006
Odhadovaný mezinárodní počet slunečních skvrn	013 - Na základě 32 stanic

Souhrn významných událostí

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

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