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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2022 Mar 16 1231 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

Quiet (A<20 and K<4)

Sluneční protony

Quiet

	10cm tok	Ap
16 Mar 2022	110	007
17 Mar 2022	108	007
18 Mar 2022	106	007

Bulletin

There are four active regions on the visible solar disc. NOAA AR 2965 continues to be the most active one, although it has decreased in size in the past 24 hours. It has produced two M-class flares and two C-class flares in the last 24 hours. The strongest was a M1.5 flare, peaking at 22:46 UT, on 15 March. The other active regions have simple magnetic field configuration (alpha or beta) and have not produced any significant flares. For the next 24 hours, C-class flares are expected and M-class flares are possible.

No Earth-directed coronal mass ejections (CMEs) were observed in available coronagraph imagery in the past 24 hours.

The greater than 10 MeV proton flux was at nominal levels and is expected to remain so in the next 24 hours. The greater than 2MeV electron flux was under the 1000 pfu threshold and is expected to remain so for the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so in next 24 hours.

The Earth is inside a slow solar wind flow, with solar wind speeds close to 410 km/s and an interplanetary magnetic field magnitude around 4 nT. Similar conditions are expected for the next 24 hours.

The geomagnetic conditions over the past 24 hours were mostly quiet (K_Bel = 1-3 and Kp = 1-3) . Similar conditions can be expected for the next 24 hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 058, na základě 08 stanic.

Solární indexy za 15 Mar 2022

Wolfovo číslo Catania	///
10cm sluneční tok	110
AK Chambon La Forêt	012
AK Wingst	008
Odhadovaný Ap	007
Odhadovaný mezinárodní počet slunečních skvrn	067 - Na základě 11 stanic

Souhrn významných událostí

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

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