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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2024 May 20 1231 UTC

SIDC Předpověď

Sluneční erupce

M-class flares expected (probability >=50%)

Geomagnetismus

Quiet (A<20 and K<4)

Sluneční protony

Warning condition (activity levels expected to increase, but no numeric forecast given)

	10cm tok	Ap
20 May 2024	201	007
21 May 2024	201	013
22 May 2024	201	022

Slunečně aktivní oblasti a vzplanutí

There are nine visible ARs on the solar disk. Flaring activity was driven by NOAA AR 3685 (beta-gamma magnetic field configuration) with three M-class flares, the strongest being an M2.5 one peaking at 17:47 UTC on 21 May. NOAA AR 3683 (beta magnetic field configuration) has produced several C-class flares today and has potential for stronger ones. More M-class flares are likely and X-class flares are possible in the next 24 hours.

Vyhazování koronální hmoty

A full halo CME was first seen at 05:36 UT on LASCO C2, originating from an eruption close to NOAA AR 3683 (located at the southwest, at S25W60), associated with a C6.7 flare. The CME speed is around 1500 km/s.The bulk of the CME is directed to the southwest, but a glancing blow can be expected on 22 May.

Solární bouře

The solar wind at the Earth is slow, with speeds around 350 km/s and interplanetary magnetic field around 8 nT. There are low chances of a glancing blow from the CME on 17 May, otherwise slow wind conditions can be expected for the next 24 hours.

Geomagnetismus

Geomagnetic conditions have been quiet in the last 24 hours (Kp and K_BEL up to 2). If we see a glancing blow from the 17 May CME, disturbed conditions may occur, otherwise quiet conditions can be expected for the next 24 hours.

Úrovně protonového toku

The 10 MeV GOES-18 proton flux was below threshold in the past 24 hours. It may increase over the next hours as a result of the halo CME from 05:36 UTC.

Elektronové toky na geostacionární oběžné dráze

The greater than 2 MeV electron flux from GOES 16 was below the threshold level in the last 24 hours. It is expected to remain below the threshold during the next 24 hours. The electron fluence was at normal levels for the last 24 hours and is expected to remain so.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 146, na základě 22 stanic.

Solární indexy za 19 May 2024

Wolfovo číslo Catania	///
10cm sluneční tok	201
AK Chambon La Forêt	015
AK Wingst	012
Odhadovaný Ap	011
Odhadovaný mezinárodní počet slunečních skvrn	167 - Na základě 25 stanic

Souhrn významných událostí

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

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