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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2021 Aug 15 1238 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

Quiet (A<20 and K<4)

Sluneční protony

Quiet

	10cm tok	Ap
15 Aug 2021	073	012
16 Aug 2021	074	010
17 Aug 2021	074	005

Bulletin

Solar flaring activity was at very low levels. NOAA regions 2853 and 2855, magnetic type alpha, are associated with sunspots once more. Newly emerged regions NOAA 2856 (north west, magnetic type beta) and NOAA 2877 (north centre, magnetic type beta) have emerged. Solar activity is expected to remain at low levels.

No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, while the 24h electron fluence was at nominal levels over the past 24 hours. Over the next 24 hours they are expected to remain at those levels.

Over the past 24 hours the solar wind speed slightly increased, reaching 480 km/s. The total magnetic field strength had values between 3 and 8 nT, while its Bz component varied between -8 and 6 nT. The interplanetary magnetic field phi angle was predominantly on the positive sector (directed away from the Sun). Over the next 24 hours, solar wind conditions are expected to continue in this pattern.

Geomagnetic conditions were at quiet to unsettled levels (NOAA Kp 1-3 and K Dourbes 0-3) over the past 24 hours. Quiet to unsettled conditions are expected over the next 24 hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 023, na základě 22 stanic.

Solární indexy za 14 Aug 2021

Wolfovo číslo Catania	///
10cm sluneční tok	073
AK Chambon La Forêt	010
AK Wingst	005
Odhadovaný Ap	004
Odhadovaný mezinárodní počet slunečních skvrn	018 - Na základě 30 stanic

Souhrn významných událostí

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

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