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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2020 May 10 1231 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
10 May 2020	069	004
11 May 2020	069	010
12 May 2020	069	007

Bulletin

The solar activity was quiet over the past 24 hours. No sunspot is visible on the solar disc facing Earth. The X-ray flux is below B-class level and the solar activity is expected to remain at low levels.

No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery in the last 24 hours.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux was between nominal and moderate levels over the past 24 hours and is expected to remain at nominal to moderate levels over the next 24 hours.

The Earth is under the influence of the slow solar wind streams. The solar wind parameters (DSCOVR) was at nominal values with the solar wind speed around 283-328 km/s. The total interplanetary magnetic field was below 5.2 nT. The Bz magnetic field components fluctuated between -2.5 nT and +3.9 nT. The solar wind regime is expected to remain mostly slow for the next days. Very mild enhancements of the solar wind conditions may occur today in response to the influence of the fast solar wind associated with the elongated extension of the southern polar coronal hole (negative polarity) that was facing Earth on May 6.

Geomagnetic conditions were quiet, and quiet conditions are expected for the next following day. In response to the mild influence of the fast solar wind streams associated with the south polar coronal hole extension, periods of unsettled conditions may occur in today and tomorrow.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 000, na základě 13 stanic.

Solární indexy za 09 May 2020

Wolfovo číslo Catania	///
10cm sluneční tok	071
AK Chambon La Forêt	005
AK Wingst	002
Odhadovaný Ap	002
Odhadovaný mezinárodní počet slunečních skvrn	000 - Na základě 30 stanic

Souhrn významných událostí

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

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