Prohlížíte si archiv středa 18. prosince 2019

Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2019 Dec 18 1230 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
18 Dec 2019	071	020
19 Dec 2019	071	021
20 Dec 2019	071	017

Bulletin

Solar X ray flux remained below B level throughout the period. There are no active regions on disk and X-ray flux is expected to remain at background levels.

No Earth-directed CME's were detected in coronagraph images.

A small negative polarity equatorial coronal hole passed the central meridian overnight. It remains to be seen if it will have any influence on Solar wind conditions later in the week.

Solar high energy proton fluxes were at background levels and are expected to remain so.

Solar wind conditions showed the expected arrival of the high speed stream. Solar wind speed increased since midnight from just over 300 km/s to well over 500 km/s since. Total magnetic field reached a peak of 12nT with a Southward component of -10nT. Solar wind speed is expected to further increase, reaching over 600km/s and then level off by the end of the next 24 hour period before starting a slow and gentle decline.

Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Dourbes reached 3 just only in the 9-12UT period). Geomagnetic conditions are expected to be unsettled to active over the next day and will continue to be at least unsettled for the next days.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 000, na základě 14 stanic.

Solární indexy za 17 Dec 2019

Wolfovo číslo Catania	///
10cm sluneční tok	071
AK Chambon La Forêt	005
AK Wingst	002
Odhadovaný Ap	001
Odhadovaný mezinárodní počet slunečních skvrn	000 - Na základě 17 stanic

Souhrn významných událostí

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

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