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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2019 Jan 24 1231 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
24 Jan 2019	073	016
25 Jan 2019	073	008
26 Jan 2019	072	006

Bulletin

There is presently only one sunspot group observed on the visible side of the Sun. NOAA AR 2733 still has beta configuration of its photospheric magnetic field and is occasionally producing low B-class flares. We expect low solar flaring activity to persist in the coming hours, with the low probability for an isolated C-class flare. There were no Earth directed CMEs reported during last 24 hours and the solar protons remained at the background level.

The Earth is presently inside the fast solar wind (originating from the equatorial coronal hole which reached central meridian in the morning of January 19) with the speed of about 600 km/s and the interplanetary magnetic field magnitude of 8 nT. Several intervals of longer negative value of the Bz component of the interplanetary magnetic field and the fast solar wind induced disturbed geomagnetic conditions. Around the midnight and early morning of January 24 local station at Dourbes and NOAA reported K=4 and Kp=4, respectively. As the solar wind speed is rather high, although the interplanetary magnetic field magnitude already significantly decreased, we still might expect unsettled to active geomagnetic conditions in the coming hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 022, na základě 09 stanic.

Solární indexy za 23 Jan 2019

Wolfovo číslo Catania	///
10cm sluneční tok	072
AK Chambon La Forêt	025
AK Wingst	017
Odhadovaný Ap	016
Odhadovaný mezinárodní počet slunečních skvrn	020 - Na základě 20 stanic

Souhrn významných událostí

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

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