Prohlížíte si archiv čtvrtek 30. května 2019

Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2019 May 30 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
30 May 2019	069	013
31 May 2019	069	010
01 Jun 2019	070	007

Bulletin

The solar activity has been quiet over the past 24 hours. The X-ray flux remains below B-level, and the visible solar disc is spotless. Solar activity is expected to remain at low levels over the next 24 hours.

No Earth directed Coronal Mass Ejection (CME) has been detected in the available coronagraph imagery. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.

The Earth is under the influence of the solar wind associated with the negative polarity equatorial coronal hole which began to traverse the central meridian on May 24. The solar wind speed was around the values of about 505 and 566 km/s. The interplanetary magnetic field slowly decreased and is now below 5 nT, and the southward component fluctuated between -6 nT and +5 nT. The solar wind parameters are expected to remain enhanced today and tomorrow.

The geomagnetic conditions have been mostly unsettled with Kp index (NOAA) and local K index (Dourbes) ranging between 1 and 3. Active conditions with intervals of K-Dourbes = 4 remained possible although not very likely today and tomorrow, due to the high-speed solar wind stream associated negative polarity equatorial coronal hole.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 000, na základě 20 stanic.

Solární indexy za 29 May 2019

Wolfovo číslo Catania	///
10cm sluneční tok	068
AK Chambon La Forêt	019
AK Wingst	018
Odhadovaný Ap	019
Odhadovaný mezinárodní počet slunečních skvrn	013 - Na základě 16 stanic

Souhrn významných událostí

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

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