Vaata kolmapäev, 17 juuni 2020 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2020 Jun 17 1231 UTC

SIDC ennustus

Päikesepursked ehk loited

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

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

	10 cm vool	Ap
17 Jun 2020	069	011
18 Jun 2020	069	008
19 Jun 2020	069	007

Bülletään

There is no active region on the visible Sun. No B or brighter flares in the past 24 hours, none expected.

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

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.

Solar wind speed near Earth has remained at around 330 km/s in the past 24 hours. The periods of high speed observed yesterday by DSCOVR were not real, there was a problem with the data. The Interplanetary Magnetic Field is at about 5 nT.

Quiet to unsettled geomagnetic conditions were observed locally (K Dourbes between 0 and 3) and Kp ranged between 0 and 2 in the past 24 hours. Unsettled to active periods could occur in the coming 24 hours, due to high speed solar wind effects, although the faint/patchy nature of the coronal hole at the Sun may indicate that there will be no observable effect at the Earth.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 000, põhineb 17 jaamadel.

Päikese indeksid 16 Jun 2020

Catania Wolfi number	000
10cm päikesevoog	069
AK Chambon La Forêt	011
AK Wingst	009
Hinnanguline Ap	006
Hinnanguline rahvusvaheline päikeselaikude arv	000 - Põhineb 26 jaamal

Märkimisväärsete sündmuste kokkuvõte

Andmed on esitanud Päikeseinfektide Andmeanalüüsi Keskus (Solar Influences Data Analysis Center)© - SIDC - Töötleb SpaceWeatherLive

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