Przeglądasz Archiwum z środa, 28 lutego 2018

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2018 Feb 28 1232 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

Quiet (A<20 and K<4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
28 Feb 2018	069	009
01 Mar 2018	069	006
02 Mar 2018	068	009

Skrót wiadomości

Solar activity remains to be low, without even B-class flares reported during last 24 hours. Occasional B-class flares are possible in the coming hours, and isolated C-class flares are possible but not very probable. The low level flaring from the Catania sunspot group 73 (NOAA AR 2700) observed this morning was associated with coronal dimming and EIT wave, i.e. on disc signature of the coronal mass ejection (CME). More will be reported when coronagraph data become available, however it is very probable that the CME was rather narrow and slow and it will therefore not arrive to the Earth. During last 24 hours solar protons remained at background level.

Solar wind speed is presently about 430 km/s and the interplanetary magnetic field magnitude is about 5 nT. The solar wind flow, associated with the equatorial coronal hole that reached central meridian in February 22, reached its maximum value of about 560 km/s on February 27 at about 15:30 UT. The fast solar wind associated with rather small and patchy equatorial coronal hole which reached central meridian in the morning of February 26 might be expected to arrive to the Earth in the morning of March 02. Due to fast solar wind and longer intervals of negative value of the Bz component of the interplanetary magnetic field disturbed geomagnetic conditions were reported around midday yesterday (NOAA reported Kp=4 and local station at Dourbes reported K=4). Presently geomagnetic conditions are quiet to unsettled and we expect them to stay so in the coming hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 012, na podstawie 21 stacji.

Indeksy solarne na 27 Feb 2018

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	068
AK Chambon La Forêt	016
AK Wingst	021
Szacunkowa Ap	021
Szacowana międzynarodowa liczba plam słonecznych	017 - Na podstawie stacji 31

Podsumowanie wydarzeń godnych uwagi

Dostarczone przez Centrum Analizy Danych Wpływów Słonecznych© - SIDC - Przetworzone przez SpaceWeatherLive

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