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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2016 Mar 02 1230 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
02 Mar 2016	097	008
03 Mar 2016	096	008
04 Mar 2016	094	008

Skrót wiadomości

The strongest flare reported in the last 24 hours was the B3.4 flare (peaked at 17:57 UT on March 1), which originated from the Catania sunspot group 27 (NOAA 2506). Although the probability for the C-class flares is low (about 20%) they are still possible, in particular from the unnamed active region which just rotated from the behind of the East solar limb. The prominence eruption was observed at about 08:00 UT on March 1, with the source region close to the East solar limb. The prominence eruption was associated with rather slow CME (speed reported by the CACTUS software is about 500 km/s) with angular width of about 115 degrees. No Earth directed CMEs were observed in the last 24 hours. The solar wind speed has increased and its current value is about 450 km/s, the interplanetary magnetic field magnitude is about 10 nT. The small equatorial corona hole has reached the central meridian this morning. The associated fast solar wind can be expected on Marc 5. The geomagnetic conditions are quiet to unsettled. Currently the Bz component of the interplanetary magnetic field is positive however if the Bz component turns negative we can expect unsettled to active conditions in the coming hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 069, na podstawie 18 stacji.

Indeksy solarne na 01 Mar 2016

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	097
AK Chambon La Forêt	014
AK Wingst	010
Szacunkowa Ap	009
Szacowana międzynarodowa liczba plam słonecznych	063 - Na podstawie stacji 15

Podsumowanie wydarzeń godnych uwagi

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

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