Przeglądasz Archiwum z czwartek, 31 grudnia 2015

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2015 Dec 31 1230 UTC

Prognoza SIDC

Rozbłyski słoneczne

C-class flares expected, (probability >=50%)

Geomagnetyzm

Active conditions expected (A>=20 or K=4)

Monitoring przepływu protonów

Warning condition (activity levels expected to increase, but no numeric forecast given)

	strumień 10cm	Ap
31 Dec 2015	100	049
01 Jan 2016	102	031
02 Jan 2016	105	024

Skrót wiadomości

Solar activity was low. The only prominent region on disk, NOAA 2473, showed decay and produced the only 2 C flares of the period of which the strongest a C4.3 flare peaking at 22:45UT. NOAA AR 2473 continued to show decay, especially in the trailing spots. Flaring at C level is expected with only a slight chance for an M flare from NOAA AR 2473. No Earth directed CMEs have been recorded. The >10MeV have recovered to nominal values with a slight chance for a proton event remaining, associated with possible activity from region 2473. Solar wind conditions remained nominal until midnight when at 00:02UT a shock occurred in ACE solar wind data, marking the arrival of the December 28 CME. Total interplanetary magnetic field jumped from 6nT to 13nT while solar wind speed jumped from 340km/s to 400 km/s. Solar wind speed kept increasing to a peak of around 500 km/s and is currently at around 460 km/s. Total magnetic field was in the 9-16nT range but Bz was initially variable and remained above -10nT. More recently, stronger and more pronounced negative peaks down to -13nT are recorded. Solar wind conditions are expected to remain enhanced over the next days in the wake of the CME today and into a sector boundary crossing with later the possible high speed stream influence from the low latitude extension of the (positive polarity) northern polar coronal hole. Only up to active geomagnetic conditions have been reported so far (both NOAA Kp and local K Dourbes reached 4). Subject to the evolution of the magnetic field and its Bz component minor to major geomagnetic storming conditions remain possible in the wake of the CME later easing to possible isolated active periods.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 019, na podstawie 17 stacji.

Indeksy solarne na 30 Dec 2015

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	102
AK Chambon La Forêt	012
AK Wingst	004
Szacunkowa Ap	003
Szacowana międzynarodowa liczba plam słonecznych	030 - Na podstawie stacji 30

Podsumowanie wydarzeń godnych uwagi

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

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