Przeglądasz Archiwum z czwartek, 25 września 2014

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2014 Sep 25 1232 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

Quiet (A<20 and K<4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
25 Sep 2014	150	013
26 Sep 2014	155	016
27 Sep 2014	160	010

Skrót wiadomości

Solar activity has been low, with just a couple of C flares. The strongest one originating, as expected, from NOAA AR 2172, peaking at 17:50 UT at C7 level. A new region (NOAA unnumbered) has emerged with current location near N15W00 developing fast both in size and complexity. This region certainly adds to the expected C flaring from NOAA AR 2172 as well as to the M flare potential. We thus expect flaring on the C level with the chance for M flares increasing further, depending on the new region development. With the filament situated closely to the west of the new region, further development of this region may also lead to the destabilization and eruption of that filament in the following days. An asymmetric halo CME is visible in SOHO/LASCO C2 coronagraph images from 21:12 UT onwards. It is primarily directed northward. Despite the main eruption taking place within a data gap, STEREO B/EUVI 195 images indicate that the eruption originated from NOAA AR 2158. The event is thus backsided and very similar to the September 22, 6:25UT event. Solar wind speed rose slightly from about 420 km/s to around 450 km/s. After reaching a peak of 8.5 nT around 18:00 UT total magnetic field decreased to around 6.5 nT currently. Bz reached negative peaks of over -7nT around 18:00 UT but is currently within a more restricted range of about +-4nT. Unsettled geomagnetic conditions with active periods have been recorded over the reporting period (NOAA Kp as well as local K Dourbes 3-4) settling locally to quiet conditions more recently (local K Dourbes 1-2 after 3:00 UT). Solar wind conditions are expected to remain slightly enhanced over the next days with periods of active geomagnetic conditions possible.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 103, na podstawie 17 stacji.

Indeksy solarne na 24 Sep 2014

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	145
AK Chambon La Forêt	032
AK Wingst	024
Szacunkowa Ap	026
Szacowana międzynarodowa liczba plam słonecznych	073 - Na podstawie stacji 17

Podsumowanie wydarzeń godnych uwagi

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

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