Przeglądasz Archiwum z środa, 24 września 2014

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2014 Sep 24 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
24 Sep 2014	142	016
25 Sep 2014	146	011
26 Sep 2014	150	010

Skrót wiadomości

Solar flaring activity has been moderate. An isolated M2.3 flare was produced by NOAA AR 2172 peaking at 23:16 UT. It was associated with a dimming as well as type II radio burst detections (Learmonth estimated shock speed 790-1250 km/s). A corresponding CME observed by STEREO B COR2 departing the west limb (as seen from STEREO B) does not appear to be fast nor very wide. SOHO/LASCO data for the relevant time slot just became available and records the CME in C2 data from midnight onwards. This imagery confirms the small angular width (roughly about 120 degrees) and indicates a primary direction towards the east. With the small recorded speeds (plane of the sky projected speed around 300 km/s) even a glancing blow seems unlikely. With background Xray flux around the B6 level and NOAA AR 2171 the only significant potential flaring source we expect flaring at C-level although their is a fair chance for another M flare from this region as it continues to evolve and grow in size. Another asymmetric halo CME was detected with first appearance in SOHO/LASCO coronagraph images at 19:00 UT, for which Cactus has sent out a corresponding alert. Despite a data gap in STEREO B EUVI 193 data between 18:16UT and 21:26 UT the start of the eruption (from the same active region as the previous two partial/asymmetric halo CME's) was recorded just before the data gap, as well as the post flare loops just after the data gap. The event is thus judged to be backsided. Solar wind speed dropped further during the first half of the reporting period to a minimum of close to 370 km/s around 19:00 UT. It increased afterwards to around 420 km/s presently. The total magnetic field slightly increased to above the 7 nT level with periods of Bt 8nT and negative BZ around -7nT. Unsettled to active geomagnetic conditions have been recorded (NOAA Kp 3-4, local hourly K Dourbes 1-4). Similar solar wind conditions and quiet to unsettled geomagnetic conditions with possible active periods are expected to continue over the next days.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 076, na podstawie 08 stacji.

Indeksy solarne na 23 Sep 2014

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	138
AK Chambon La Forêt	021
AK Wingst	014
Szacunkowa Ap	014
Szacowana międzynarodowa liczba plam słonecznych	088 - Na podstawie stacji 23

Podsumowanie wydarzeń godnych uwagi

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

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