查看星期一, 25 8月 2014歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2014 Aug 25 1250 UTC

SIDC太陽影響數據分析中心的預報

太陽閃焰

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

地磁

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

太陽質子

Quiet

	10公分通量	Ap
25 Aug 2014	142	005
26 Aug 2014	142	014
27 Aug 2014	142	010

公告

The Sun produced several C-class flares and one isolated M-class flare. The C-class flares mainly originated from NOAA AR 2149. A partial halo CME was visible in SOHO/LASCO C2 imagery with first measurement on August 24 at 12:36 UT. The CME was also visible in Stereo B/COR2 images from 13:24 UT onwards. The CME is associated with a M6 flare peaking at 12:17 UT and a type II radio burst (shock speed estimated at 593 km/s by the San Vito station). NOAA AR 2151 is identified to be source region. The CME is propagating in the eastern direction from the Sun- Earth line with a projected line-of-sight speed of 473 km/s (CACTus estimate). Due to the position of the source region, the CME is not expected to have an Earth-directed component. Two filament eruptions occurred; one centered at S30E35 on August 24 at 13:29 UT and one centered at N15W15 lifting off on August 25 at 7:09 UT. No associated CMEs were identified so far. Flaring activity is expected to continue with C-class flares and potentially an M-class flare. Solar wind speed has decreased till 260 km/s currently. The amplitude of the interplanetary magnetic field ranged from 0 to 6 nT, with a varying Bz component. The phi angle was mostly negative (toward), but changed to positive (away) at 11:00 UT. Geomagnetic conditions were quiet to unsettled and are expected to remain so until the combined arrival of the August 22 CME's. This may potentially result in active geomagnetic conditions from the afternoon of August 26 onwards.

今日估計的國際太陽黑子數（ISN）：086，基於11個觀測站。

太陽活動指數 24 Aug 2014

卡塔尼亞沃爾夫數	///
10厘米太陽通量	141
AK Chambon La Forêt	004
AK Wingst	003
估計地磁Ap指數	002
估計國際太陽黑子數	104 - 基於22個觀測站

顯著活動摘要

由太陽影響數據分析中心提供© - SIDC - 由 SpaceWeatherLive處理

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