查看星期日, 16 3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 Mar 16 1228 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 16 Mar 2014 到 18 Mar 2014 都有效
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
16 Mar 2014141006
17 Mar 2014141018
18 Mar 2014141008

公告

There were five C flares on the Sun during the past 24 hours, released by NOAA AR 12003, 12005, and 11998. The brightest flare was a C7.3 flare produced by AR 12003 peaking at 06:45 UT on March 16. In the next 48 hours, the probability for C flares is high (over 90%) and for M flares around 55%, mainly from AR 12003 and returning region AR 11986. CACTUS detected a CME on LASCO C2 and C3 images starting at 3:36 UT on March 16. This CME was also observed by the coronagraphs COR2 A and COR2 B, and is most probably related to the filament eruption that took place around 02:54 UT near 25S45E. This CME will probably not be geoeffective. In the past 24 hours, solar wind speed as observed by ACE varied between about 360 and 410 km/s, while the magnitude of the Interplanetary Magnetic Field (IMF) fluctuated between about 1.5 and 4.5 nT. In the past 24 hours, quiet geomagnetic levels were registered (K Dourbes between 0 and 2; NOAA Kp between 0 and 1). Quiet geomagnetic conditions (K Dourbes < 4) are expected on March 16. Quiet to active conditions (K Dourbes < 5) are possible on March 17 and 18, due to a coronal hole high speed stream.

今日估計的國際太陽黑子數(ISN):087,基於15個觀測站。

太陽活動指數 15 Mar 2014

卡塔尼亞沃爾夫數///
10厘米太陽通量139
AK Chambon La Forêt007
AK Wingst005
估計地磁Ap指數004
估計國際太陽黑子數079 - 基於17個觀測站

顯著活動摘要

開始最大值結束位置強度OP10cm卡塔尼亞天體物理觀測站/美國國家海洋暨大氣管理局電波爆發類型

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

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