查看星期一, 13 10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 Oct 13 1302 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 13 Oct 2014 到 15 Oct 2014 都有效
太陽閃焰

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

地磁

Quiet (A<20 and K<4)

太陽質子

Quiet

10公分通量Ap
13 Oct 2014113006
14 Oct 2014113011
15 Oct 2014113007

公告

There are only two sunspot groups currently visible on the solar disk, and no C flares occurred during the past 24 hours. In the next 48 hours, eruptive conditions (C flaring) are possible, especially from beta region NOAA AR 2187. A bright CME was first seen in the SOHO LASCO C2 field of view at 00:00 UT on October 13. It had an angular width of about 90 degrees and is probably associated with an eruption in a backside region close to the west limb. This CME is not expected to be geoeffective. Over the last 24 hours, solar wind speed observed by ACE was low and fluctuated between about 310 and 340 km/s. The magnitude of the Interplanetary Magnetic Field (IMF) first varied between 4 and 8.5 nT, and jumped from 5.5 to 9 nT around 5:45 UT on October 13, possibly due to an unidentified ICME structure. Over the past 24 hours, geomagnetic conditions were quiet (K Dourbes between 1 and 3; NOAA Kp between 1 and 2). Quiet geomagnetic levels (K Dourbes < 4) are expected on October 13, 14 and 15, with a slight chance for active levels (K Dourbes = 4) in the early hours of October 14 in case the glancing blow of the CME from October 10 encounters the Earth.

今日估計的國際太陽黑子數(ISN):031,基於10個觀測站。

太陽活動指數 12 Oct 2014

卡塔尼亞沃爾夫數///
10厘米太陽通量111
AK Chambon La Forêt008
AK Wingst002
估計地磁Ap指數002
估計國際太陽黑子數021 - 基於15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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