查看星期日, 27 10月 2013歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2013 Oct 27 1205 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 27 Oct 2013 到 29 Oct 2013 都有效
太陽閃焰

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

地磁

Minor storm expected (A>=30 or K=5)

太陽質子

Quiet

10公分通量Ap
27 Oct 2013158006
28 Oct 2013160023
29 Oct 2013159023

公告

There were two M flares and eleven C flares on the Sun in the past 24 hours. New region NOAA AR 11884 in the East produced an M3.1 flare peaking at 19:27 UT on October 26 while beta-gamma-delta region AR 11882 released an M1.0 flare peaking at 19:53 UT on October 26. The other flares were produced by AR 11882, 11875, 11877 and 11873. In the next 48 hours, M flares are expected, with a chance for X flares. LASCO C2 and STEREO COR2 A and B observed several CMEs on October 26 and 27, among which a partial halo CME first registered by LASCO C2 at 11:24 UT on October 26 (associated with the M1.8 flare of 11:17 UT). This CME could deliver a glancing blow in the second half of October 29. ACE observed a jump in the solar wind at 21:44 UT on October 26. Solar wind speed jumped from about 280 to 310 km/s, while the Interplanetary Magnetic Field jumped from 4.5 to 6.5 nT. A smooth decrease in the phi angle clearly shows rotation of the Interplanetary Magnetic Field consistent with the flux rope of an ICME. This jump was probably the result of the arrival of the October 22 (M4.2) CME. Phi jumped from 110 to 270 degrees around 9h UT on October 27, probably indicating the end of the (weak) ICME influence and return to nominal conditions, with solar wind speed around 270 km/s and Interplanetary Magnetic Field around 2 nT. Geomagnetic activity was at quiet levels (K Dourbes between 0 and 2; NOAA Kp between 0 and 1) during the past 24 hours. Quiet geomagnetic conditions (K Dourbes < 4) are expected for the second half of October 27 and the first half of October 28. Active conditions with minor storm intervals are possible on the second half of October 28 and the first half of October 29, due to the expected joint arrival of several CMEs, mainly from October 25. Active geomagnetic levels are possible in the second half of October 29, due to a possible glancing blow by the partial halo CME of October 26.

今日估計的國際太陽黑子數(ISN):099,基於13個觀測站。

太陽活動指數 26 Oct 2013

卡塔尼亞沃爾夫數///
10厘米太陽通量165
AK Chambon La Forêt005
AK Wingst002
估計地磁Ap指數001
估計國際太陽黑子數090 - 基於20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
26104811171134S05E58M1.81N38023/1882
26192419271930S09E81M3.1SF--/1884
26194919531958S07E53M1.0SF23/1882

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

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