查看星期五, 1 11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 Nov 01 1221 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 01 Nov 2013 到 03 Nov 2013 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
01 Nov 2013140009
02 Nov 2013140003
03 Nov 2013140006

公告

The sun produced one M and seven C flares during the past 24 hours. Catania sunspot region 18 (NOAA AR 11877) was responsible for the M1.9 flare peaking at 13:51 UT on October 31. Most C flares originated from Catania sunspot region 29 (NOAA AR 11884). During the next 48 hours, more C flaring activity is expected with a slight chance for an M flare, especially from Catania sunspot region 29 (NOAA AR 11884), which retains a beta-gamma-delta configuration of its photospheric magnetic field. LASCO/C2 (at 18:12 UT on October 31) and LASCO/C3 observed a mainly south directed CME, which will at most only produce a glancing blow. Due to the low speed (CACTus estimation 254 km/s), no effect on geomagnetic conditions is expected. Solar wind parameters observed by ACE indicated the arrival of a weak transient at 10:00 UTC on October 31, possibly related to the CME of 15:24 UT on October 28. A slight increase in solar wind speed, temperature and density was measured. The magnitude of the interplanetary magnetic field (IMF) went to 12 nT and is now stable around 5 nT. Current solar wind speed is around 350 km/s. Geomagnetic activity is quiet to unsettled (local K at Dourbes and NOAA Kp between 0 and 3), which is expected to remain so within the next 48 hours.

今日估計的國際太陽黑子數(ISN):085,基於08個觀測站。

太陽活動指數 31 Oct 2013

卡塔尼亞沃爾夫數138
10厘米太陽通量143
AK Chambon La Forêt013
AK Wingst008
估計地磁Ap指數007
估計國際太陽黑子數/// - 基於///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
31133613511402----M1.918/1877

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

所有時間均採用 UTC 時間

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