查看星期六, 8 6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 Jun 08 1247 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 08 Jun 2013 到 10 Jun 2013 都有效
太陽閃焰

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

地磁

Quiet (A<20 and K<4)

太陽質子

Quiet

10公分通量Ap
08 Jun 2013109013
09 Jun 2013108011
10 Jun 2013106008

公告

Solar activity is low, with only three C-class flares and one M-class flare detected in last 24 hours. The M5.9 flare peaking at 22:49 UT on June 07 originated from the Catania sunspot group 96 (NOAA AR 1765) situated at that moment at the west solar limb, and was associated with a CME. From the currently available data it seems that the bulk of the CME mass was directed mostly southward of the Sun-Earth line and it is therefore not probable that the CME will arrive at the Earth. Fast growing Catania sunspot group 96 (NOAA AR 1765) which currently has beta-gamma configurations of its photospheric magnetic field, has a significant potential to produce a C-class flares, and possibly also M-class flares. The interplanetary magnetic field magnitude is about 4 nT, and the solar wind speed is currently 450 km/s. The arrival of the fast flow from the small equatorial coronal hole is expected today without significant geomagnetic impact. A CME-driven shock wave associated with the M1.3 flare on June 05, might be expected on June 09 producing at most unsettled geomagnetic conditions. We expect quiet to unsettled geomagnetic conditions during following 48 hours.

今日估計的國際太陽黑子數(ISN):017,基於16個觀測站。

太陽活動指數 07 Jun 2013

卡塔尼亞沃爾夫數066
10厘米太陽通量110
AK Chambon La Forêt021
AK Wingst025
估計地磁Ap指數033
估計國際太陽黑子數032 - 基於21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
07221122492304----M5.992/1762VI/1

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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