查看星期六, 16 10月 2021歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2021 Oct 16 1231 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 16 Oct 2021 到 18 Oct 2021 都有效
太陽閃焰

C-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 Oct 2021082012
17 Oct 2021082010
18 Oct 2021082016

公告

Region NOAA 2885 produced a B9.7 flare peaking at 15:16 UT on October 15. The chance for a C flare in the next 24 hours is estimated at 50%, especially from region 2885.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.

DSCOVR registered a fast forward shock in the solar wind at 00:12 UT on October 16. The solar wind speed jumped from about 300 to 345 km/s, while the magnitude of the Interplanetary Field (IMF) jumped from about 6 to 8 nT and the density jumped from about 4.5 to 6.5 counts/cc. The IMF orientation stayed predominantly towards the Sun. This probably corresponds to the Corotating Interaction Region (CIR) in front of the high speed stream from a negative polarity equatorial coronal hole. Current solar wind speed values are near 400 km/s, and current values for the magnitude of the IMF are about 9 nT. There were no extended time intervals in which Bz was below -5 nT. Enhanced solar wind conditions are expected on October 16, with a gradual return to nominal levels on October 17 and the first half of October 18. In the second half of October 18, a high speed stream from a positive polarity coronal hole is expected to arrive near Earth, which will likely lead to enhanced solar wind levels.

Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 0 and 2) were registered in the past 24 hours. On October 16, active intervals (K Dourbes = 4) are possible, with a slight chance for minor storm intervals (K Dourbes = 5). Quiet to unsettled geomagnetic levels are expected on October 17 and the first half of October 18. In the second half of October 18, active intervals are possible due to the expected arrival of a high speed stream from a positive polarity coronal hole, with a slight chance for minor storm intervals.

今日估計的國際太陽黑子數(ISN):011,基於22個觀測站。

太陽活動指數 15 Oct 2021

卡塔尼亞沃爾夫數011
10厘米太陽通量084
AK Chambon La Forêt///
AK Wingst///
估計地磁Ap指數///
估計國際太陽黑子數011 - 基於30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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