查看星期一, 27 9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 Sep 27 1231 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 27 Sep 2021 到 29 Sep 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
27 Sep 2021086007
28 Sep 2021086007
29 Sep 2021086007

公告

Four active regions (ARs) present on the visible solar disk. No flares above the B-class level in the past 24 hours. Over the next 24 hours, C-class flares can be expected, in particular from NOAA AR 2871 which has a beta-gamma magnetic field configuration (the other 3 ARs have a beta magnetic field configuration).

No Earth directed CMEs have been observed in coronagraph data in the last 24 hours.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay there in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold. Over the next 24 hours, it is expected to remain below the threshold. The electron fluence was at normal levels over the past 24 hours, and is expected to remain so for the next 24 hours.

Over the past 24 hours the solar wind speed has been around 400 km/s. The total magnetic field strength had reached 11 nT, while its Bz component reached -6 nT. This slightly elevated magnetic field, together with low temperature plasma, could mark the expected arrival of the ICMEs from 23 and 24 September. Due to the low speeds and mostly positive Bz, the effect is very mild, the situation may change in the coming hours since more than one ICME was expected.

Geomagnetic conditions were quiet to unsettled (NOAA Kp and K Dourbes 1-3) over the past 24 hours. Active periods can be expected over the next 24 hours.

今日估計的國際太陽黑子數(ISN):049,基於10個觀測站。

太陽活動指數 26 Sep 2021

卡塔尼亞沃爾夫數///
10厘米太陽通量086
AK Chambon La Forêt006
AK Wingst002
估計地磁Ap指數001
估計國際太陽黑子數048 - 基於26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

所有時間均採用 UTC 時間

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