查看星期二, 22 11月 2022歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2022 Nov 22 1247 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 22 Nov 2022 到 24 Nov 2022 都有效
太陽閃焰

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
22 Nov 2022116006
23 Nov 2022117007
24 Nov 2022117006

公告

The strongest flare reported during last 24 hours was GOES C7.0 flare (peaked at 07:27 UT this morning). The source region of this flare was the newly emerged and fast developing NOAA AR 3151 (Catania group 5). Presently available coronagraph observations show only one image of the associated CME. More will be reported when the additional coronagraph data become available. We expect flaring activity at the C-class level in the coming hours, in particular from the NOAA AR 3151. The isolated M-class flares are still possible but not very probable. No other Earth-directed CMEs were detected in the available coronagraph observations over the past 24 hours.

During last 24 hours the greater than 10 MeV proton flux remained at the background level, and the greater than 2 MeV electron flux was bellow the threshold value of 1000 pfu. The 24h electron fluence is presently at normal level and we expect it will stay so in the coming 24 hours.

The solar wind speed is presently about 380 km/s and the interplanetary magnetic field magnitude is 4 nT. The solar wind originating from the small positive polarity coronal hole, that has rotated across the central meridian yesterday, might be expected at Earth on November 25. During last 24 hours the geomagnetic conditions were quiet and we expect such a geomagnetic conditions to persist in the coming hours.

今日估計的國際太陽黑子數(ISN):058,基於05個觀測站。

太陽活動指數 21 Nov 2022

卡塔尼亞沃爾夫數108
10厘米太陽通量117
AK Chambon La Forêt///
AK Wingst010
估計地磁Ap指數009
估計國際太陽黑子數072 - 基於16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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