查看星期一, 24 11月 2025歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2025 Nov 24 1231 UTC

SIDC太陽影響數據分析中心的預報

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
24 Nov 2025121026
25 Nov 2025121031
26 Nov 2025121017

太陽活動區和耀斑

Solar flaring activity was low over the past 24 hours, with several C-class flares recorded. The largest flare was a C2.5 flare (SIDC Flare 6189), peaking on November 24 at 06:18 UTC, associated with SIDC Sunspot Group 705 (NOAA Active Region 4290; magnetic type beta). There are currently seven numbered active regions on the visible solar disk. SIDC Sunspot Group 705 was the main driver of the flaring activity observed over the past 24 hours. A new region rotated on the disk from behind the east limb and was numbered SIDC Sunspot Group 708 (NOAA Active Region 4293; magnetic type beta), but it remained quiet. The remaining active regions did not produce any significant flaring activity. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.

日冕物質拋射

No Earth-directed coronal mass ejections (CMEs) have been identified in the available coronagraph imagery over the past 24 hours.

太陽風

Over the past 24 hours, the solar wind parameters (ACE and DSCOVR) became slightly disturbed, possibly due to arrival of a high-speed stream from a positive polarity coronal hole (SIDC Coronal Hole 128). The interplanetary magnetic field reaching values up to 15 nT. The solar wind speed increased from 430 to 710 km/s. The southward component of the interplanetary magnetic field fluctuated between -15 nT and 11 nT. Solar wind conditions are expected to remain slightly elevated over the next days under the influence of a high-speed stream (HSS).

地磁

Geomagnetic conditions reached active levels globally (NOAA Kp 4-), between 15:00 and 18:00 UTC on November 23. Locally over Belgium quiet to unsettled conditions were observed (K-Bel: 1 to 3). Mostly unsettled to active geomagnetic conditions are expected over the next 24 hours, with a chance of isolated minor or moderate storm periods due to the ongoing high-speed stream influence.

質子通量水平

Over the past 24 hours the greater than 10 MeV GOES proton flux has been at nominal levels and is expected to remain at nominal levels over the next days.

地球靜止軌道上的電子通量

The greater than 2 MeV electron flux measured by GOES 18 and GOES 19 was below the 1000 pfu threshold. The greater than 2 MeV electron flux is expected to remain below the 1000 pfu threshold over the next 24 hours. The 24-hour electron fluence was at normal levels and is expected to be at normal levels over the next 24 hours.

今日估計的國際太陽黑子數(ISN):102,基於09個觀測站。

太陽活動指數 23 Nov 2025

卡塔尼亞沃爾夫數///
10厘米太陽通量120
AK Chambon La Forêt026
AK Wingst018
估計地磁Ap指數016
估計國際太陽黑子數080 - 基於10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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