查看星期一, 10 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 10 1247 UTC

SIDC太陽影響數據分析中心的預報

太陽閃焰

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

地磁

Quiet (A<20 and K<4)

太陽質子

Warning condition (activity levels expected to increase, but no numeric forecast given)

	10公分通量	Ap
10 Nov 2025	173	007
11 Nov 2025	173	007
12 Nov 2025	173	023

太陽活動區和耀斑

Solar flaring activity was high over the past 24 hours, with one X-class flare and several C-class flares. The largest was an X1.2 event (SIDC Flare 6010) that peaked on 10 November at 09:19 UTC, produced by SIDC Sunspot Group 687 (NOAA Active Region 4274) at N24W15. Eight numbered sunspot groups were present on the disk. SIDC Sunspot Group 687 (NOAA 4274) is the largest and most magnetically complex region on the disk (Beta-Gamma-Delta; McIntosh Ekc) and remained the primary source of significant activity, producing the X-class and multiple C-class flares. SIDC Sunspot Groups 689 (NOAA Active Region 4276) and 690 (NOAA Active Region 4277), both with Beta magnetic configurations, produced several C-class flares and have been decreasing over the past 24 hours. Solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares very likely and a small chance of X-class flares.

日冕物質拋射

No Earth-directed coronal mass ejection (CME) has been identified in the currently available coronagraph imagery. However, the X1.2 flare (SIDC Flare 6010) that peaked at 09:19 UTC from SIDC Sunspot Group 687 (NOAA AR 4274) showed Type IV radio emission, a signature often linked to major eruptions and strong CMEs. An Earth-directed component is therefore plausible, pending confirmation from ongoing coronagraph analysis.

日冕洞

SIDC Coronal Hole 126, an equatorial coronal hole with negative polarity, has reappeared on the disk and is currently situated on the western side of the Sun.

太陽風

Over the past 24 hours the flow was variable and the speed remained moderately elevated, ranging from 455 to 595 km/s. The total interplanetary magnetic field stayed below 8 nT, with Bz component of the interplanetary magnetic was between +7 and -6 nT, including several southward intervals near -6 nT. The phi angle fluctuated between the negative sector (toward the Sun) and the positive sector. Over the next 48 hours conditions are expected to become disturbed due to a possible glancing blow from the coronal mass ejection (SIDC CME 597), which left the Sun on 07 November around 12:48 UTC, followed shortly after, or possibly around the same time, by the arrival of the Earth-directed coronal mass ejection (SIDC CME 598) associated with the X1.8 flare, with an estimated arrival near 07:12 UTC on 12 November.

地磁

Global conditions were quiet to unsettled. NOAA Kp briefly reached 3, and the Belgian K index peaked at 3 before easing to 1-2 later this morning UTC. Over the next 24 hours, quiet to unsettled levels are most likely, with isolated short-lived active intervals possible if Bz turns persistently southward. Additional disturbances remain possible around 12 November from a glancing blow of coronal mass ejection (SIDC CME 597, launched 07 Nov around 12:48 UTC) and the potential arrival of the Earth-directed coronal mass ejection (SIDC CME 598) associated with the X1.8 flare, with an estimated arrival near 07:12 UTC on 12 November.

質子通量水平

The greater than 10 MeV GOES proton flux stayed at background until about 09:40 UTC, then rose promptly following the X1.2 flare from SIDC Sunspot Group 687 at 09:19 UTC. It reached event levels shortly after 10:00 UTC and was still increasing at the time of writing.

地球靜止軌道上的電子通量

The GOES-18 >2 MeV electron flux remained below the 1000 pfu threshold throughout the period. The 24-hour fluence is at normal levels and is expected to stay mostly normal over the next 24 hours, with only brief enhancements possible if the solar wind strengthens ahead of the anticipated CME influences on 11–12 Nov.

今日估計的國際太陽黑子數（ISN）：160，基於13個觀測站。

太陽活動指數 09 Nov 2025

卡塔尼亞沃爾夫數	///
10厘米太陽通量	176
AK Chambon La Forêt	013
AK Wingst	006
估計地磁Ap指數	007
估計國際太陽黑子數	164 - 基於23個觀測站

顯著活動摘要

由太陽影響數據分析中心提供© - SIDC - 由 SpaceWeatherLive處理

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