查看星期二, 2 9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 Sep 02 1232 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

Moderate (ISES: Major) magstorm expected (A>=50 or K=6)

太陽質子

Quiet

10公分通量Ap
02 Sep 2025190029
03 Sep 2025185031
04 Sep 2025181017

太陽活動區和耀斑

Solar flaring activity was low over the past 24 hours, with only C-class flares identified. The largest flare was a C3.9 flare (SIDC Flare 5405) peaking on September 01 at 19:22 UTC, which was produced by SIDC Sunspot Group 614 (NOAA Active Region 4197). A total of 13 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 614 (NOAA Active Region 4197) is the largest region on disk, has a Beta-Gamma magnetic configuration and produced most of the flaring activity in the last 24 hours. Solar flaring activity is expected to be moderate over the next 24 hours, with C-class flares expected and M-class flares likely.

日冕物質拋射

No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.

日冕洞

SIDC Coronal Hole 123 (equatorial coronal hole with a positive polarity) started crossing the central meridian on September 02, its associated high-speed stream is expected to arrive at Earth on September 05. (Other crossing times: August 06)

太陽風

Over the past 24 hours, the solar wind conditions at Earth have become disturbed, due to the arrival of an ICME that left the Sun on August 30 at 20:12 UTC. The solar wind speed jumped from 377 km/s to 676 km/s, the total interplanetary magnetic field jumped from 5 nT to 26 nT and the solar wind density jumped from 3 ppcc to around 10 ppcc on September 01 at 20:20 UTC. Over the entire period, the Bz reached a minimum value of -23 nT. At the end of the period, the total interplanetary magnetic field remains elevated around 19 nT and the solar wind speed has a value around 550 km/s The solar wind conditions are expected to remain disturbed in the next 24, due to the ongoing ICME passage.

地磁

The geomagnetic conditions over the past 24 hours reached moderate storm conditions globally (Kp 6) and minor storm conditions locally (K BEL 5). For the next 24 hours, major storm conditions can be expected if Bz turns negative.

質子通量水平

Over the past 24 hours, the greater than 10 MeV GOES proton flux decreased and is expected to return to background levels in the next 24 hours.

地球靜止軌道上的電子通量

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

今日估計的國際太陽黑子數(ISN):175,基於18個觀測站。

太陽活動指數 01 Sep 2025

卡塔尼亞沃爾夫數198
10厘米太陽通量202
AK Chambon La Forêt036
AK Wingst018
估計地磁Ap指數016
估計國際太陽黑子數186 - 基於19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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