查看星期六, 3 1月 2026歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2026 Jan 03 1238 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

Minor storm expected (A>=30 or K=5)

太陽質子

Quiet

10公分通量Ap
03 Jan 2026164020
04 Jan 2026164017
05 Jan 2026162032

太陽活動區和耀斑

Solar flaring activity was low over the past 24 hours. The largest flare was a C2.9 flare (SIDC Flare 6567) peaking on January 03 at 01:37 UTC, which was produced by SIDC Sunspot Group 744 (NOAA Active Region 4324). This region has reduced in size over the period and has Beta-Delta magnetic configuration. There are currently 8 numbered regions on the disk. SIDC Sunspot Group 745 (NOAA Active Region 4325, Beta configuration) is the largest region on disk and also produced low level C-class flares, but became less complex magnetically. SIDC Sunspot Group 709 (NOAA Active Region 4323) developed into a bipolar region (beta magnetic configuration). A new region emerged in the south-west quadrant and was numbered SIDC Sunspot Group 753 (alpha magnetic configuration). SIDC Sunspot Group 749 (NOAA Active Region 4331) decayed over the period. The remaining regions are simple and mostly quiet or in decay. Solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares expected and a chance for X-class flares.

日冕物質拋射

No new Earth-directed Coronal Mass Ejection (CMEs) were observed in the available coronagraph imagery.

太陽風

Over the past 24 hours, the solar wind parameters were enhanced. It is unclear if this is due to the ongoing high speed stream or in combination with an earlier than expected weak glancing blow CME arrival of the CME of January 31. The solar wind speed ranged between 500 and 700 km/s. The total magnetic field ranged between 2 and 10 nT, and Bz had a minimum of -9 nT. The interplanetary magnetic field phi angle was mostly in the negative sector (directed towards the Sun). Further disturbed solar wind conditions are expected over the next 24 hours, due ongoing high speed stream and possible further CME effects. Further enhancements are possible from late on January 04 due to the arrival of a CME from January 01.

地磁

Over the past 24 hours, the geomagnetic conditions reached minor storm levels globally (NOAA Kp 5) and active levels locally (K BEL 4). Active to minor storm conditions are expected for the next 24 hours, with moderate storm intervals possible, particularly from January 04, due to the ongoing high speed stream and further CME effects.

質子通量水平

The greater than 10 MeV proton flux was below the 10 pfu threshold over the past 24 hours. It is expected to remain below this threshold level over 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 GOES-18 and GOES-19 satellites, exceeded the 1000 pfu threshold. The greater than 2 MeV electron flux is expected to again exceed the 1000 pfu threshold over the next 24 hours. The electron fluence was at moderate levels and is expected to be at moderate levels for the next 24 hours.

今日估計的國際太陽黑子數(ISN):105,基於09個觀測站。

太陽活動指數 02 Jan 2026

卡塔尼亞沃爾夫數121
10厘米太陽通量166
AK Chambon La Forêt044
AK Wingst032
估計地磁Ap指數031
估計國際太陽黑子數123 - 基於17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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