查看星期一, 30 1月 2023歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2023 Jan 30 1231 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 30 Jan 2023 到 01 Feb 2023 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
30 Jan 2023143006
31 Jan 2023141007
01 Feb 2023143007

公告

There are six active regions visible on the solar disc, all of them with simple alpha or beta magnetic field configuration. Solar flaring activity was at low levels over the past 24 hours, with several C-class flares detected. The strongest one was a C3.1 flare from a region rotating over the east limb, that peaked at 12:07 UTC, this event is still ongoing at the moment of writing. Further C class flaring is expected.

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

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux has been below the 1000 pfu threshold and is expected to remain so. The 24h electron fluence was at normal levels and is expected to remain so over the next 24 hours.

A small equatorial coronal hole of negative polarity has crossed the central meridian and is expected to influence solar wind conditions starting February 1.

The solar wind speed at the Earth has decreased to 400 km/s. The magnitude of the interplanetary magnetic field is around 5 nT. The interplanetary magnetic field changed from positive to negative polarity. Similar slow solar wind conditions can be expected for the next 24 hours.

Geomagnetic conditions were quiet (both NOAA Kp and local K Belgium 0-2). Similar conditions expected for the next 24 hours.

今日估計的國際太陽黑子數(ISN):071,基於14個觀測站。

太陽活動指數 29 Jan 2023

卡塔尼亞沃爾夫數///
10厘米太陽通量137
AK Chambon La Forêt009
AK Wingst006
估計地磁Ap指數004
估計國際太陽黑子數084 - 基於09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

所有時間均採用 UTC 時間

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