查看星期六, 23 9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 Sep 23 1231 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
23 Sep 2023176013
24 Sep 2023176023
25 Sep 2023176019

太陽活動區和耀斑

There are twelve active regions visible on the disk. There were three M-class flares in the last 24 hours, the strongest one was an M1.9 from NOAA AR 3435 (beta magnetic field configuration), peaking at 23:00 UTC on 22 September. The other two M_class flares were produced by the new NOAA ARs 3443 (beta-gamma magnetic field configuration). All the other regions have simpler alpha or beta magnetic field configuration. More M-class flares can be expected in the next 24 hours, X-class flares are possible but less likely.

日冕物質拋射

A wide CME with angular width around 90 degrees was first seen by LASCO-C2 at 02:24 UTC on 22 September. The CME was related to the M1.2 flare from NOAA AR 3435. The CME speed was estimated to be around 730 km/s, with the bulk of the material directed to the NE. Since the source is located close to disk center, an impact at Earth can be expected on 24 September(this ICME will probably interact with the one from 21 September on its way to the Earth).

日冕洞

There are two small negative coronal holes that crossed the central meridian on 20 September, one at the equator and one in the northern hemisphere.

太陽風

In the last 24 hours, the solar wind speed at the Earth has been around 400 km/s and the interplanetary magnetic field around 5 nT. Similar slow solar wind conditions can be expected for the next 24 hours. Nevertheless, the CME from 20 September can arrive to the Earth and change the solar wind conditions. Furthermore, we may observe the arrival of a (mild) high speed stream from the two coronal holes that traversed the central meridian on 20 September.

地磁

During the last 24 hours the geomagnetic conditions have been quiet to unsettled, both globally and locally (NOAA KP 3, K_Bel 3). Geomagnetic conditions are expected to reach minor to moderate storm levels if the expected CMEs and high speed streams arrive.

質子通量水平

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

地球靜止軌道上的電子通量

The greater than 2 MeV electron flux was above the 1000 pfu, as measured by GOES 16. It has gone down in the last hours, but it may increase over the threshold again in the next 24 hours. The 24 hour electron fluence was at moderate levels, it is expected to stay at those levels for the next 24 hours.

今日估計的國際太陽黑子數(ISN):214,基於13個觀測站。

太陽活動指數 22 Sep 2023

卡塔尼亞沃爾夫數239
10厘米太陽通量176
AK Chambon La Forêt021
AK Wingst010
估計地磁Ap指數011
估計國際太陽黑子數221 - 基於16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
22155316231646----M1.473/3443
22170617151720----M1.573/3443III/2
22222523002313N02W03M1.9SF70/3435III/2

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

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