查看星期六, 18 10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 Oct 18 1235 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

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

	10公分通量	Ap
18 Oct 2025	168	040
19 Oct 2025	171	035
20 Oct 2025	173	029

太陽活動區和耀斑

Solar flaring activity was moderate over the past 24 hours with 10 M-class flares recorded. The largest flare was an M1.5 flare (SIDC Flare 5830) peaking on October 18 at 10:51 UTC, which was produced by SIDC Sunspot Group 639 (NOAA Active Region 4246). This is the most complex on disk and was responsible for all of the M-class flaring activity and is now rotating over the west limb. SIDC Sunspot group 621 (NOAA Active region 4248), another complex region on disk, was stable and quiet. A new region rotated over the east solar limb and was numbered SIDC Sunspot Group 674 (NOAA Active region 4257). A new region also emerged in the west quadrant and was numbered SIDC Sunspot Group 673 (NOAA Active region 4258). These and the remaining regions on disk were mostly quiet and either stable or in decay. The 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 Ejections (CMEs) were observed.

日冕洞

SIDC Coronal Hole 126 (extended equatorial coronal hole with a negative polarity) continues to transit the central meridian since October 16.

太陽風

The solar wind conditions reflected ongoing transient magnetic features, likely associated with the CMEs from October 13-15. The magnetic field was around 10 nT over the first half of the period and increased to a maximum of 20 nT around 08:30 UTC October 18. The Bz was mostly positive with an extended period of negative Bz between 04:00 and 07:00 UTC October 18 with a minimum value of -12 nT. The solar wind speed was stable around 400 km/s but increased from 06:00 UTC on October 18 to around 500 km/s at the end of the period. Over the next 24 hours the solar wind conditions are expected to continue to be slightly perturbed due to further influence from the glancing blow CME arrival from the partial halo CME observed on October 15. From late October 19, the high-speed stream associated with the negative polarity coronal hole (SIDC Coronal Hole 126) is also expected to arrive.

地磁

Geomagnetic conditions were at quiet to unsettled levels on October 17. From October 18 the geomagnetic conditions increased to active levels with one period of minor storm conditions (Kp 5) globally between 06:00 and 09:00 UTC. Locally active conditions were reached (K Bel 1-4). Minor storm conditions (Kp 5) are expected on October 18 and 19 in response CME influence and arrival of the high-speed stream arrival, with periods of moderate storm conditions possible (Kp 6).

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. There is a small chance of an increase related to any high-level flaring, particularly from SIDC Sunspot Group 639 (NOAA Active Region 4246).

地球靜止軌道上的電子通量

The greater than 2 MeV electron flux measured by GOES 18 and GOES 19 briefly exceeded the 1000 pfu threshold. The greater than 2 MeV electron flux is expected to again be at or just below the 1000 pfu threshold over the next 24 hours. The 24-hour electron fluence was at moderate levels and is expected to be at low to moderate levels over the next 24 hours.

今日估計的國際太陽黑子數（ISN）：115，基於13個觀測站。

太陽活動指數 17 Oct 2025

卡塔尼亞沃爾夫數	131
10厘米太陽通量	164
AK Chambon La Forêt	023
AK Wingst	009
估計地磁Ap指數	010
估計國際太陽黑子數	118 - 基於14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

所有時間均採用 UTC 時間

<< 回到每日概觀