查看星期四, 20 5月 2021歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2021 May 20 1231 UTC

SIDC太陽影響數據分析中心的預報

太陽閃焰

Quiet conditions (<50% probability of C-class flares)

地磁

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

太陽質子

Quiet

	10公分通量	Ap
20 May 2021	076	028
21 May 2021	076	007
22 May 2021	077	007

公告

Two active regions (ARs) visible on the disk, NOAA AR 2822 (Catania 93, alpha magnetic field configuration, rotating over the west limb) and AR 2824 (Catania 96, decayed to alpha magnetic field configuration). Solar activity is very low, only B-class flares were seen in the past 24 hours. The situation is expected to remain the same for the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraphic imagery in the last 24 hours.

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

In the last hours, the solar wind speed has shown a gradual increase from about 320 km/s to 410 km/s, accompanied by similar increases in density and strong magnetic fields (with intensity up to 17 nT and Bz reaching -13 nT). This marks the arrival of the high speed stream from the coronal hole that crossed central meridian late on May 15. The interplanetary magnetic field polarity was mostly negative (towards the Sun). The solar wind speed is expected to increase more in the next 24 hours.

Geomagnetic conditions have been quiet to unsettled (KDourbes 1-3, Kp 1-3). Minor storm periods, and up to isolated major storm periods, can be expected due to the high speed solar wind stream arriving to the Earth.

今日估計的國際太陽黑子數（ISN）：019，基於23個觀測站。

太陽活動指數 19 May 2021

卡塔尼亞沃爾夫數	037
10厘米太陽通量	076
AK Chambon La Forêt	014
AK Wingst	007
估計地磁Ap指數	006
估計國際太陽黑子數	025 - 基於31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

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