查看星期五, 9 4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 Apr 09 1239 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 09 Apr 2021 到 11 Apr 2021 都有效
太陽閃焰

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

地磁

Quiet (A<20 and K<4)

太陽質子

Quiet

10公分通量Ap
09 Apr 2021074004
10 Apr 2021073006
11 Apr 2021075013

公告

The solar activity has been very low over the past 24 hours. The Sun is currently spotless. A small bipolar region is visible at the SE quadrant. The solar activity is expected to remain at low levels over the next 24 hours.

No Earth-directed coronal mass ejections were observed in the available coronagraphic imagery.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, with a chance to exceed this level during the next 24 hours. This is due to the influence of the high speed stream associated with the Coronal Hole at Central Meridian on April 3. The 24h electron fluence was at nominal levels and is expected to increase over the next 24 hours.

The solar wind speed decreased from between 475 to 390 km/s over the past 24 hours. The total magnetic field strength fluctuated between 1 and 5 nT. The values of the Bz component varied between -4 and +3 nT. The interplanetary magnetic field phi angle was predominantly in the positive sector (directed away from the Sun), until April 9 09:30UT when it switched to the negative sector. Solar wind conditions are expected to reflect a slow solar wind regime.

Geomagnetic conditions were at quiet levels (NOAA Kp and local K Dourbes 0-2) over the past 24 hours. Quiet conditions are expected over the next 24 hours.

今日估計的國際太陽黑子數(ISN):000,基於23個觀測站。

太陽活動指數 08 Apr 2021

卡塔尼亞沃爾夫數000
10厘米太陽通量074
AK Chambon La Forêt008
AK Wingst004
估計地磁Ap指數003
估計國際太陽黑子數000 - 基於24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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