查看星期三, 2 6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 Jun 02 1233 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 02 Jun 2021 到 04 Jun 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
02 Jun 2021076006
03 Jun 2021077013
04 Jun 2021077007

公告

The solar activity was quiet over the past 24 hours, with the GOES X-ray flux remaining below C-level. The bipolar sunspot group (Catania sunspot group 1, NOAA 2827) has decayed and a new sunspot region (not numbered) has rotated over the East limb in the South hemisphere. The solar activity is expected to remain mostly quiet.

No Earth directed Coronal Mass Ejection (CME) has been detected in the available coronagraph imagery.

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 was below the 1000 pfu threshold in the past 24 hours and is expected to remain so during the next 24 hours. The 24h electron fluence was at normal levels in the last 24 hours and is expected to stay at normal levels for the next 24 hours.

The solar wind parameters (as observed by ACE and DSCOVR) showed an ambient background and slow solar wind speed regime. The solar wind speed ranged between 280 km/s to 300 km/s. The interplanetary magnetic field magnitude was below 3.5 nT, and Bz components varied between -3.0 nT and 2.2 nT. The high-speed stream associated with the equatorial coronal hole (that reached the central meridian on May 31) is expected to enhance the solar wind condition later today or tomorrow.

The geomagnetic conditions were quiet over the past 24 hours. The conditions may become more active with the arrival of the high-speed streams from the equatorial coronal hole (that reached the central meridian on May 31) later today or tomorrow.

今日估計的國際太陽黑子數(ISN):028,基於19個觀測站。

太陽活動指數 01 Jun 2021

卡塔尼亞沃爾夫數021
10厘米太陽通量075
AK Chambon La Forêt003
AK Wingst001
估計地磁Ap指數001
估計國際太陽黑子數019 - 基於29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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