查看星期四, 8 9月 2005歷史檔案

太陽活動報表

本報告中提到的任何太陽耀斑都有太空天氣預報中心(SWPC) 應用的比例因子。由於 SWPC 比例因子,據報導太陽耀斑比科學質量數據小 42%。比例因子已從我們存檔的太陽耀斑資料中刪除,以反映真實的物理單位。
太陽地球物理活動報告 2005 Sep 08 2204 UTC
由美國國家海洋暨大氣總署 NOAA 及 太空天氣預測中心 SWPC 複製並編製,並由 ©SpaceWeatherLive.com 處理

美國空軍/美國國家海洋暨大氣總署太陽與地球物理活動聯合報告

SDF 編號 251 在 08 Sep 2005 上以 2200Z 發行

IA. 太陽活動區域和 07-2100Z到 08-2100Z的活動分析

Solar activity remains at high levels. An X5/2b flare was in progress from Region 808 (S09E67) at the time of this writing. Moderate centimetric radio bursts are also in progress, including a 990 sfu Tenflare. Very active Region 808 is rotating into view as a large and complex sunspot cluster. Limb proximity is still hindering the analysis, but this compact spot group will likely exceed 1000 millionths of white light area. Numerous C-class flares and two M2 flares preceded the X5 event. New Region 809 (N10E60) was numbered today.
IB. 太陽活動預報
Solar activity is expected to remain at high levels. Region 808 is a large and complex sunspot group capable of producing M and X-class flares.
IIA. 地球物理活動摘要 07-2100Z 至 08-2100Z
The geomagnetic field was quiet to unsettled. A sudden disturbance of 41 nT (magnetic crochet) was observed in the geomagnetic field following today's X5 flare. A greater than 10 and greater than 100 MeV proton event occurred following yesterday's X17 flare on the southeast limb. The greater than 10 MeV proton event began at 08/0215Z and remains in progress. The peak flux so far was 87 pfu at 08/1950Z. The greater than 100 MeV proton event began at 08/0405Z and also remains in progress. The peak flux was 7 pfu at 08/1925Z. A greater than 100 MeV proton event from a source on the east limb is extremely rare. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels again today.
IIB. 地球物理活動預報
The geomagnetic field is expected to range from quiet to minor storm levels. The CME associated with yesterday's X17 flare was very large and very fast. Although the magnetic cloud associated with this CME is not expected to impact Earth, a shock passage is expected, which will likely produce active to minor storm periods on 09 Sep. Isolated active periods are expected on 10 and 11 Sep. The greater than 10 MeV proton event currently in progress is expected to continue through 10 Sep. A further enhancement in the greater than 10 MeV protons will likely follow the anticipated shock passage on 09 Sep. Today's X5 flare may enhance the existing proton event. The greater than 100 MeV proton event will persist through 09 Sep.
III. 事件機率 09 Sep 至 11 Sep
M級80%80%80%
X級50%50%50%
質子99%90%75%
碳核算金融聯盟in progress
IV. 彭迪克頓10.7厘米通量
  觀測的       08 Sep 094
  預測的   09 Sep-11 Sep  100/110/110
  90天平均值        08 Sep 091
V. 地磁 A 指數
  觀測的 Afr/Ap 07 Sep  018/015
  估算值     Afr/Ap 08 Sep  008/012
  預測的    Afr/Ap 09 Sep-11 Sep  020/025-015/020-008/010
VI. 地磁活動機率 09 Sep 至 11 Sep
A. 中緯度
可見40%30%25%
小風暴20%15%10%
特大強風暴10%05%01%
B. 高緯度
可見50%40%30%
小風暴30%20%15%
特大強風暴15%10%05%

所有時間均採用 UTC 時間

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