查看星期日, 7 11月 2004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 2004 Nov 07 2200 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 312 在 07 Nov 2004 上以 2200Z 發行

IA. 太陽活動區域和 06-2100Z到 07-2100Z的活動分析

Solar activity has been high. Region 696 (N08W22) produced numerous C-class flares, and at 1606 UTC a long duration X2.0 flare, accompanied by a Type II radio sweep (673 km/s), a Type IV radio sweep, and a 4600 sfu Tenflare. A CME may have occurred in association with this flare, although LASCO imagery was not available. Region 696 decayed significantly to an area of 650 millionths in white light. The region maintains its complex beta-gamma-delta magnetic configuration. No new regions were numbered today.
IB. 太陽活動預報
Solar activity is expected to be moderate to high. Although it has decayed in size, Region 696 is expected to produce M-class and isolated X-class flares.
IIA. 地球物理活動摘要 06-2100Z 至 07-2100Z
The geomagnetic field has been at quiet to major storm levels. A shock arrived at ACE at 1555 UTC which caused subsequent major storming in Earth's magnetic field beginning at 1608 UTC. Another shock passage was observed at ACE at 1755 UTC that resulted in a 41nT sudden impulse at 1831 UTC followed by minor storming. These shock passages are most likely from the CMEs associated with flare activity on 3 and 4 November. The greater than 10 MeV proton flux crossed 10 pfu at 1910 UTC and ended the period at 72 pfu. The greater than 100 MeV proton flux was elevated but did not cross the 1 pfu threshold. Energetic proton activity was most likely associated with the X2 flare.
IIB. 地球物理活動預報
The geomagnetic field is expected to be at unsettled to major storm levels. A shock passage from the CME associated with the M2/M5 flares from 5 November is expected to arrive early on 8 November, and a shock passage from the CME associated with the M9 flare from 6 November is expected to arrive on 9 November. Today's X2 flare very likely produced a CME that could arrive late on 9 November. These anticipated shock passages, along with the elevation in solar wind speed due to a geoeffective coronal hole, should keep geomagnetic activity at unsettled to minor storm levels all three days, with isolated major storming possible on 8-9 November. The greater than 10 MeV proton flux at GOES is expected to stay above the 10 pfu threshold through 8 November, and will likely cross the 100 pfu threshold early on 8 November.
III. 事件機率 08 Nov 至 10 Nov
M級75%75%75%
X級20%20%20%
質子20%20%20%
碳核算金融聯盟yellow
IV. 彭迪克頓10.7厘米通量
  觀測的       07 Nov 130
  預測的   08 Nov-10 Nov  125/125/120
  90天平均值        07 Nov 110
V. 地磁 A 指數
  觀測的 Afr/Ap 06 Nov  004/003
  估算值     Afr/Ap 07 Nov  022/025
  預測的    Afr/Ap 08 Nov-10 Nov  020/030-025/030-025/040
VI. 地磁活動機率 08 Nov 至 10 Nov
A. 中緯度
可見40%40%30%
小風暴30%30%20%
特大強風暴20%20%15%
B. 高緯度
可見40%40%40%
小風暴40%40%30%
特大強風暴20%20%20%

所有時間均採用 UTC 時間

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