查看星期四, 14 7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 Jul 14 2210 UTC
# Prepared jointly by the U.S. Dept. of Commerce, NOAA, #Space Environment Center and the U.S. Air Force. #

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 195 在 14 Jul 2005 上以 2200Z 發行

IA. 太陽活動區域和 13-2100Z到 14-2100Z的活動分析

Solar activity was at high levels this period. Region 786 (N12W97) continues to be very active as it rotates around the west limb. Two major events occurred from this region today. The first was an M9 x-ray event with a 220 sfu Tenflare at 14/0725Z. A CME was observed on LASCO imagery in association with this event. A considerably more powerful, long duration X1 proton flare occurred at 14/1055Z. Strong radio emissions accompanied this flare including a 3400 sfu Tenflare, a 120,000 sfu burst at 610 MHz, and a Type IV radio sweep. A very bright and fast (approximately 1430 km/s) halo CME was observed on LASCO imagery. The remainder of the solar disk and limb was quiet.
IB. 太陽活動預報
Solar activity is expected to be moderate, although there is still a chance for another major flare from Region 786 as it rotates around the west limb. Low to very low conditions are expected on 16 and 17 July.
IIA. 地球物理活動摘要 13-2100Z 至 14-2100Z
The geomagnetic field was quiet to active. Solar wind speed remains elevated near 500 km/s, but is declining. The most disturbed geomagnetic periods occurred between 14/0100 - 1300Z when the IMF Bz was predominantly southward. A slow, gradual rise in the greater than 10 MeV protons began soon after yesterday's M5 event. The 10 pfu alert threshold was finally reached at 14/0245Z. A second, larger influx of high energy protons followed today's X1 flare. The greater than 10 MeV proton flux were still slowly increasing at issue time, and the peak flux so far is 53 pfu at 14/1905Z. The greater than 2 MeV electron flux 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 over the next three days. Occasional major storm periods are possible at high latitudes. At least three CMEs from the M1, M5, and X1 events on 12, 13, and 14 July respectively, are expected to generate the storm periods. The greater than 10 MeV proton event currently in progress is expected to continue through 15 July. Assuming no new injection of particles, this event will likely end by 16 July.
III. 事件機率 15 Jul 至 17 Jul
M級50%20%10%
X級10%01%01%
質子20%10%05%
碳核算金融聯盟In Progress
IV. 彭迪克頓10.7厘米通量
  觀測的       14 Jul 090
  預測的   15 Jul-17 Jul  085/080/080
  90天平均值        14 Jul 097
V. 地磁 A 指數
  觀測的 Afr/Ap 13 Jul  020/030
  估算值     Afr/Ap 14 Jul  010/015
  預測的    Afr/Ap 15 Jul-17 Jul  025/025-025/025-015/020
VI. 地磁活動機率 15 Jul 至 17 Jul
A. 中緯度
可見50%50%40%
小風暴30%30%20%
特大強風暴10%10%05%
B. 高緯度
可見45%45%40%
小風暴35%35%25%
特大強風暴20%20%10%

所有時間均採用 UTC 時間

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