查看星期一, 18 3月 2002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 2002 Mar 18 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 077 在 18 Mar 2002 上以 2200Z 發行

IA. 太陽活動區域和 17-2100Z到 18-2100Z的活動分析

Solar activity was moderate. Activity in the vicinity of Region 9866 (S09W46) was associated with a long duration M1 flare which began at 0216 UTC and ended at 0400 UTC. Also associated with this event were a type IV sweep and a halo CME visible in LASCO imagery. Region 9866 continues to decay slowly. C-class flare activity was observed from Region 9870 (S20W39) which appears to have some new, opposite polarity flux emergence. Region 9871 (S19E07) produced a C8/1f flare at 1918 UTC and is currently the largest region on the disk.
IB. 太陽活動預報
Solar activity is expected to be moderate. Regions 9866 and 9871 are considered to be the most likely sources for M-class flares. There is a slight chance for a major flare during the next three days.
IIA. 地球物理活動摘要 17-2100Z 至 18-2100Z
The geomagnetic field was quiet until 1323 UTC when a strong sudden impulse (SI) was observed. The SI measured 42 nT on the Boulder magnetometer. The SI followed the passage of a shock at ACE at 1237 UTC. The post shock flow at ACE consisted of enhanced magnetic fields but so far they have been predominantly northward. Geomagnetic activity subsequent to the SI has been unsettled to active. The greater than 10 MeV proton event that began at 17/0820 UTC officially ended at 17/1230 UTC, but flux levels remained enhanced thereafter. With the arrival of the shock the protons once again reached event level, beginning at 19/1300 UTC. The maximum flux observed so far was 25 PFU at 19/1535 UTC.
IIB. 地球物理活動預報
The geomagnetic field is expected to be mostly active for the next 24 hours, with a chance for some isolated minor storm periods. After the current transient flow subsides there should be a lull in activity, but another shock is expected to arrive near mid-day (UT time) on the 20th in response to today's halo CME. Activity following this shock is expected to be mostly active. Conditions should subside to unsettled sometime on the third day. The greater than 10 MeV proton event is likely to end sometime in the next 12 hours.
III. 事件機率 19 Mar 至 21 Mar
M級55%55%55%
X級10%10%10%
質子30%10%10%
碳核算金融聯盟yellow
IV. 彭迪克頓10.7厘米通量
  觀測的       18 Mar 178
  預測的   19 Mar-21 Mar  180/175/175
  90天平均值        18 Mar 214
V. 地磁 A 指數
  觀測的 Afr/Ap 17 Mar  002/004
  估算值     Afr/Ap 18 Mar  015/012
  預測的    Afr/Ap 19 Mar-21 Mar  020/020-020/020-015/015
VI. 地磁活動機率 19 Mar 至 21 Mar
A. 中緯度
可見35%35%30%
小風暴25%25%20%
特大強風暴10%10%05%
B. 高緯度
可見35%35%30%
小風暴25%25%20%
特大強風暴15%15%10%

所有時間均採用 UTC 時間

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