查看星期一, 28 6月 1999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 1999 Jun 28 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 179 在 28 JUN 1999 上以 2200Z 發行

IA. 太陽活動區域和 27-2100Z到 28-2100Z的活動分析

SOLAR ACTIVITY WAS LOW. REGION 8611 (S25E47) WAS THE MOST ACTIVE REGION ON THE DISK TODAY AND PRODUCED NUMEROUS C-CLASS SUBFLARES. THE LARGEST OF THESE WAS A C6/1F AT 1934Z. THIS GROUP EXHIBITED VERY BRIGHT PLAGE ALL DAY AND IS GROWING STEADILY. REGION 8598 (N22W25) IS STILL THE LARGEST SUNSPOT GROUP ON THE DISK BUT COULD ONLY MUSTER ONE SUBFLARE, IN SPITE OF A DELTA SPOT NEAR REGION CENTER. THIS GROUP SHOWED SIGNIFICANT DECAY OF MAGNETIC FLUX AND IS CLEARLY ON THE DECLINE. A PARTIAL HALO CME WAS REPORTED BY LASCO THAT WAS ASSOCIATED WITH A SIGNATURE IN EIT IN THE NORTHWEST QUADRANT OF THE SOLAR DISK. THESE EVENTS WERE ALSO TIME COINCIDENT WITH YESTERDAY'S M1 FLARE FROM REGION 8592 AT N23W25.
IB. 太陽活動預報
SOLAR ACTIVITY IS EXPECTED TO BE LOW TO MODERATE. REGIONS 8598 AND 8611 ARE THE BEST CANDIDATES FOR PRODUCING AN ISOLATED M-CLASS EVENT OVER THE NEXT THREE DAYS. REGIONS 8602 (N18E08), AND 8603 (S15E18) MIGHT ALSO CONTRIBUTE, GIVEN THE CURRENT SLOW GROWTH TREND IN THESE REGIONS.
IIA. 地球物理活動摘要 27-2100Z 至 28-2100Z
THE GEOMAGNETIC FIELD RANGED FROM QUIET TO MAJOR STORM LEVELS. YESTERDAY'S ACTIVE CONDITIONS DECLINED TO QUIET AROUND 28/0000Z. AROUND 28/0400Z THE SOLAR WIND VELOCITY BEGAN TO INCREASE SIGNIFICANTLY, REACHING SPEEDS AS HIGH AS 900 KM/S BY 0510Z. THE GEOMAGNETIC FIELD RESPONDED WITH A PERIOD OF MAJOR STORM FROM 0300-0600Z, FOLLOWED BY AN ACTIVE TO MINOR STORM PERIOD FROM 0600-0900Z. THE INTERPLANETARY MAGNETIC FIELD SHOWED SOME MILDLY NEGATIVE BZ FROM 0400-0600Z BUT RETURNED TO NOMINAL LEVELS THEREAFTER. IN RESPONSE THE GEOMAGNETIC FIELD ALSO CALMED TO QUIET TO UNSETTLED FROM 0900Z THROUGH THE END OF THE DAY. GIVEN THE HIGH SPEED AND VERY LOW DENSITY SEEN WITH THIS SOLAR WIND EVENT, IT IS MOST LIKELY THAT ACE OBSERVED THE RAREFACTION REGION BEHIND THE PARTIAL HALO CME OF 24 JUNE, WHICH WAS KNOWN TO BE DIRECTED SLIGHTLY TO THE WEST OF THE SUN-EARTH LINE.
IIB. 地球物理活動預報
THE GEOMAGNETIC FIELD IS EXPECTED TO BE UNSETTLED TO ACTIVE FOR THE NEXT 24 HOURS. MOSTLY UNSETTLED CONDITIONS SHOULD DOMINATE ON THE SECOND DAY. PREDOMINANTLY UNSETTLED LEVELS ARE ALSO EXPECTED ON THE THIRD DAY, BUT THERE WILL BE AN ENHANCED PROBABILITY FOR SOME ACTIVE PERIODS BECAUSE OF THE PARTIAL HALO CME OF THE 27TH.
III. 事件機率 29 JUN 至 01 JUL
M級55%50%45%
X級05%05%05%
質子10%10%05%
碳核算金融聯盟GREEN
IV. 彭迪克頓10.7厘米通量
  觀測的       28 JUN 197
  預測的   29 JUN-01 JUL  180/175/170
  90天平均值        28 JUN 144
V. 地磁 A 指數
OBSERVED AFR/AP 27 JUN  015/021
ESTIMATED AFR/AP 28 JUN  020/025
PREDICTED AFR/AP 29 JUN-01 JUL  012/018-010/012-012/015
VI. 地磁活動機率 29 JUN 至 01 JUL
A. 中緯度
可見25%15%20%
小風暴05%05%10%
特大強風暴05%01%05%
B. 高緯度
可見25%15%20%
小風暴05%05%15%
特大強風暴05%01%05%

所有時間均採用 UTC 時間

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