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1989年8月17日耀斑后环系速度场分析
引用本文:顾啸马,郭金平.1989年8月17日耀斑后环系速度场分析[J].紫金山天文台台刊,1999,18(2):128-130.
作者姓名:顾啸马  郭金平
作者单位:中国科学院云南天文台!昆明650011,中国科学院光学天文联合开放实验室,中国科学院云南天文台!昆明650011,中国科学院光学天文联合开放实验室,中国科学院云南天文台!昆明650011,中国科学院光学天文联合开放实验室
摘    要:本文给出了1989 年8 月17 日耀斑后环的观测视向速度场,在环内物质在太阳重力、磁场梯度和大气压力梯度联合作用下沿环腿螺旋上升和环内物质密度由环腿向环顶和环足线性递增的假设下,理论上计算了该环系的视向速度场,理论计算和观测结果基本相符,似乎为耀斑物质由色球蒸发作上升运动的观点提供了间接的例证

关 键 词:耀斑后环  速度场

AN ANALYSIS ON VELOCITY FIELD OF THE POST FLARE LOOP SYSTEM OF AUGUST 17, 1989
Authors:Gu Xiao  Ma  Dun Jin  Ping  Zhong Shu  Hua
Abstract:The line of sight velocity fields of the post flare loop system observed at Yunnan Observatory on August 17 in 1989 are given. A theoretical velocity field is computed under some assumptions that the matter within loop system up flows in helical lines from the loop feet to the top of the system under an united actions of solar gravity, both gradients of magnetic field and atmospoheric pressure, and the density distribution in the system increases linearly from the middle of the loops towards the top and the feet. The velocity field computed is basically similar to that observed. It shows that the assumptions mentioned above are acceptable. It seems to provide an indirect evidence for the evaporation model of solar flares.
Keywords:post  flare loops  velocity field
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