Three-dimensional image reconstruction of an Hα flare on 26 March 2001

被引：0
|
作者：
徐稚
屈中权
张霄宇
栾蒂
刘子忠
机构：
[1] Yunnan Astronomical Observatory National Astronomical Observatories Chinese Academy of Sciences Kunming 650011 China
[2] Yunnan Astronomical Observatory National Astronomical Observatories Chinese Academy of Sciences Kunming 650011 China
来源：
Science China Mathematics | 2002年 / S1期
关键词：
line formation; contribution function; radiative transfer; solar flare;
D O I：
暂无
中图分类号：
P182.51 [];
学科分类号：
070401 ;
摘要：
Three-dimensional (3D) image reconstruction of an Hoc flare near the solar disk centeris done by a series of line-center and off-line-center filtering observation, according to the physicalmeaning of contribution function based on the line formation theory. The contribution functionrepresents the contribution from stellar atmospheric layers to the emergent specific intensity anddescribes the depth distribution of escape photons. In this paper, an Hot flare of 26 March 2001 isused to illustrate the 3D line-of-sight reconstruction and its development.
引用
收藏
页码：51 / 56
页数：6
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