中国科学A辑(英文版)
中國科學A輯(英文版)
중국과학A집(영문판)
SCIENCE IN CHINA
2002年
z1期
51-56
,共6页
徐稚%屈中权%张霄宇%栾蒂%刘子忠
徐稚%屈中權%張霄宇%欒蒂%劉子忠
서치%굴중권%장소우%란체%류자충
line formation%contribution function%radiative transfer%solar flare
Three-dimensional (3D) image reconstruction of an Hα flare near the solar disk center, is done by a series of line-center and off-line-center filtering observation, according to the physical meaning of contribution function based on the line formation theory. The contribution function represents the contribution from stellar atmospheric layers to the emergent specific intensity and describes the depth distribution of escape photons. In this paper, an Hα flare of 26 March 2001 is used to illustrate the 3D line-of-sight reconstruction and its development.
