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太阳宁静区的高分辨率像复原
引用本文:邓元勇,仇朴章.太阳宁静区的高分辨率像复原[J].天文学报,1994,35(4):380-386.
作者姓名:邓元勇  仇朴章
作者单位:中国科学院北京天文台,中国科学院云南天文台
摘    要:本文介绍在怀柔60cm多通道太阳望远镜上运用斑点干涉像复原方法所取得的一些初步结果,对用短暴光方法(暴光时间不大于10毫秒)获得的一系列“冻结”大气后的目标像用斑点干涉像复原方法进行处理,即可获得消除了地球大气影响的目标复原像,斑点掩模法即为斑点干涉像复原方法的一种,我们用它对日面中心的宁静区米粒进行处理,复原出了分率不劣于0.〃5的白光米粒象。

关 键 词:太阳物理  小尺度结构  高分辨观测  像复原

HIGH RESOLUTION IMAGE RECOVERY IN THE QUIET REGION OF THE SUN
Deng Yuan-yong,Ai Guo-xiang, Zhang Bin.HIGH RESOLUTION IMAGE RECOVERY IN THE QUIET REGION OF THE SUN[J].Acta Astronomica Sinica,1994,35(4):380-386.
Authors:Deng Yuan-yong  Ai Guo-xiang  Zhang Bin
Abstract:In this article, we introduce some preliminary results obtained by the method of speckle interference image recovery in Huairou's 60cm Multi-Channel Solar Telescope. When the atmosphere turbulence of the earth is "frozen" by the means of short exposure (the exposure time is not longer than 10 milliseconds),we collect a sequence of images of a solar object. Then,by the method of speckle interference image recovery,the atmosphere effect on these images may be removed and the reconstructed images of the solar object obtained.We have used Speckle-Masking method,one of the speckle interference method,to process the solar granulation in the quiet region near the disk center and reconstructed some white light granular images with resolution not worse than 0.5 arcsec.
Keywords:Solar physics  Fine structure of the Sun  High resolution observation  
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