摘要
介绍一种天文高分辨率像复原的方法——斑点全息术,并给出了人造目标和真实大气的模拟计算结果,最后指出此方法的应用局限及克服局限性的可能途径。
A method for the high resolution image reconstruction, or the speckle holograghy, is introduced and the results of the simulating calculation of an artificial object and the real atmosphere are given. Then, the limitation of application of this method and some ways to get rid of the limitation are discussed.
出处
《云南天文台台刊》
CSCD
1992年第2期48-52,共5页
Publications of the Yunnan Observatoty
