Doppler radial velocity detection based on Doppler asymmetric spatial heterodyne spectroscopy technique for absorption lines  

作　　者：Yin-Li Kuang Liang Fang Xiang Peng Xin Cheng Hui Zhang En-Hai Liu 况银丽;方亮;彭翔;程欣;张辉;刘恩海(Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610209,China;University of Chinese Academy of Sciences,Beijing 100049,China)

机构地区：[1]Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610209,China [2]University of Chinese Academy of Sciences,Beijing 100049,China

出　　处：《Chinese Physics B》2020年第2期183-189,共7页中国物理B（英文版）

基　　金：Project supported by the National Basic Research Program of China(Grant No.2014CB744204).

摘　　要：Doppler asymmetric spatial heterodyne spectroscopy(DASH)technique has developed rapidly in passive Doppler-shift measurements of atmospheric emission lines over the last decade.With the advantages of high phase shift sensitivity,compact,and rugged structure,DASH is proposed to be used for celestial autonomous navigation based on Doppler radial velocity measurement in this work.Unlike atmospheric emission lines,almost all targeted lines in the research field of deep-space exploration are the absorption lines of stars,so a mathematical model for the Doppler-shift measurements of absorption lines with a DASH interferometer is established.According to the analysis of the components of the interferogram received by the detector array,we find that the interferogram generated only by absorption lines in a passband can be extracted and processed by a method similar to the approach to studying the emission lines.In the end,numerical simulation experiments of Doppler-shift measurements of absorption lines are carried out.The simulation results show that the relative errors of the retrieved speeds are less than 0.7%under ideal conditions,proving the feasibility of measuring Doppler shifts of absorption lines by DASH instruments.Doppler asymmetric spatial heterodyne spectroscopy(DASH) technique has developed rapidly in passive Dopplershift measurements of atmospheric emission lines over the last decade.With the advantages of high phase shift sensitivity,compact,and rugged structure,DASH is proposed to be used for celestial autonomous navigation based on Doppler radial velocity measurement in this work.Unlike atmospheric emission lines,almost all targeted lines in the research field of deep-space exploration are the absorption lines of stars,so a mathematical model for the Doppler-shift measurements of absorption lines with a DASH interferometer is established.According to the analysis of the components of the interferogram received by the detector array,we find that the interferogram generated only by absorption lines in a passband can be extracted and processed by a method similar to the approach to studying the emission lines.In the end,numerical simulation experiments of Doppler-shift measurements of absorption lines are carried out.The simulation results show that the relative errors of the retrieved speeds are less than 0.7% under ideal conditions,proving the feasibility of measuring Doppler shifts of absorption lines by DASH instruments.

关 键 词：DOPPLER ASYMMETRIC SPATIAL HETERODYNE spectroscopy(DASH) Doppler-shift measurement absorption line celestial autonomous navigation 

分 类 号：P128.4[天文地球—天体测量] V448.2[天文地球—天文学]