Laser ranging and data communication for space gravitational wave detection

被引：12
|
作者：
Liu He-shan [1 ]
Gao Rui-hong [1 ,2 ]
Luo Zi-ren [1 ]
Jin Gang [1 ,2 ]
机构：
[1] Chinese Acad Sci, Inst Mech, Beijing 100190, Peoples R China
[2] Univ Chinese Acad Sci, Sch Engn Sci, Beijing 100049, Peoples R China
来源：
CHINESE OPTICS | 2019年 / 12卷 / 03期
关键词：
space gravitational wave detection; absolute ranging measurement; laser communication;
D O I：
10.3788/CO.20191203.0486
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
Due to the large unequal interferometer arm, laser frequency jitter noise is the dominant noise in space gravitational wave detection. This noise can be less than shot noise when the frequency jitter is suppressed below than 10(-6) HZ(1/2) through the combination of PDH (Pound-Drever-Hall), arm locking and TDI (Time Delay Interferometer) technologies. However, absolute ranging and laser communication are the preconditions of the TDI. In this paper, we discuss the principle and implementation of the absolute ranging and laser communication. The pseudo-random code and communication code are modulated by the EOM (Electro-Optic Modulator) into the phase of the main laser beam and then sent to the far satellite. The absolute distance and the message can be obtained through the PLL (Phase Lock Loop) and the DLL (Delay Lock Loop). The related conclusions can be regarded as the basis and principle for related experimentation and will give a design reference for future space gravitational wave detection in our country.
引用
收藏
页码：486 / 492
页数：7
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