Interferometry for LISA

被引:8
作者
Robertson, D
Hough, J
机构
[1] Department of Physics and Astronomy, Glasgow University
关键词
D O I
10.1088/0264-9381/13/11A/036
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss some of the details of the optical layout and interferometry in the LISA project. The limitations on performance imposed by a variety of constraints and noise sources are considered. In addition a scheme to acquire and maintain optimum optical alignment is presented.
引用
收藏
页码:A271 / A277
页数:7
相关论文
共 5 条
[1]   LISA: Laser interferometer space antenna for gravitational wave measurements [J].
Danzmann, K .
CLASSICAL AND QUANTUM GRAVITY, 1996, 13 (11A) :A247-A250
[2]  
FALLER J, 1991, WORKSH P TECHN LAS G, V2
[3]  
MORRISON E, 1994, APPL OPTICS, V33, P22
[4]   NOISE BEHAVIOR OF THE GARCHING 30-METER PROTOTYPE GRAVITATIONAL-WAVE DETECTOR [J].
SHOEMAKER, D ;
SCHILLING, R ;
SCHNUPP, L ;
WINKLER, W ;
MAISCHBERGER, K ;
RUDIGER, A .
PHYSICAL REVIEW D, 1988, 38 (02) :423-432
[5]  
TYLER GL, 1992, J GEOPHYS RES, V97, pE5