Sensitivities of alternate LISA configurations

被引：27

作者：

Armstrong, JW ^{[1
]}

Estabrook, FB ^{[1
]}

Tinto, M ^{[1
]}

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

来源：

CLASSICAL AND QUANTUM GRAVITY | 2001年 / 18卷 / 19期

关键词：

D O I：

10.1088/0264-9381/18/19/313

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

LISA can be considered as six proof masses, pairwise Doppler tracked with one-way optical links. An appropriate combination of these one-way Doppler links can cancel the principal noise sources (laser phase noise and optical bench motion noise). Here we compute the gravitational wave sensitivities for the baseline Michelson combination and for several other LISA data combinations which also cancel the leading noise.

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收藏

页码：4059 / 4065

页数：7

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