J W Armstrong et al 2001 Class. Quantum Grav. 18 4059 doi:10.1088/0264-9381/18/19/313
J W Armstrong, F B Estabrook and Massimo Tinto
Show affiliationsLISA 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.
78A60 Lasers, masers, optical bistability, nonlinear optics (See also 81V80)
Issue 19 (7 October 2001)
Received 15 November 2000
Published 17 September 2001
J W Armstrong et al 2001 Class. Quantum Grav. 18 4059
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