LISA telescope sensitivity analysis

Details LISA telescope sensitivity analysis LISA telescope sensitivity analysis

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002spie.4767..114w&link_type=abstract

Current Developments in Lens Design and Optical Engineering III. Edited by Fischer, Robert E.; Smith, Warren J.; Johnson, R. Ba

Physics

Scientific paper

The Laser Interferometer Space Antenna (LISA) for the detection of Gravitational Waves is a very long baseline interferometer which will measure the changes in the distance of a five million kilometer arm to picometer accuracies. As with any optical system, even one with such very large separations between the transmitting and receiving telescopes, a sensitivity analysis has to be performed to see how, in this case, the far field phase varies when the telescope parameters change as a result of structural stress relief or temperature changes. The results of the sensitivity analysis are presented.

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