Drag-free performance in a LISA mission with spherical proof masses

Details Drag-free performance in a LISA mission with spherical proof masses Drag-free performance in a LISA mission with spherical proof masses

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.1739l&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 7, pp. 1739-1743 (2002).

Computer Science

Performance

2

Scientific paper

The acceleration perturbations of a drag-free satellite with a free-floating spherical proof mass for the LISA space mission to detect gravity waves are presented. These calculations show that the RSS of all disturbances is less than 3.4 × 10-16 m s-2 Hz-1/2. This is about a factor of 10 less than the calculated value for cubical single-axis proof masses and could potentially decrease the low-frequency response correspondingly. The performance calculations presented here have been confirmed by the flight of the DISCOS drag-free satellite.

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