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Proceedings Paper • Open Access

Opto-mechanical architecture of the LISA instrument
Author(s): Dennis Weise; Pierangelo Marenaci; Peter Weimer; Marcel Berger; Hans Reiner Schulte; Peter Gath; Ulrich Johann

Paper Abstract

We report on the latest iteration of the baseline opto-mechanical architecture of the LISA instru- ment, which has been developed within the current LISA Mission Formulation study under ESA con- tract. The collective features of the current architec- ture have been consolidated in an extensive trade of various alternative payload configurations, including variants with only one active proof mass per space- craft and the application of “In-Field Pointing” for accommodation of constellation breathing.

With respect to the original configuration [1], the newly established architecture most notably distin- guishes itself by the use of an off-axis telescope and a “non-frequency-swap” science interferometer for stray light mitigation, as well as the implementa- tion of ancillary pathlength metrology in terms of an “Optical Truss” and Point Ahead Angle sensing.

Paper Details

Date Published: 21 November 2017
PDF: 8 pages
Proc. SPIE 10566, International Conference on Space Optics — ICSO 2008, 1056611 (21 November 2017); doi: 10.1117/12.2308192
Show Author Affiliations
Dennis Weise, EADS Astrium GmbH (Germany)
Pierangelo Marenaci, EADS Astrium GmbH (Germany)
Peter Weimer, EADS Astrium GmbH (Germany)
Marcel Berger, EADS Astrium GmbH (Germany)
Hans Reiner Schulte, EADS Astrium GmbH (Germany)
Peter Gath, EADS Astrium GmbH (Germany)
Ulrich Johann, EADS Astrium GmbH (Germany)


Published in SPIE Proceedings Vol. 10566:
International Conference on Space Optics — ICSO 2008
Josiane Costeraste; Errico Armandillo; Nikos Karafolas, Editor(s)

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