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Konferenzbeitrag

LISA Optical Bench Testing

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons40503

Tröbs,  M.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4350

Bogenstahl,  J.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons40460

Heinzel,  G.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons40437

Danzmann,  K.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Trobs.pdf
(beliebiger Volltext), 58KB

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Zitation

Tröbs, M., d'Arcio, L., Barke, S., Bogenstahl, J., Diekmann, C., Fitzsimons, E. D., et al. (2013). LISA Optical Bench Testing.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-FD0A-D
Zusammenfassung
Each LISA satellite carries optical benches, one for each test mass, that measure the distance to the local test mass and to the remote optical bench on the distant satellite. Currently, an elegant bread board of the optical bench is developed for the European Space Agency (ESA) by EADS Astrium, TNO Science and Technology, University of Glasgow and the Albert Einstein Institute. To test the optical bench the two interferometers mentioned above must be completed by an external simulator, the test mass and telescope simulator. We give an overview of the simulator layout and performance predictions.