Automatic beam alignment in the Garching 30-m prototype of a 
laser-interferometric gravitational wave detector

Heinzel, Gerhard; Rüdiger, Albrecht; Schilling, Roland; Strain, Kenneth A.; Winkler, Walter; Mizuno, J.; Danzmann, Karsten

doi:10.1016/S0030-4018(98)00654-3

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Automatic beam alignment in the Garching 30-m prototype of a laser-interferometric gravitational wave detector

MPG-Autoren

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

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Rüdiger, Albrecht
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40488

Schilling, Roland
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Strain, Kenneth A.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Winkler, Walter
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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

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

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Zitation

Heinzel, G., Rüdiger, A., Schilling, R., Strain, K. A., Winkler, W., Mizuno, J., et al. (1999). Automatic beam alignment in the Garching 30-m prototype of a laser-interferometric gravitational wave detector. Optics Communications, 160(4-6), 321-334. doi:10.1016/S0030-4018(98)00654-3.

Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0013-5850-7

Zusammenfassung

We describe a system for complete autoalignment of a suspended, power-recycled Michelson interferometer. All ten angular degrees of freedom are controlled by servo systems, thus ensuring optimal interference and fixing all beams in space. The methods and results are applicable to laser-interferometric gravitational wave detectors, and possibly also to other types of sensitive interferometers.