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Development of a high-resolution optical inertial sensor for sub-Hz seismic isolation

Watchi, Jennifer and Ding, Binlei and Matichard, Fabrice and Collette, Christophe (2016) Development of a high-resolution optical inertial sensor for sub-Hz seismic isolation. In: Proceedings of ISMA2016 International Conference on Noise and Vibration Engineering and USD2016 International Conference on Uncertainty in Structural Dynamics. Katholieke Universiteit , Heverlee, Belgium, pp. 275-288. ISBN 978-90-73802-94-0. http://resolver.caltech.edu/CaltechAUTHORS:20170224-075907420

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Abstract

Precision engineering tasks require active isolation systems that are efficient especially at low frequencies. The limitations of such control systems include the resolution of the sensor used and the magnetic coupling between the sensor and the actuator. In order to bypass these limitations, inertial sensors using Michelson interferometer are being developed. A first prototype has been built and tested. It has been shown that it has a sub-nanometer resolution over a large frequency range, extending from 0.1 Hz to 100 Hz. To further improve the resolution, a new optical design will be presented in this paper. The elements of the setup are chosen to lower the noise of the whole system. Actually, two main sources of noise can be reduced. The first one is due to the optical components, inducing a phase shift which is converted into a displacement error. The second is a consequence of the pendulum movement of the piece/spring holding the moving mass. It couples the vertical translation and the rotation. By choosing correctly the optical components, the first source can be diminished. The resolution reached is compared with that predicted by the optical model implemented on MATLAB. With the best optical resolution of the setup achieved, the interferometer had been integrated into a STS1 seismometer to reduce the pendulum movement. The optical sensor replaces the conventional capacitive sensor of the device without disturbing the mechanical parts. The resulting modified STS1 has a spectral resolution below 10^(-13) m/rtHz, while at the same time is insensitive to magnetic field. The final objective of this research consists in introducing the inertial sensor into a single-axis isolation system equipped with a voice coil actuator. In feedback configuration, the setup will allow to reach an unprecedented high level of isolation, opening a new window in gravimetry and gravitational wave detection.


Item Type:Book Section
Additional Information:© 2016 Katholieke Universiteit.
Group:LIGO
Funders:
Funding AgencyGrant Number
Fonds de la Recherche Scientifique (FNRS)UNSPECIFIED
NSFPHY-0107417
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentLIGO-P1600214
Record Number:CaltechAUTHORS:20170224-075907420
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170224-075907420
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74519
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 Feb 2017 18:22
Last Modified:24 Feb 2017 18:22

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