Passive and active seismic isolation for gravitational radiation detectors and other instruments
Abstract
Some new passive and active methods for reducing the effects of seismic disturbances on suspended masses are described, with special reference to gravitational radiation detectors in which differential horizontal motions of two or more suspended test masses are monitored. In these methods it is important to be able to determine horizontal seismic accelerations independent of tilts of the ground. Measurement of changes in inclination of the suspension wire of a test mass, relative to a direction defined by a reference arm of long period of oscillation, makes it possible to carry this out over the frequency range of interest for earth-based gravitational radiation detectors. The signal obtained can then be used to compensate for the effects of seismic disturbances on the test mass if necessary. Alternatively the signal corresponding to horizontal acceleration can be used to move the point from which the test mass is suspended in such a way as to reduce the effect of the seismic disturbance and also damp pendulum motions of the suspended test mass. Experimental work with an active anti-seismic system of this type is described.
Additional Information
© 1982 The Institute of Physics Received 26 February 1982, in final form 20 May 1982 We acknowledge the financial support of the University of Glasgow and the Science and Engineering Research Council. We wish to thank R V Pound, Harvard University, for helpful private communications on some aspects of the system and D Murray Smith, Glasgow University, for useful advice on control systems.Attached Files
Published - ROBjpe82.pdf
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Additional details
- Eprint ID
- 1651
- Resolver ID
- CaltechAUTHORS:ROBjpe82
- University of Glasgow
- Science and Engineering Research Council (SERC)
- Created
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2006-02-09Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field