Highly sensitive wideband seismometer using a laser interferometer
- 1 May 1993
- journal article
- Published by AIP Publishing in Review of Scientific Instruments
- Vol. 64 (5) , 1337-1341
- https://doi.org/10.1063/1.1144089
Abstract
A wideband (dc to 2 kHz) highly sensitive seismometer using a Michelson laser interferometer has been developed. The horizontal acceleration of the ground is sensed by a suspended mirror; its position is then detected as the fringe signal of the light in the interferometer. The minimum measurable displacement with this seismometer is 3×10−11 m/√Hz at 1 Hz (limited by the thermal fluctuation of air and the frequency noise of the laser) and 2×10−15 m/√Hz above 2 kHz (limited by the shot noise of the light). One application of this seismometer is to use it for very sensitive vibration measurements, such as in seismic noise investigations of possible sites for a large-scale laser-interferometric gravitational wave detector.Keywords
This publication has 9 references indexed in Scilit:
- High-frequency seismic noise as a function of depthBulletin of the Seismological Society of America, 1991
- High frequency (1–100 HZ) noise and signal recorded at different depths in a mine, northwest Adirondacks, NYGeophysical Research Letters, 1990
- Noise behavior of the Garching 30-meter prototype gravitational-wave detectorPhysical Review D, 1988
- Performance of a gas spring harmonic oscillatorReview of Scientific Instruments, 1988
- Observation of a neutrino burst from the supernova SN1987APhysical Review Letters, 1987
- Frequency stabilization of a HeNe laser using a thin film heater coated on the laser tubeOptics Communications, 1985
- Comments on: Frequency Stabilization of Internal Mirror He–Ne LasersApplied Optics, 1973
- Frequency Stabilization of Internal-Mirror Helium–Neon LasersApplied Optics, 1972
- Photon-Noise-Limited Laser Transducer for Gravitational AntennaApplied Optics, 1971