Abstract
We present a modified commercial L-4C geophone with interferometric readout that demonstrates a resolution 60 times lower than the included coil-magnet readout at low frequencies. The intended application for the modified sensor is in vibration isolation platforms that require improved performance at frequencies lower than 1 Hz. To illustrate it's application a controls- and noise-model of an Advanced LIGO 'HAM-ISI' vibration isolation system was developed, and shows that our sensor can reduce the residual motion of the platforms by a factor of 70 at 0.1 Hz.
| Original language | English |
|---|---|
| Article number | 075023 |
| Pages (from-to) | 1-11 |
| Number of pages | 11 |
| Journal | Classical and Quantum Gravity |
| Volume | 39 |
| Issue number | 7 |
| Early online date | 17 Mar 2022 |
| DOIs | |
| Publication status | Published - 7 Apr 2022 |
Bibliographical note
Funding Information:We thank John Bryant for technical support, Maura Shea and Isaac Davis for integration and testing of the data acquisition systems used in this project. The authors acknowledge the support of the Institute for Gravitational Wave Astronomy at the University of Birmingham, STFC ‘Astrophysics at the University of Birmingham’ Grant ST/S000305/1.
Publisher Copyright:
© 2022 The Author(s). Published by IOP Publishing Ltd.
Funding
We thank John Bryant for technical support, Maura Shea and Isaac Davis for integration and testing of the data acquisition systems used in this project. The authors acknowledge the support of the Institute for Gravitational Wave Astronomy at the University of Birmingham, STFC ‘Astrophysics at the University of Birmingham’ Grant ST/S000305/1.
| Funders | Funder number |
|---|---|
| University of Birmingham | |
| Science and Technology Facilities Council | |
| UK Research and Innovation | ST/S000305/1 |
Keywords
- homodyne detection
- inertial sensing
- interferometry
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