A 1.82 m^2 ring laser gyroscope for nano-rotational motion sensing

TL;DR

This paper introduces a highly sensitive, actively stabilized He-Ne ring laser gyroscope with low drift, capable of detecting nanoradian-level rotations, suitable for environmental noise measurement in gravitational wave detectors.

Contribution

The paper presents a novel 1.82 m^2 ring laser gyroscope with active control and low drift, demonstrating high rotational sensitivity for environmental noise monitoring.

Findings

Achieved rotational sensitivity of ten nanoradians per square root Hz below 1 Hz

Operated continuously for over 30 days in the Virgo detector environment

Demonstrated stability and sensitivity suitable for gravitational wave detector applications

Abstract

We present a fully active-controlled He-Ne ring laser gyroscope, operating in square cavity 1.35 m in side. The apparatus is designed to provide a very low mechanical and thermal drift of the ring cavity geometry and is conceived to be operative in two different orientations of the laser plane, in order to detect rotations around the vertical or the horizontal direction. Since June 2010 the system is active inside the Virgo interferometer central area with the aim of performing high sensitivity measurements of environmental rotational noise. So far, continuous not attempted operation of the gyroscope has been longer than 30 days. The main characteristics of the laser, the active remote-controlled stabilization systems and the data acquisition techniques are presented. An off-line data processing, supported by a simple model of the sensor, is shown to improve the effective long term stability. A rotational sensitivity at the level of ten nanoradiants per squareroot of Hz below 1 Hz, very close to the required specification for the improvement of the Virgo suspension control system, is demonstrated for the configuration where the laser plane is horizontal.