A laser gyroscope system to detect the Gravito-Magnetic effect on Earth
A. Di Virgilio, K. U. Schreiber, A. Gebauer, J-P. R. Wells, A., Tartaglia, J. Belfi, N. Beverini, A.Ortolan

TL;DR
This paper discusses a large-scale laser gyroscope system designed to detect Earth's gravitomagnetic effect, analyzing configurations of multiple gyros for optimal sensitivity and noise reduction.
Contribution
It introduces a twin gyro configuration with controllable relative angles and evaluates its potential to measure Earth's gravitomagnetic effect with high sensitivity.
Findings
A four-meter square ring laser gyroscope approaches the sensitivity needed to detect the Lense-Thirring effect.
A quadruple twin gyro system could achieve 1% sensitivity in about 3.5 years under ideal conditions.
Adding more gyros improves signal-to-noise ratio and provides intra-system bias checks.
Abstract
Large scale square ring laser gyros with a length of four meters on each side are approaching a sensitivity of 1x10^-11 rad/s/sqrt(Hz). This is about the regime required to measure the gravitomagnetic effect (Lense Thirring) of the Earth. For an ensemble of linearly independent gyros each measurement signal depends upon the orientation of each single axis gyro with respect to the rotational axis of the Earth. Therefore at least 3 gyros are necessary to reconstruct the complete angular orientation of the apparatus. In general, the setup consists of several laser gyroscopes (we would prefer more than 3 for sufficient redundancy), rigidly referenced to each other. Adding more gyros for one plane of observation provides a cross-check against intra-system biases and furthermore has the advantage of improving the signal to noise ratio by the square root of the number of gyros. In this paper…
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