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Ring laser gyroscope

Instrument to measure angular velocity

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  • 4 chapters

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Description

The first experimental ring laser gyroscope was demonstrated in the US by Macek and Davis in 1963. Various organizations worldwide subsequently developed ring-laser technology further. Many tens of thousands of RLGs are operating in inertial navigation systems and have established high accuracy, with better than 0.01°/hour bias uncertainty, and mean time between failures in excess of 60,000 hours.

Ring laser gyroscopes can be used as the stable elements (for one degree of freedom each) in an inertial reference system. One key advantage of the RLG is that there are no moving parts apart from the dither motor assembly (see further description below). Compared to the conventional spinning gyroscope, this means there is no friction, which eliminates a significant source of drift. Additionally, the entire unit is compact, lightweight and highly durable, making it suitable for use in mobile systems such as aircraft, missiles, and satellites. Unlike a mechanical gyroscope, the device does not resist changes to its orientation.

Contemporary applications of the ring laser gyroscope include an embedded GPS capability to further enhance accuracy of RLG inertial navigation systems on military aircraft, commercial airliners, ships, and spacecraft. These hybrid INS/GPS units have replaced their mechanical counterparts in most applications.

"Ring laser gyroscopes (RLG) have demonstrated to currently be the most sensitive device for testing rotational motion with respect to an inertial frame." The lower noise limit of an active ring laser have been recently measured at the Gran Sasso National Laboratory of INFN (Italy) on the GINGERINO prototype. The measured noise level is below the calculated shot noise for a RLG where the counterpopagating beams are considered two coherent totally independent modes. Actually this discrepancy is supposed to be related to cross-coupling among the two modes.

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