Simon Stellmer (Bonn) - Ring lasers for rotation sensing in the geosciences
Ring laser gyroscopes are highly sensitive inertial optical interferometers,
exploiting the Sagnac effect on two counter-propagating laser beams in a
ring cavity. Meter-sized and highly stable interferometers have been
developed in the past 30 years and reach a resolution of 0.3 prad/s after a
few hours of integration time. The rotation of Earth, including its
variations, is a commonly available signal used to benchmark the performance
of large ring lasers, which succeed to quantify variations in the
length-of-day (LoD) and to resolve the precession and nutation of Earth's
axis.
Similarily, ring laser gyroscopes can also be employed in the field of
seismology to reconstruct rotational motions in seismic wavefields. Building
on the technology of optical clocks and gravitational wave detection, new
developments are underway to realize so-called passive ring laser
gyroscopes. This approach relies on an external laser referenced to the
counterpropagating modes of a ring resonator and might allow for
miniaturization of sensors with large bandwidth.
In my presentation, I will trace the development of ring interferometers
over the past 100 years, and I will highlight future developments
specifically in the recently established DFG research unit RING.