GC12-FibreOptic-67, updated on 06 May 2024
https://doi.org/10.5194/egusphere-gc12-fibreoptic-67
Galileo conference: Fibre Optic Sensing in Geosciences
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

What we learn from multi-component, direct observations of rotational ground motions about atmospheric ground deformation processes

Andreas Brotzer1, Heiner Igel1, and Rudolf Widmer-Schnidrig2
Andreas Brotzer et al.
  • 1Ludwig-Maximilians Universität München, Geophysical Observatory, Department of Earth and Environmental Sciences, Fuerstenfeldbruck, Germany (andreas.brotzer@lmu.de)
  • 2University of Stuttgart, Institute of Geodesy, Black Forest Observatory, Wolfach, Germany

A high-sensitive, large-scale optical Sagnac gyroscope provides access to direct observations of the rotational part of the gradient of the seismic wavefield. A tetrahedral configuration of optical Sagnac gyroscopes, such as ROMY (ROtational Motions in seismologY), located in a Geophysical Observatory near Munich, Germany, enables to redundantly observe all three components of the curl of the displacement field.
For seismic accelerations below 30 mHz, the separation of low noise background levels between vertical and horizontal component are well established and understood to result from local tilts driven by atmospheric pressure variations. The promise of multi-component rotational observations is that ideally they can be used to decontaminate a co-located horizontal component acceleration sensor from contributions of ground tilt. Moreover, knowing and understanding the background levels for vertical and horizontal rotational ground motions at long periods can refine our current understanding of the low noise model for ground motions and is essential as a benchmark for instrument development.
We use several months of multi-component data of vertical and horizontal rotation rates by ROMY and a co-located atmospheric pressure sensor to derive the pressure compliance for both vertical and horizontal rotational motions. Focusing on frequencies below 20 mHz, we find that time windows with energetic weather patterns consistently lead to high coherence of atmospheric pressure and horizontal rotations, but only little coherence between the atmospheric pressure and vertical rotation.
We consider this as a first indication that atmospheric pressure induced ground tilts are detected by the ROMY horizontal components. Different effects of ambient atmospheric pressure changes on the optical gyroscope itself, such as cavity deformation, are discussed. A small aperture barometer array surrounding ROMY provides observations of lateral pressure gradients to provide additional constraints on ground deformations from atmospheric pressure waves.

How to cite: Brotzer, A., Igel, H., and Widmer-Schnidrig, R.: What we learn from multi-component, direct observations of rotational ground motions about atmospheric ground deformation processes, Galileo conference: Fibre Optic Sensing in Geosciences, Catania, Italy, 16–20 Jun 2024, GC12-FibreOptic-67, https://doi.org/10.5194/egusphere-gc12-fibreoptic-67, 2024.