EGU24-9603, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-9603
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Accurate Inertial Earth Rotation Measurements

Karl Ulrich Schreiber and Jan Kodet
Karl Ulrich Schreiber and Jan Kodet
  • Technische Universitaet Muenchen, Forschungseinrichtung Satellitengeodaesie, Geodaetisches Observatorium Wettzell, Bad Koetzting, Germany (ulrich.schreiber@tum.de)

The complex interaction between the fluids of the Earth and the solid Earth results in small variations in the rotational velocity of the Earth at the level of ∆Ω ≈ 10e-8, which are not predictable. These signals are usually observed utilizing the GNSS constellation and the global IGS receiver network. Stability is provided by the VLBI technique. Inertial Earth rotation sensing, based on ring laser gyroscopes, is now capable of detecting these signals with high temporal resolution. Therefore it is important to closely examine the inherent accuracy of the utilized gyroscope technology. 

This presentation outlines the latest improvements in sensor operation, reviews some crucial sensor properties and puts them into perspective with the established techniques in space geodesy.

How to cite: Schreiber, K. U. and Kodet, J.: Accurate Inertial Earth Rotation Measurements, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9603, https://doi.org/10.5194/egusphere-egu24-9603, 2024.