Towards exact relativistic theory of Earth's geoid undulation
arXiv:1411.4205 · doi:10.1016/j.physleta.2015.02.046
Abstract
The present paper extends the Newtonian concept of the geoid in classic geodesy towards the realm of general relativity by utilizing the covariant geometric methods of the perturbation theory of curved manifolds. It yields a covariant definition of the anomalous (disturbing) gravity potential and formulate differential equation for it in the form of a covariant Laplace equation. The paper also derives the Bruns equation for calculation of geoid's height with full account for relativistic effects beyond the Newtonian approximation. A brief discussion of the relativistic Bruns formula is provided.
14 pages, no figures, several typos in equations, footnotes and bibliography were found and fixed
References in corpus (5)
- Gravity Probe B: Final Results of a Space Experiment to Test General Relativity
- A strontium lattice clock with inaccuracy and its frequency
- Testing General Relativity and gravitational physics using the LARES satellite
- Post-Newtonian Celestial Dynamics in Cosmology: Field Equations
- Dynamic Field Theory and Equations of Motion in Cosmology
Cited by in corpus (9)
- Low-Earth Orbit Determination from Gravity Gradient Measurements
- Chronometric geodesy: methods and applications
- Post-Newtonian reference-ellipsoid for relativistic geodesy
- Definition of the relativistic geoid in terms of isochronometric surfaces
- The Relativistic Geoid: Gravity Potential and Relativistic Effects
- Normal gravity field in relativistic geodesy
- Potentials for general-relativistic geodesy
- General Relativity and Geodesy
- Relativistic geoids and time dependence: quasilocal frames versus isochronometric surfaces