Radial, transverse and normal satellite position perturbations due to the geopotential

DOI10.1007/BF01235855zbMath0698.70022OpenAlexW2016748071MaRDI QIDQ3476329

G. W. Rosborough, B. D. Tapley

Publication date: 1987

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01235855

zbMATH Keywords

Earth's gravitational effectsKepler element perturbationsposition of a satellite

Mathematics Subject Classification ID

Orbital mechanics (70M20) Statics (70C20) Nonlinear resonances for nonlinear problems in mechanics (70K30)

Related Items (8)

The gravitational perturbation spectrum in linear satellite theory ⋮ A new method for computing the spectrum of the gravitational perturbations on satellite orbits ⋮ Tesseral harmonic perturbations in radial transverse and binormal components ⋮ Rosborough approach for the determination of regional time variability of the gravity field from satellite gradiometry data ⋮ Position and velocity perturbations for the determination of geopotential from space geodetic measurements ⋮ Position and velocity perturbations in the orbital frame in terms of classical element perturbations ⋮ The mapping of Kaula's solution into the orbital reference frame ⋮ First-order theory of weakly eccentric orbital motion

Cites Work

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• A linear solution of the equations of motion of an earth-orbiting satellite based on a Lie-series
• Along-track oscillations of a satellite due to tesseral harmonics.
• Linearized solutions for a circular orbit perturbed by tesseral harmonics.
• Satellite resonances and librations associated with Tesseral harmonics of the geopotential
• Tesseral resonance effects on satellite orbits

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