Tesseral harmonic perturbations for high order and degree harmonics

DOI10.1007/BF01230714zbMath0662.70008MaRDI QIDQ3813352

Edwin Wnuk

Publication date: 1988

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

zbMATH Keywords

geopotentialorbital elementstesseral harmonic perturbationsHori's perturbation methodGRM satellites

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Statics (70C20)

Related Items (8)

Closed-form perturbation theory in the restricted three-body problem without relegation ⋮ Exact Delaunay normalization of the perturbed Keplerian Hamiltonian with tesseral harmonics ⋮ The gravitational perturbation spectrum in linear satellite theory ⋮ On the inclination functions and a rapid stable procedure for their evaluation together with derivatives ⋮ Tesseral harmonic perturbations in radial transverse and binormal components ⋮ First-order accurate theory of perturbed circular motion ⋮ Kepler problem with time-dependent and resonant perturbations ⋮ Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential

Cites Work

• Unnamed Item
• Gravitational harmonics from shallow resonant orbits
• The main problem of artificial satellite theory for small and moderate eccentricities
• A recurrence relation for inclination functions

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