Tesseral harmonic perturbations in radial transverse and binormal components

DOI10.1007/BF00049391zbMath1375.70013MaRDI QIDQ1685329

Edwin Wnuk, Sławomir Breiter

Publication date: 13 December 2017

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

zbMATH Keywords

artificial satelliteEarth artificial satelliteorbital elementartificial satellite motionharmonic perturbation

Mathematics Subject Classification ID

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

Related Items (3)

A new method for computing the spectrum of the gravitational perturbations on satellite orbits ⋮ Analytical treatment of the Earth oblateness and solar radiation pressure effects on an artificial satellite. I: The equations of motion. ⋮ Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential

Cites Work

• Unnamed Item
• Radial, transverse and normal satellite position perturbations due to the geopotential
• Tesseral harmonic perturbations for high order and degree harmonics

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