Averaging tesseral effects: Closed form relegation versus expansions of elliptic motion

  1. Lara, M. 1
  2. San-Juan, J.F. 2
  3. López-Ochoa, L.M. 2
  1. 1 C/Columnas de Hercules 1, San Fernando, Spain
  2. 2 Universidad de La Rioja
    info

    Universidad de La Rioja

    Logroño, España

    ROR https://ror.org/0553yr311

Revista:
Mathematical Problems in Engineering

ISSN: 1024-123X

Año de publicación: 2013

Volumen: 2013

Páginas: 1-11

Tipo: Artículo

DOI: 10.1155/2013/570127 SCOPUS: 2-s2.0-84877285782 WoS: WOS:000318093100001 GOOGLE SCHOLAR lock_openAcceso abierto editor

Otras publicaciones en: Mathematical Problems in Engineering

Repositorio institucional: lock_openAcceso abierto Editor

Resumen

Longitude-dependent terms of the geopotential cause nonnegligible short-period effects in orbit propagation of artificial satellites. Hence, accurate analytical and semianalytical theories must cope with tesseral harmonics. Modern algorithms for dealing analytically with them allow for closed form relegation. Nevertheless, current procedures for the relegation of tesseral effects from subsynchronous orbits are unavoidably related to orbit eccentricity, a key fact that is not enough emphasized and constrains application of this technique to small and moderate eccentricities. Comparisons with averaging procedures based on classical expansions of elliptic motion are carried out, and the pros and cons of each approach are discussed. © 2013 Martin Lara et al.