Skip to main content
Log in

East-west stationkeeping requirements of 24-h satellites due to Earth's triaxiality and luni-solar effects

  • Published:
Celestial mechanics Aims and scope Submit manuscript

Abstract

Ignoring luni-solar perturbations, analytical solution for longitude deviation of the ‘stroboscopic’ mean center of 24-h satellites ground trace in the neighborhood of a prespecified station is obtained. The initial semimajor axis for two-maneuver east-west stationkeeping is then deduced. Finally, the luni-solar long and short period effects on this initial semimajor axis are discussed.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Escobal, P. 1968,Methods of Astrodynamics, John Wiley and Sons Inc., New York.

    Google Scholar 

  • Fisher, D.: 1972,Celes. Mech. 6, 447.

    Google Scholar 

  • Gedeon, G. S.: 1969,Celes. Mech,1, 167.

    Google Scholar 

  • Giacaglia, E. O.: 1973, Smithsonian Astrophysical Observatory, Special Report 352, Cambridge, Mass., October 1, 1973.

  • Kozai, Y.: 1973, Smithsonian Astrophysical Observatory, Special Report 349, Cambridge, Mass., February 1, 1973.

  • Kamel, A., Ekman, D., and Tibbitts, R.: 1973,Celes. Mech. 8, 129.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Kamel, A.A. East-west stationkeeping requirements of 24-h satellites due to Earth's triaxiality and luni-solar effects. Celestial Mechanics 12, 425–438 (1975). https://doi.org/10.1007/BF01595389

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01595389

Keywords

Navigation