Planetary motion calculation method

Authors

  • HAROLD CITRYNELL

DOI:

https://doi.org/10.54302/mausam.v27i2.2435

Abstract

An accurate method for calculating the unperturbed motion and position of the earth, a planet, or a satellite, moving in an elliptical orbit, as a function of time, is presented. The method is easy to apply and is suitable for use in the modelling of various type of problem in meteorology and geophysics.

 

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Published

1976-04-01

Issue

Vol. 27 No. 2 (1976): MAUSAM

Section

Shorter Contribution

Categories

License

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How to Cite

[1]
“Planetary motion calculation method”, MAUSAM, vol. 27, no. 2, pp. 185–186, Apr. 1976, doi: 10.54302/mausam.v27i2.2435.