A better approximation for period on radially perturbed orbits

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  • Vasile Mioc Astronomical Observatory, Cluj-Napoca, Romania
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References

Blaga, P., Mioc, V., Elliptic-Type Motion in a Schwarzschild-De Gravitational Field, Europhys., Lett., 17 (1992), pp. 275-278, https://doi.org/10.1209/0295-5075/17/3/015

Mioc, V., the Difference between the Nodal and Keplerian Periods of an Artificial Satellite as an Effect of Atmospheric Drag, Astron. Nachr., 301 (1980), pp. 311-315, https://doi.org/10.1002/asna.2103010608

Mioc, V., The Lorentz Force Effects in the Period of Artificial Satellites, Rev. Roum. Phys., 33 (1988), pp. 1295-1300.

Mioc, V., Extension of a Method for Nodal Period Determination in Perturbed Orbital Motion, Romanian Astron. J., 2 (1992), (in press).

Mioc, V., Blaga, P., Orbital Motion with the Mücket-Treder Post-Newtoian Gravitational Law, Romanian Astron. J., 1 (1991), pp. 103-108.

Mioc, V., Radu, E., Some Radiation Effects in the Nodal Period of Artificial Satellites, Studia Univ. Babeş-Bolyai, ser. Mathematica, 25(1980), No.2, pp. 22-31.

Mioc, V., Radu, E., Perturbation in the Nodal Period of Artificial Satellites caused by the Terrestrial Infrared Radiation Pressure, Astron. Nachr., 303 (1982), pp. 313-315, https://doi.org/10.1002/asna.2103030509

Zhongolovich, I.D., Some Formulae Occuring in the Motion of a Material point in the Attraction Field of a Rotation Level Ellipsoid, Byull, Inst. Teor, Astron., 7 (196), pp. 521-536 (Russ.).

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Published

1993-08-01

How to Cite

Mioc, V. (1993). A better approximation for period on radially perturbed orbits. Rev. Anal. Numér. Théor. Approx., 22(2), 201–205. Retrieved from https://ictp.acad.ro/jnaat/journal/article/view/1993-vol22-no2-art10

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Vol. 22 No. 2 (1993)

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Copyright (c) 2015 Journal of Numerical Analysis and Approximation Theory

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