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(1968) The contraction of satellite orbits under the influence of air drag - VI. Near-circular orbits with day-to-night variation in air density. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 303 (1472). 17-35 doi:10.1098/rspa.1968.0037

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Reference TypeJournal (article/letter/editorial)
TitleThe contraction of satellite orbits under the influence of air drag - VI. Near-circular orbits with day-to-night variation in air density
JournalProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences
Year1968 (February 6)Volume303
Issue1472
PublisherThe Royal Society
DOIdoi:10.1098/rspa.1968.0037Search in ResearchGate
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Mindat Ref. ID7361131Long-form Identifiermindat:1:5:7361131:8
GUID0
Full Reference(1968) The contraction of satellite orbits under the influence of air drag - VI. Near-circular orbits with day-to-night variation in air density. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 303 (1472). 17-35 doi:10.1098/rspa.1968.0037
Plain Text(1968) The contraction of satellite orbits under the influence of air drag - VI. Near-circular orbits with day-to-night variation in air density. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 303 (1472). 17-35 doi:10.1098/rspa.1968.0037
In(1968, February) Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences Vol. 303 (1472) The Royal Society

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(1965) The contraction of satellite orbits under the influence of air drag V. With day-to-night variation in air density. Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 259. 33-67 doi:10.1098/rsta.1965.0053
(1987) The contraction of satellite orbits under the influence of air drag. VII. Orbits of high eccentricity, with scale height dependent on altitude. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 411 (1840). 1-17 doi:10.1098/rspa.1987.0050
(1961) The contraction of satellite orbits under the influence of air drag. II. With oblate atmosphere. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 264 (1316). 88-121 doi:10.1098/rspa.1961.0186
(1960) The contraction of satellite orbits under the influence of air drag. I. With spherically symmetrical atmosphere. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 257 (1289). 224-249 doi:10.1098/rspa.1960.0146
(1963) The contraction of satellite orbits under the influence of air drag IV. With scale height dependent on altitude. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 275 (1362). 357-390 doi:10.1098/rspa.1963.0175
(1982) Contraction of satellite orbits in an oblate atmosphere with a diurnal density variation. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 383 (1784). 127-145 doi:10.1098/rspa.1982.0124
(1987) The contraction of satellite orbits under the influence of air drag. VIII. Orbital lifetime in an oblate atmosphere, when perigee distance is perturbed by odd zonal harmonics in the geopotential. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 414 (1847). 271-295 doi:10.1098/rspa.1987.0144
(1977) A study of near-circular satellite orbits: with an application to lunisolar perturbations. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 355 (1680). 131-140 doi:10.1098/rspa.1977.0090
(1962) The contraction of satellite orbits under the influence of air drag, III. High-eccentricity orbits (0·2≤ e <1). Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 267 (1331). 541-557 doi:10.1098/rspa.1962.0117
(1983) Near-circular satellite orbits in an oblate, diurnally varying atmosphere. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 389 (1796). 153-170 doi:10.1098/rspa.1983.0100
(1958) Method for computations of satellite orbits. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 248 (1252). 43-44 doi:10.1098/rspa.1958.0220
 
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