Dynamics of Satellites (1969) 1970
DOI: 10.1007/978-3-642-99966-6_32
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Radiation Pressure Effects in the Motion of Artificial Satellites

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Cited by 10 publications
(4 citation statements)
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“…Where, the dynamic accelerationã consists of the following ones: [1] two-body gravitational attractions of Earthã TB , [2] N-body gravitational attractions of the Sun, Moon and so onã NB , [3] relativistic perturbationã RL , [4] gravitational attractions of the non-spherical Earthã NS (Earth gravity model JGM3 (Tapley et al, 1996;Xu, 2007;Xu and Xu, 2013), truncated to the 10th degree and order), [5] gravitational attractions of solid-Earth tides , oceanic tides and atmospheric tides a TD (Li, 1995;Wahr, 1981;Xu, 2007;Xu and Xu, 2013;McCarthy and Petit, 2004), [6] perturbation of Earth's rotational deformationã ED (Buffett et al, 1993), [7] radiation pressure of the Sunã SR (Tapley et al, 2004;Parkinson et al, 1960;Xu, 2007;Xu and Xu, 2013;McCarthy and Petit, 2004), [8] Earth albedo radiation pressureã ER (Sehnal, 1980;Borderies and Longaretti, 1990), [9] empirical radial-transverse-normal accelerations a TR (Huang et al, 2011;Eanes and Bettaadpur, 1996) and…”
Section: Orbit Determination Strategy During Repositioning Maneuvermentioning
confidence: 99%
“…Where, the dynamic accelerationã consists of the following ones: [1] two-body gravitational attractions of Earthã TB , [2] N-body gravitational attractions of the Sun, Moon and so onã NB , [3] relativistic perturbationã RL , [4] gravitational attractions of the non-spherical Earthã NS (Earth gravity model JGM3 (Tapley et al, 1996;Xu, 2007;Xu and Xu, 2013), truncated to the 10th degree and order), [5] gravitational attractions of solid-Earth tides , oceanic tides and atmospheric tides a TD (Li, 1995;Wahr, 1981;Xu, 2007;Xu and Xu, 2013;McCarthy and Petit, 2004), [6] perturbation of Earth's rotational deformationã ED (Buffett et al, 1993), [7] radiation pressure of the Sunã SR (Tapley et al, 2004;Parkinson et al, 1960;Xu, 2007;Xu and Xu, 2013;McCarthy and Petit, 2004), [8] Earth albedo radiation pressureã ER (Sehnal, 1980;Borderies and Longaretti, 1990), [9] empirical radial-transverse-normal accelerations a TR (Huang et al, 2011;Eanes and Bettaadpur, 1996) and…”
Section: Orbit Determination Strategy During Repositioning Maneuvermentioning
confidence: 99%
“…The dynamic acceleration consists of the following: (1) two-body gravitational attractions of the Earth, (2) N-body gravitational attractions of the Sun and Moon, (3) relativistic perturbation, (4) gravitational attractions of the non-spherical Earth (Earth gravity model JGM3, truncated to the 10th degree and order) (Tapley et al, 1996; Xu, 2007; Xu and Xu, 2013), (5) gravitational attractions of solid-Earth tides, oceanic tides and atmospheric tides (Wahr, 1981; Li, 1995; McCarthy and Petit, 2004; Xu, 2007; Xu and Xu, 2013), (6) perturbation of Earth's rotational deformation (Buffett et al, 1993), (7) radiation pressure of the Sun (Parkinson et al, 1960; McCarthy and Petit, 2004; Tapley et al, 2004; Xu, 2007; Xu and Xu, 2013), (8) Earth albedo radiation pressure (Sehnal, 1980; Borderies and Longaretti, 1990) and (9) empirical radial-transverse-normal accelerations (Eanes and Bettaadpur, 1996; Huang et al, 2011; Cao, 2014c).…”
Section: The Signal Biases Calibration Of Caps Using Slr and Cbtrmentioning
confidence: 99%
“…The study of the effect of direct solar radiation pressure on the orbits of the artificial satellites was discussed in a lot of literatures, starting from pioneering works of [1][2][3][4] and other of [5][6][7][8][9]. Also the theory of third body perturbations on an artificial satellite motion was developed by many authors in the past.…”
Section: Introductionmentioning
confidence: 99%