2003
DOI: 10.1016/s0273-1177(03)00175-3
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Analytical short-term orbit prediction with J2 , J3, J4 in terms of K-S uniformly regular canonical elements

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Cited by 8 publications
(6 citation statements)
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“…Only one of the eight equations needs to be integrated analytically to generate the state vector, as a result of symmetry in the equations of motion, and the computation for the other equations is by changing the initial conditions. The integrals are much simpler than earlier obtained in [20] in terms of the independent variable 's'. Numerical results indicate that the solution is reasonably accurate for a wide range of orbital parameters during a revolution.…”
Section: Introductionmentioning
confidence: 87%
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“…Only one of the eight equations needs to be integrated analytically to generate the state vector, as a result of symmetry in the equations of motion, and the computation for the other equations is by changing the initial conditions. The integrals are much simpler than earlier obtained in [20] in terms of the independent variable 's'. Numerical results indicate that the solution is reasonably accurate for a wide range of orbital parameters during a revolution.…”
Section: Introductionmentioning
confidence: 87%
“…The integrals are found to be much simpler than obtained in [20]. The solution can have number of applications.…”
Section: Introductionmentioning
confidence: 92%
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“…Analytical theory in terms of KS elements with J2 [14] and [16], and with J3 and J4 [15] was developed for short-term orbit predictions. [8] analytically integrated the uniformly regular KS canonical elements with Earth's zonal harmonics J2, J3 and J4. The independent variable, fictitious time 's' given by dt/ds = r with t and r being the physical time and radial distance, respectively, and used for analytical integration, resulted in complicated integrals.…”
Section: Introductionmentioning
confidence: 99%
“…{18] developed a new non-singular analytical solution with J2 in close form in eccentricity 'e' for short-term orbit predictions by analytically integrating the uniformly regular KS canonical equations of motion, using the generalized eccentric anomaly 'E' as the independent variable. The integrals are found to be much simpler than obtained in [8]. In this paper, the analytical solution of [18] is improved by using King-Hele's expression [10] for radial distance r as function of J2.…”
Section: Introductionmentioning
confidence: 99%