2017
DOI: 10.1007/s40295-017-0118-4
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Unified Lambert Tool for Massively Parallel Applications in Space Situational Awareness

Abstract: This paper introduces a parallel-compiled tool that combines several of our recently developed methods for solving the perturbed Lambert problem using modified Chebyshev-Picard iteration. This tool (unified Lambert tool) consists of four individual algorithms, each of which is unique and better suited for solving a particular type of orbit transfer. The first is a Keplerian Lambert solver, which is used to provide a good initial guess (warm start) for solving the perturbed problem. It is also used to determine… Show more

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Cited by 9 publications
(3 citation statements)
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“…Later, Koblick and Shankar [15] extended the analysis to the propagation of accurate orbits testing difference force models with NASA's Java Astrodynamics toolkit. Woollands et al [16][17][18] applied the method as numerical integrator for the solution of the Lambert two-point boundary value problem, assessing also the benefits of adopting the Kuustanheimo-Stiefel formulation of the dynamics and proposing a solution for the multi-revolution trajectory design. Swenson et al [19] applied the modified PC method on the circular restricted three-body problem, using the differential correction approach.…”
Section: Introductionmentioning
confidence: 99%
“…Later, Koblick and Shankar [15] extended the analysis to the propagation of accurate orbits testing difference force models with NASA's Java Astrodynamics toolkit. Woollands et al [16][17][18] applied the method as numerical integrator for the solution of the Lambert two-point boundary value problem, assessing also the benefits of adopting the Kuustanheimo-Stiefel formulation of the dynamics and proposing a solution for the multi-revolution trajectory design. Swenson et al [19] applied the modified PC method on the circular restricted three-body problem, using the differential correction approach.…”
Section: Introductionmentioning
confidence: 99%
“…specified angular momentum vector, and applied it to the design of low thrust trajectories. Woollands et al [55] developed a Lambert solver based on KS coordinates and used it to provide a good initial guess to the Picard-Chebyshev numerical integration of the perturbed two-body problem. Sellamuthu and Sharma analysed the J 2 , J 3 , J 4 terms of Earth's oblateness and the third body luni-solar perturbation when approximated with a Legendre polynomial expansion with KS coordinates [56][57][58].…”
Section: Introductionmentioning
confidence: 99%
“…This kind of problem is abbreviated as the minimum velocity increment problem (MVIP) in this paper. It is worth noting that the aforementioned algorithms cannot be directly applied to the MVIP, because the TOF should be regarded as an unspecified parameter in the optimization process [30][31][32]. Commonly, an additional single-variable algorithm needs to be developed to repeatedly solve Lambert's problem so as to determine the optimal TOF.…”
Section: Introductionmentioning
confidence: 99%