2016
DOI: 10.1016/j.actaastro.2016.08.016
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Spacecraft relative guidance via spatio-temporal resolution in atmospheric density forecasting

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Cited by 6 publications
(4 citation statements)
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“…In the same year, Cho et al [62] developed a chattering free sliding mode controller based on the insights from [57] and Peréz and Bevilacqua [63] proposed using artificial neuronal networks to predict the future behavior of the density in order to enhance the fidelity of the created guidance trajectories. The method was further advanced to reflect the dependence on spatial and temporal differences, donated as spatial-temporal resolution, in a follow-up publication by Guglielmo et al [64] published in the same year.…”
Section: Rendezvous Scenariomentioning
confidence: 99%
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“…In the same year, Cho et al [62] developed a chattering free sliding mode controller based on the insights from [57] and Peréz and Bevilacqua [63] proposed using artificial neuronal networks to predict the future behavior of the density in order to enhance the fidelity of the created guidance trajectories. The method was further advanced to reflect the dependence on spatial and temporal differences, donated as spatial-temporal resolution, in a follow-up publication by Guglielmo et al [64] published in the same year.…”
Section: Rendezvous Scenariomentioning
confidence: 99%
“…However, instead of a linear model, artificial neural networks were used. Even more realistic results can be obtained using a method denoted as spatiotemporal resolution developed by Guglielmo et al [64], which reflects the dependence of the density on both spatial and temporal differences [64,117]: "Spatiotemporal resolution can be achieved by propagating multiple orbits of spacecraft using a density forecast/estimate, varying the ballistic coefficient for each one. The density-location pairs result in the creation of a density field.…”
Section: Coping With Uncertaintiesmentioning
confidence: 99%
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“…The atmospheric density is allowed to be time varying, as is the case for real missions. Almost all prior work in differential drag, except for Guglielmo et al 20 , assumes a constant density. Intra-constellation coupling is also included when computing the control.…”
Section: Introductionmentioning
confidence: 99%