Development of a relative motion model for satellite formation flying around L2

dc.contributor.authorRoberts, Jennifer A.en_UK
dc.date.accessioned2005-11-22T13:33:35Z
dc.date.available2005-11-22T13:33:35Z
dc.date.issued2004-12-18T10:57:38Zen_UK
dc.descriptionPaper given at Dynamics and Control of Systems and Structures in Space (DCSSS), 6th conference, Riomaggiore, Italy, July 2004en_UK
dc.description.abstractA technique for satellite formation flying modelling in LEO is applied at L2. Analytical solutions to the equations of motion of a hub satellite relative to L2 are used to define a halo reference orbit. An expression for the gravity gradient is obtained at the hub and the linearised equations of motion of the mirror satellites relative to the hub are derived. The relative motion model is implemented in Matlab/Simulink and evaluated for different initial conditions. The analytical solutions to the equations of relative motion are derived. These and other equations of motion are compared to the Satellite Tool Kit numerical orbit propagator.en_UK
dc.format.extent1883 bytes
dc.format.extent321901 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.identifier.urihttp://hdl.handle.net/1826/788
dc.language.isoen_UKen_UK
dc.publisherCranfield University; School of Engineeringen_UK
dc.titleDevelopment of a relative motion model for satellite formation flying around L2en_UK
dc.typePresentationen_UK

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