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dc.contributor.authorGe, ZMen_US
dc.contributor.authorChen, HKen_US
dc.date.accessioned2014-12-08T15:02:03Z-
dc.date.available2014-12-08T15:02:03Z-
dc.date.issued1997-02-01en_US
dc.identifier.issn0021-4922en_US
dc.identifier.urihttp://hdl.handle.net/11536/764-
dc.description.abstractSufficient conditions for the global stability of equilibrium positions of a dual-spin satellite in a circular orbital system in a Newtonian central force field are obtained by Liapunov's direct method. The new results are compared with those already known. The problem is then studied with respect to all variables, including the angular velocity of the rotor. Further, sufficient conditions for the global stability of rotation with arbitrary angular velocity for an axisymmetric dual-spin satellite are presented by Liapunov's direct method, which improve on Kane's result of infinitesimal stability obtained by linearized equations of motion.en_US
dc.language.isoen_USen_US
dc.subjectglobal stabilityen_US
dc.subjectdual-spin satelliteen_US
dc.subjectLiapunov's direct methoden_US
dc.titleImproved stability of a dual-spin satellite in circular orbiten_US
dc.typeArticleen_US
dc.identifier.journalJAPANESE JOURNAL OF APPLIED PHYSICS PART 1-REGULAR PAPERS SHORT NOTES & REVIEW PAPERSen_US
dc.citation.volume36en_US
dc.citation.issue2en_US
dc.citation.spage948en_US
dc.citation.epage956en_US
dc.contributor.department交大名義發表zh_TW
dc.contributor.department機械工程學系zh_TW
dc.contributor.departmentNational Chiao Tung Universityen_US
dc.contributor.departmentDepartment of Mechanical Engineeringen_US
dc.identifier.wosnumberWOS:A1997WN16000066-
dc.citation.woscount0-
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