Characterization of X-Ray Pulsar Navigation for Tracking Closed Earth Orbits
2019; American Institute of Aeronautics and Astronautics; Volume: 42; Issue: 10 Linguagem: Inglês
10.2514/1.g003677
ISSN1533-3884
Autores Tópico(s)Advanced Frequency and Time Standards
ResumoNo AccessEngineering NotesCharacterization of X-Ray Pulsar Navigation for Tracking Closed Earth OrbitsWayne H. YuWayne H. YuNASA Goddard Space Flight Center, Greenbelt, Maryland 20771Published Online:3 Jul 2019https://doi.org/10.2514/1.G003677SectionsRead Now ToolsAdd to favoritesDownload citationTrack citations ShareShare onFacebookTwitterLinked InRedditEmail About References [1] Montenbruck O., Van Helleputte T., Kroes R. and Gill E., "Reduced Dynamic Orbit Determination Using GPS Code and Carrier Measurements," Aerospace Science and Technology, Vol. 9, No. 3, 2005, pp. 261–271. doi:https://doi.org/10.1016/j.ast.2005.01.003 CrossrefGoogle Scholar[2] Sheikh S. I., "The Use of Variable Celestial X-Ray Sources for Spacecraft Navigation," Ph.D. Thesis, Univ. of Maryland, College Park, MD, 2005, http://hdl.handle.net/1903/2856. Google Scholar[3] Hanson J. 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TopicsAstronomical ObservatoryAstronomyCelestial Coordinate SystemCelestial MechanicsControl TheoryGlobal Positioning SystemGuidance, Navigation, and Control SystemsKalman FilterPlanetary Science and ExplorationPlanetsSatellite BroadcastingSatellite Navigation SystemsSatellite TechnologySatellite-Based ServicesSpace MissionsSpace Science and TechnologySpacecraft Guidance and ControlTelescopes KeywordsEarthExtended Kalman FilterGPSRight AscensionDSNInterplanetary TrajectoriesPeriapsisInternational Space StationSpacecraft DynamicsGround StationAcknowledgmentsThis research was a master's thesis funded by the NASA Goddard Spaceflight Center's Academic Investment for Mission Success work study program. The author would like to thank Keith Gendreau, Zaven Arzoumanian, Jason Mitchell, Luke Winternitz, and Liam Healy for their input on this study. Software Routines from the International Astronautical Union Standards of Fundamental Astronomy Collection were used (http://www.iausofa.org). This research has made use of data, software, and/or web tools obtained from NASA's High Energy Astrophysics Science Archive Research Center (HEASARC), a service of Goddard Space Flight Center and the Smithsonian Astrophysical Observatory.PDF Received29 October 2018Accepted27 May 2019Published online3 July 2019
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