Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique

dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorDuev, D. A.en_US
dc.contributor.authorPogrebenko, S. V.en_US
dc.contributor.authorCimò, G.en_US
dc.contributor.authorMolera Calvés, G.en_US
dc.contributor.authorBocanegra Bahamón, T. M.en_US
dc.contributor.authorGurvits, L. I.en_US
dc.contributor.authorKettenis, M. M.en_US
dc.contributor.authorKania, J.en_US
dc.contributor.authorTudose, V.en_US
dc.contributor.authorRosenblatt, P.en_US
dc.contributor.authorMarty, J. C.en_US
dc.contributor.authorLainey, V.en_US
dc.contributor.authorDe Vicente, P.en_US
dc.contributor.authorQuick, J.en_US
dc.contributor.authorNickola, M.en_US
dc.contributor.authorNeidhardt, A.en_US
dc.contributor.authorKronschnabl, G.en_US
dc.contributor.authorPloetz, C.en_US
dc.contributor.authorHaas, R.en_US
dc.contributor.authorLindqvist, Michaelen_US
dc.contributor.authorOrlati, A.en_US
dc.contributor.authorIpatov, A. V.en_US
dc.contributor.authorKharinov, M. A.en_US
dc.contributor.authorMikhailov, A. G.en_US
dc.contributor.authorLovell, J. E Jen_US
dc.contributor.authorMcCallum, J. N.en_US
dc.contributor.authorStevens, J.en_US
dc.contributor.authorGulyaev, S. A.en_US
dc.contributor.authorNatush, T.en_US
dc.contributor.authorWeston, S.en_US
dc.contributor.authorWang, W. H.en_US
dc.contributor.authorXia, B.en_US
dc.contributor.authorYang, W. J.en_US
dc.contributor.authorHao, L. F.en_US
dc.contributor.authorKallunki, J.en_US
dc.contributor.authorWitasse, O.en_US
dc.contributor.departmentLomonosov Moscow State Universityen_US
dc.contributor.departmentJoint Institute for VLBI ERICen_US
dc.contributor.departmentNetherlands Institute for Radio Astronomyen_US
dc.contributor.departmentDepartment of Radio Science and Engineeringen_US
dc.contributor.departmentCAS - Shanghai Astronomical Observatoryen_US
dc.contributor.departmentDelft University of Technologyen_US
dc.contributor.departmentCarnegie Mellon Universityen_US
dc.contributor.departmentInstitute for Space Sciencesen_US
dc.contributor.departmentRoyal Observatory of Belgiumen_US
dc.contributor.departmentCentre national d'études spatialesen_US
dc.contributor.departmentObservatoire de Parisen_US
dc.contributor.departmentObservatorio de Yebesen_US
dc.contributor.departmentHartebeesthoek Radio Astronomy Observatoryen_US
dc.contributor.departmentFederal Agency for Cartography and Geodesyen_US
dc.contributor.departmentChalmers University of Technologyen_US
dc.contributor.departmentRadio Observatory Medicinaen_US
dc.contributor.departmentRussian Academy of Sciencesen_US
dc.contributor.departmentUniversity of Tasmaniaen_US
dc.contributor.departmentCSIROen_US
dc.contributor.departmentAuckland University of Technologyen_US
dc.contributor.departmentChinese Academy of Sciencesen_US
dc.contributor.departmentMetsähovi Radio Observatoryen_US
dc.contributor.departmentEuropean Space Agency - ESAen_US
dc.date.accessioned2017-05-11T07:14:45Z
dc.date.available2017-05-11T07:14:45Z
dc.date.issued2016-09-01en_US
dc.description.abstractContext. The closest ever fly-by of the Martian moon Phobos, performed by the European Space Agency's Mars Express spacecraft, gives a unique opportunity to sharpen and test the Planetary Radio Interferometry and Doppler Experiments (PRIDE) technique in the interest of studying planet-satellite systems. Aims. The aim of this work is to demonstrate a technique of providing high precision positional and Doppler measurements of planetary spacecraft using the Mars Express spacecraft. The technique will be used in the framework of Planetary Radio Interferometry and Doppler Experiments in various planetary missions, in particular in fly-by mode. Methods. We advanced a novel approach to spacecraft data processing using the techniques of Doppler and phase-referenced very long baseline interferometry spacecraft tracking. Results. We achieved, on average, mHz precision (30 μm/s at a 10 s integration time) for radial three-way Doppler estimates and sub-nanoradian precision for lateral position measurements, which in a linear measure (at a distance of 1.4 AU) corresponds to ∼50 m.en
dc.description.versionPeer revieweden
dc.format.extent10
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationDuev , D A , Pogrebenko , S V , Cimò , G , Molera Calvés , G , Bocanegra Bahamón , T M , Gurvits , L I , Kettenis , M M , Kania , J , Tudose , V , Rosenblatt , P , Marty , J C , Lainey , V , De Vicente , P , Quick , J , Nickola , M , Neidhardt , A , Kronschnabl , G , Ploetz , C , Haas , R , Lindqvist , M , Orlati , A , Ipatov , A V , Kharinov , M A , Mikhailov , A G , Lovell , J E J , McCallum , J N , Stevens , J , Gulyaev , S A , Natush , T , Weston , S , Wang , W H , Xia , B , Yang , W J , Hao , L F , Kallunki , J & Witasse , O 2016 , ' Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique : A test case of the Mars Express Phobos fly-by ' , Astronomy and Astrophysics , vol. 593 , A34 . https://doi.org/10.1051/0004-6361/201628869en
dc.identifier.doi10.1051/0004-6361/201628869en_US
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.otherPURE UUID: 511a4e34-e06b-47aa-8576-1591f57c239ben_US
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/511a4e34-e06b-47aa-8576-1591f57c239ben_US
dc.identifier.otherPURE LINK: http://www.scopus.com/inward/record.url?scp=84986309983&partnerID=8YFLogxKen_US
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/11611109/aa28869_16.pdfen_US
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/25509
dc.identifier.urnURN:NBN:fi:aalto-201705113893
dc.language.isoenen
dc.relation.ispartofseriesAstronomy and Astrophysicsen
dc.relation.ispartofseriesVolume 593en
dc.rightsopenAccessen
dc.subject.keywordAstrometryen_US
dc.subject.keywordMethods: data analysisen_US
dc.subject.keywordTechniques: interferometricen_US
dc.subject.keywordTechniques: miscellaneousen_US
dc.titlePlanetary Radio Interferometry and Doppler Experiment (PRIDE) techniqueen
dc.typeA1 Alkuperäisartikkeli tieteellisessä aikakauslehdessäfi
dc.type.versionpublishedVersion
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