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• W4224215486 abstract "Free Access References Book Editor(s):Sami W Asmar, Sami W Asmar Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CaliforniaSearch for more papers by this author First published: 26 March 2022 https://doi.org/10.1002/9781119734178.biblio AboutPDFPDF ToolsRequest permissionExport citationAdd to favoritesTrack citation ShareShareShare a linkShare onFacebookTwitterLinked InRedditWechat Abbate , S.F. , Armstrong , J.W. , Asmar , S.W. , Barbinis , E. , Bertotti , B. , Fleischman , D. , Gatti , M. , Goltz , G.L. , Herrera , R.G. , Iess , L. , Lee , K.J. , Ray , T.L. , Tinto , M. , Tortora , P. , and Wahlquist , H. ( 2003 ). The Cassini gravitational wave experiment . In: Gravitational Wave Detection , (eds. M. Cruise and P. Saulson ), 4856 : 90 – 97 . Proceedings of the International Society for Optical Engineering (SPIE) . CrossrefGoogle Scholar Abbott , B.P. , the LIGO Scientific Collaboration and Virgo Collaboration . ( 2016 ). Observation of gravitational waves for a binary black hole merger . Physical Review Letters 116 ( 6 ): 061102 . CrossrefCASPubMedWeb of Science®Google Scholar Acton , C.H. ( 1996 ). Ancillary data services of NASA's navigation and ancillary information facility . Planetary and Space Science 44 ( 1 ): 65 – 70 . CrossrefWeb of Science®Google Scholar Allan , D.W. ( 1966 ). Statistics of atomic frequency standards . Proceedings of the IEEE 54 ( 2 ): 221-230 . CrossrefGoogle Scholar Allan , D.W. ( 2016 ). Historicity, strengths, and weaknesses of Allan variances and their general applications . Gyroscopy and Navigation 7 ( 1 ): 1 – 17 . CrossrefGoogle Scholar Allen , C.W. ( 1947 ). Interpretation of electron densities from corona brightness . Monthly Notices of the Royal Astronomical Society 107 ( 5–6 ): 426 – 432 . CrossrefCASWeb of Science®Google Scholar Aleksandrov , Y.N. , Alexandrov , Y.N. , Vasilyev , M.B. , Vyshlov , A.S. , Dubrovin , V.M. , Zaitsev , A.L. , Kolosov , M.A. , Savich , N.A. , Samovol , V.A. , Samoznaev , L.N. , and Sidorenko , A.I. ( 1977 ). Some results of dual-frequency radio occultation exploration of the night-time ionosphere of Venus with satellites Venera 9 and 10 . Space Research XVII : 663 – 666 . Google Scholar Ambrosini , R. , Asmar , S.W. , Bolli , P. , and Flamini , E. ( 2011 ). The planned space science utilizations of the new Sardinia 64-m radio telescope . Proceedings of the IEEE 99 ( 5 ): 875 – 880 . doi: 10.1109/JPROC.2010.2063690 . CrossrefWeb of Science®Google Scholar Anderson , A.J. ( 1971 ). Probability of long period gravitational radiation . Nature 229 : 547 – 548 . CrossrefCASPubMedWeb of Science®Google Scholar Anderson , J.D. ( 1974 ). Geodetic and dynamical properties of planets . Eos, Transactions American Geophysical Union 55 ( 5 ): 515 – 523 . Wiley Online LibraryWeb of Science®Google Scholar Anderson , J.D. , Armstrong , J.W. , Campbell , J.K. , Estabrook , F.B. , Krisher , T.P. , and Lau , E.L. ( 1992 ). Gravitation and celestial mechanics investigations with Galileo . Space Science Reviews 60 ( 1–4 ): 591 – 610 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Armstrong , J.W. , Estabrook , F.B. , Hellings , R.W. , Lau , E.K. , and Wahlquist , H.D. ( 1984 ). Pioneer 10 search for gravitational waves – no evidence for coherent radiation from Geminga . Nature 308 ( 5955 ): 158 – 160 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Campbell , J.K. , Ekelund , J.E. , Ellis , J. and Jordan , J.F. ( 2008 ). Anomalous orbital-energy changes observed during spacecraft flybys of Earth . Physical Review Letters 100 ( 9 ): 091102 . CrossrefPubMedWeb of Science®Google Scholar Anderson , J.D. , Campbell , J.K. , Jacobson , R.A. , Sweetnam , D.N. , Taylor , A.H. , Prentice , A.J.R. , and Tyler , G.L. ( 1987a ). Radio science with Voyager 2 at Uranus: Results on masses and densities of the planet and five principal satellites . Journal of Geophysical Research: Space Physics 92 ( A13 ): 14877 – 14883 . Wiley Online LibraryWeb of Science®Google Scholar Anderson , J.D. , Colombo , G. , Esposito , P.B. , Lau , E.L. , and Trager , G.B. ( 1987b ). The mass, gravity field, and ephemeris of Mercury . Icarus 71 ( 3 ): 337 – 349 . CrossrefCASWeb of Science®Google Scholar Anderson , J.D. , Jacobson , R.A. , Lau , E.L. , Moore , W.B. , Olsen , O. , Schubert , G. , and Thomas , P.C. ( 2001a ). Shape, mean radius, gravity field and interior structure of Ganymede . Bulletin of the American Astronomical Society 33 : 1101 . Google Scholar Anderson , J.D. , Jacobson , R.A. , Lau , E.L. , Moore , W.B. , and Schubert , G. ( 2001b ). Io's gravity field and interior structure . Journal of Geophysical Research: Planets 106 ( E12 ): 32963 – 32969 . Wiley Online LibraryGoogle Scholar Anderson , J.D. , Jacobson , R.A. , McElrath , T.P. , Moore , W.B. , Schubert , G. , and Thomas , P.C. ( 2001c ). Shape, mean radius, gravity field, and interior structure of Callisto . Icarus 153 ( 1 ): 157 – 161 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Johnson , T.V. , Schubert , G. , Asmar , S.W. , Jacobson , R.A. , Johnston , D. , Lau , E.L. , Lewis , G. , Moore , W. , Taylor , A.H. , Thomas , P.C. , and Weinwurm , G. ( 2005 ). Amalthea's density is less than that of water . Science 308 ( 5726 ): 1291 – 1293 . doi: 10.1126/science.1110422 . CrossrefCASPubMedWeb of Science®Google Scholar Anderson , J.D. , Krisher , T.P. , Borutzki , S.E. , Connally , M.J. , Eshe , P.M. , Hotz , H.B. , Kinslow , S. , Kursinski , E.R. , Light , L.B. , Matousek , S.E. , and Moyd , K.I. ( 1987c ). Radio range measurements of coronal electron densities at 13 and 3.6 centimeter wavelengths during the 1985 solar conjunction of Voyager 2 . The Astrophysical Journal 323 : L141 – 143 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Laing , P.A. , Lau , E.L. , Liu , A.S. , Nieto , M.M. , and Turyshev , S.G. ( 2002 ). Study of the anomalous acceleration of Pioneer 10 and 11 . Physical Review D 65 ( 8 ): 082004 . CrossrefCASWeb of Science®Google Scholar Anderson , J.D. , Lau , E. , Asmar , S.W. , Bird , M.K. , Clark , B.C. , Giampieri , G. , Gilliand , K. , and Pätzold , M. ( 2004a ). Stardust dynamic science at comet 81P/Wild 2 . Journal of Geophysical Research: Planets 109 : E12 . Google Scholar Anderson , J.D. , Lau , E.L. , Sjogren , W.L. , Schubert , G. , and Moore , W.B. ( 1996 ). Gravitational constraints on the internal structure of Ganymede . Nature 384 ( 6609 ): 541 – 543 . CrossrefCASWeb of Science®Google Scholar Anderson , J.D. and Mashoon , B. ( 1985 ). Pioneer 10 search for gravitational waves – limits on a possible isotropic cosmic background in the microhertz region . Astrophysical Journal 290 : 445 – 448 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Null , G.W. , and Wong , S.K. ( 1974 ). Gravity results from Pioneer 10 Doppler data . Journal of Geophysical Research 79 ( 25 ): 3661 – 3664 . Wiley Online LibraryWeb of Science®Google Scholar Anderson , J.D. and Schubert , G. ( 2007 ). Saturn's satellite Rhea is a homogeneous mix of rock and ice . Geophysical Research Letters 34 ( 2 ). Wiley Online LibraryWeb of Science®Google Scholar Anderson , J.D. and Schubert , G. ( 2010 ). Rhea's gravitational field and interior structure inferred from archival data files of the 2005 Cassini flyby . Physics of the Earth and Planetary Interiors 178 ( 3 ): 176 – 182 . CrossrefWeb of Science®Google Scholar Anderson , J.D. , Schubert , G. , Asmar , S.W. , Jurgens , R.F. , Lau , E.L. , Moore , W.B. , Slade , M.A. , and Standish , E.M. ( 2001d ). Mercury's global topography from radar ranging data . In: Workshop on Mercury: Space Environment, Surface, and Interior (ed. Mark Robinbson, G. Jeffrey Taylor) , Chicago, IL : The Field Museum . (October 2001). Google Scholar Anderson , J.D. , Schubert , G. , Jacobson , R.A. , Lau , E.L. , Moore , W.B. , and Palguta , J.L. ( 2004b ). Discovery of mass anomalies on Ganymede . Science 305 ( 5686 ): 989 – 991 . CrossrefCASPubMedWeb of Science®Google Scholar Anderson , J.D. , Schubert , G. , Jacobson , R.A. , Lau , E.L. , Moore , W.B. , and Sjogren , W.L. ( 1998 ). Europa's differentiated internal structure: inferences from four Galileo encounters . Science 281 ( 5385 ): 2019 – 2022 . CrossrefCASPubMedWeb of Science®Google Scholar Anderson , J.D. , Turyshev , S.G. , Asmar , S.W. , Bird , M.K. , Konopliv , A.S. , Krisher , T.P. , Lau , E.L. , Schubert , G. , and Sjogren , W.L. ( 1997 ). Radio science investigations on a Mercury orbiter mission . Planetary and Space Science 45 ( 1 ): 21 – 29 . CrossrefWeb of Science®Google Scholar Anderson , J.D. and Warner , M.R. ( 1966 ). J. Kovalevsky Determination of the masses of the Moon and Venus, and the astronomical unit from the radio tracking of Mariner II . In: Trajectories of Artificial Celestial Bodies as Determined from Observations/Trajectoires Des Corps Celestes Artificiels Déterminées D'après Les Observations (ed. J. Kovalevsky), 216 – 246 . Berlin : Springer . CrossrefGoogle Scholar Anderson , J.D. , Campbell , J.K. , Ekelund , J.E. , Ellis , J. and Jordan , J.F. ( 2008 ). Anomalous orbital-energy changes observed during spacecraft flybys of Earth . Physical Review Letters 100 ( 9 ): 091102 . CrossrefPubMedWeb of Science®Google Scholar Andreev , V.E. , Efimov , A.I. , Samoznaev , L.N. , Chashei , I.V. , and Bird , M.K. ( 1997 ). Characteristics of coronal Alfvén waves deduced from Helios Faraday rotation measurements . Solar Physics 176 ( 2 ): 387 – 402 . CrossrefWeb of Science®Google Scholar Andreev , V.E. and Gavrik , A.L. ( 1993 ). Radio transmission measurements of the plasma shell of comet Halley . Astronomy Letters 19 : 437 – 440 . Web of Science®Google Scholar Andrews-Hanna , J.C. , Asmar , S.W. , Head III , J.W. , Wieczorek , M. , Kiefer , W.S. , Taylor , G.J. , Konopliv , A.S. , Lemoine , F.G. , Mazarico , E.M. , McGovern , P.J. , Melosh , H.J. , Neumann , G.A. , Phillips , R.J. , Smith , D.E. , Solomon , S.C. , Williams , J.G. , and Zuber , M.T. ( 2013 ). Ancient igneous intrusions and the early expansion of the M" @default.
• W4224215486 created "2022-04-26" @default.
• W4224215486 date "2022-03-26" @default.
• W4224215486 modified "2023-10-16" @default.
• W4224215486 title "References" @default.
• W4224215486 cites W10761317 @default.
• W4224215486 cites W1495535916 @default.
• W4224215486 cites W1500041086 @default.
• W4224215486 cites W1514437651 @default.
• W4224215486 cites W1532228020 @default.
• W4224215486 cites W1550532157 @default.
• W4224215486 cites W156442276 @default.
• W4224215486 cites W1570009896 @default.
• W4224215486 cites W1571636493 @default.
• W4224215486 cites W1601205716 @default.
• W4224215486 cites W1602876949 @default.
• W4224215486 cites W1617391310 @default.
• W4224215486 cites W1620995071 @default.
• W4224215486 cites W1653723834 @default.
• W4224215486 cites W1654291065 @default.
• W4224215486 cites W1665500180 @default.
• W4224215486 cites W1679819849 @default.
• W4224215486 cites W169818938 @default.
• W4224215486 cites W1731032083 @default.
• W4224215486 cites W1749947268 @default.
• W4224215486 cites W1787046893 @default.
• W4224215486 cites W1813144344 @default.
• W4224215486 cites W1825191605 @default.
• W4224215486 cites W1843849655 @default.
• W4224215486 cites W1864520882 @default.
• W4224215486 cites W1900783992 @default.
• W4224215486 cites W1959961340 @default.
• W4224215486 cites W1963009443 @default.
• W4224215486 cites W1963655311 @default.
• W4224215486 cites W1963722072 @default.
• W4224215486 cites W1963898447 @default.
• W4224215486 cites W1965050829 @default.
• W4224215486 cites W1965536519 @default.
• W4224215486 cites W1966183161 @default.
• W4224215486 cites W1966329758 @default.
• W4224215486 cites W1966711776 @default.
• W4224215486 cites W1967144177 @default.
• W4224215486 cites W1968794517 @default.
• W4224215486 cites W1969539124 @default.
• W4224215486 cites W1970236033 @default.
• W4224215486 cites W1970373549 @default.
• W4224215486 cites W1974143480 @default.
• W4224215486 cites W1974704365 @default.
• W4224215486 cites W1974816849 @default.
• W4224215486 cites W1974941523 @default.
• W4224215486 cites W1974991265 @default.
• W4224215486 cites W1975082943 @default.
• W4224215486 cites W1975753496 @default.
• W4224215486 cites W1976799607 @default.
• W4224215486 cites W1976925252 @default.
• W4224215486 cites W1977045967 @default.
• W4224215486 cites W1977884433 @default.
• W4224215486 cites W1978512827 @default.
• W4224215486 cites W1978690472 @default.
• W4224215486 cites W1978802573 @default.
• W4224215486 cites W1978947013 @default.
• W4224215486 cites W1979061492 @default.
• W4224215486 cites W1979219735 @default.
• W4224215486 cites W1980271221 @default.
• W4224215486 cites W1980620962 @default.
• W4224215486 cites W1981091796 @default.
• W4224215486 cites W1983012380 @default.
• W4224215486 cites W1983246890 @default.
• W4224215486 cites W1983918128 @default.
• W4224215486 cites W1984016459 @default.
• W4224215486 cites W1984426445 @default.
• W4224215486 cites W1984608767 @default.
• W4224215486 cites W1984801545 @default.
• W4224215486 cites W1985218703 @default.
• W4224215486 cites W1985471241 @default.
• W4224215486 cites W1985813871 @default.
• W4224215486 cites W1986061846 @default.
• W4224215486 cites W1987326676 @default.
• W4224215486 cites W1987811467 @default.
• W4224215486 cites W1988579372 @default.
• W4224215486 cites W1988628049 @default.
• W4224215486 cites W1988634113 @default.
• W4224215486 cites W1989038475 @default.
• W4224215486 cites W1989471415 @default.
• W4224215486 cites W1989690676 @default.
• W4224215486 cites W1990282419 @default.
• W4224215486 cites W1990777750 @default.
• W4224215486 cites W1991187198 @default.
• W4224215486 cites W1991276312 @default.
• W4224215486 cites W1991686876 @default.
• W4224215486 cites W1991801386 @default.
• W4224215486 cites W1991801950 @default.
• W4224215486 cites W1991987378 @default.
• W4224215486 cites W1992912239 @default.
• W4224215486 cites W1993650262 @default.
• W4224215486 cites W1995715587 @default.
• W4224215486 cites W1996532980 @default.
• W4224215486 cites W1996651173 @default.

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