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Titlebook: Relativity in Astrometry, Celestial Mechanics and Geodesy; Michael H. Soffel Book 1989 Springer-Verlag Berlin Heidelberg 1989 Astrometry.C

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書目名稱Relativity in Astrometry, Celestial Mechanics and Geodesy
編輯Michael H. Soffel
視頻videohttp://file.papertrans.cn/827/826269/826269.mp4
叢書名稱Astronomy and Astrophysics Library
圖書封面Titlebook: Relativity in Astrometry, Celestial Mechanics and Geodesy;  Michael H. Soffel Book 1989 Springer-Verlag Berlin Heidelberg 1989 Astrometry.C
描述The book "Relativity in Astrometry, Celestial Mechanics and Geodesy" repre- sents a significant contribution to modern relativistic celestial mechanics and astrometry. In these branches of astronomy the theory of general relativity is used nowadays as an efficient practical framework for constructing accurate dynamical theories of motion of celestial bodies and discussing high-precision observations. The author develops the useful tools for this purpose and intro- duces the reader into the modern state of the art in these domains. More specifically, the distinctive feature of the book is the wide application of the tetrad formalism to astronomical problems. One may not agree with the author‘s opinion that this is the only method so far to be able to treat the rel- ativistic astronomical problems in a consistent and satisfactory manner. (On the contrary, one may foresee in the nearest future other books on relativistic celestial mechanics and astrometry based on different approaches solving the same problems. ) However, we are now at the beginning of practical relativis- tic astronomy and it will demand much effort to reconstruct in a relativistic manner all Newtonian conceptions of
出版日期Book 1989
關(guān)鍵詞Astrometry; Celestial mechanics; Gravity; Relativity; general relativity
版次1
doihttps://doi.org/10.1007/978-3-642-73406-9
isbn_softcover978-3-642-73408-3
isbn_ebook978-3-642-73406-9Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 1989
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Geodesy,avimetric measurements in the frame of his multi-parameter formalism (parameters γ, β, ξ, α., α., α., ζ., ζ., ζ., and ζ. (2.2.18)) with an accuracy of 10. .. In this theory the post-Newtonian . of gravimeter readings, according to Will, are essentially given by: . where α denotes the usual gravimetr
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Geodesy,ic factor and . (the locally measured gravitational constant) is given by: . where . and . denote the spherical moment of inertia, mass and radius of the Earth, ê is a (Euclidean) unit vector, pointing from the test mass of the gravimeter to the center of the Earth (in usual PN coordinates) and ..
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Book 1989ure other books on relativistic celestial mechanics and astrometry based on different approaches solving the same problems. ) However, we are now at the beginning of practical relativis- tic astronomy and it will demand much effort to reconstruct in a relativistic manner all Newtonian conceptions of
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0941-7834 e now at the beginning of practical relativis- tic astronomy and it will demand much effort to reconstruct in a relativistic manner all Newtonian conceptions of978-3-642-73408-3978-3-642-73406-9Series ISSN 0941-7834 Series E-ISSN 2196-9698
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