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Archive for History of Exact Sciences, 2002
The author shows convincingly that J. B. J. Delambre (1817) was right in attributing to Hipparchus the use of celestial spherical coordinates and that \textit{O. Neugebauer}, on pp. 277-280 of [`A history of ancient mathematical astronomy. Vol. I. New York: Springer (1975; Zbl 0323.01002)] was wrong in denying this fact.
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The author shows convincingly that J. B. J. Delambre (1817) was right in attributing to Hipparchus the use of celestial spherical coordinates and that \textit{O. Neugebauer}, on pp. 277-280 of [`A history of ancient mathematical astronomy. Vol. I. New York: Springer (1975; Zbl 0323.01002)] was wrong in denying this fact.
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1996
Abstract In this book, all coordinate systems used are orthogonal unless stated otherwise. The coordinate variables and the corresponding unit vectors in the general orthogonal system will be denoted by (v1, v2, v3) and (u1, u2, u3). The coefficients hi 's are called the metric coefficients of that system.
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Abstract In this book, all coordinate systems used are orthogonal unless stated otherwise. The coordinate variables and the corresponding unit vectors in the general orthogonal system will be denoted by (v1, v2, v3) and (u1, u2, u3). The coefficients hi 's are called the metric coefficients of that system.
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