Dimension of the Earth's General Ellipsoid |
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Authors: | Burša Milan Kenyon Steve Kouba Jan Raděj Karel Šíma Zdislav Vatrt Viliam Vojtíšková Marie |
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Institution: | (1) Astronomical Institute, Academy of Sciences of the Czech Republic, Prague, Czech Republic;(2) National Imagery and Mapping Agency, St.Louis, MO 63118–3399, USA;(3) Geodetic Survey Division, Natural Resources Canada, Ottawa, Canada;(4) Topographical Service of the Army of the Czech Republic, Topographical Institute VTOPU, Dobruka, Czech Republic;(5) Topographical Service of the Army of the Czech Republic, Topographical Institute VTOPU, Dobruka, Czech Republic;(6) Special Study Group Global Geodesy Topics: Satellite Altimetry Applications, Czech Republic |
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Abstract: | The problem of specifying the Earth's mean (general)ellipsoid is discussed. This problem has been greatly simplified in the era of satellite altimetry, especially thanks to the adopted geoidal geopotential value, W0 = (62 636 856.0 ± 0.5) m2 s-2.Consequently, the semimajor axis a of the Earth's mean ellipsoid can be easily derived. However, an a priori condition must be posed first. Two such a priori conditions have been examined, namely an ellipsoid with the corresponding geopotential that fits best W0 in the least squares sense and an ellipsoid that has the global geopotential average equal to W0. It has been demonstrated that both a priori conditions yield ellipsoids of the same dimension, with a–values that are practically identical to the value corresponding to the Pizzetti theory of the level ellipsoid: a = (6 378 136.68 ± 0.06) m. |
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Keywords: | Earth's dimensions Earth's ellipsoid fundamental constants |
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