Methods of Celestial Mechanics: Volume II: Application to Planetary System, Geodynamics and Satellite GeodesySpringer Science & Business Media, 21.11.2005 - 448 Seiten G. Beutler's Methods of Celestial Mechanics is a coherent textbook for students as well as an excellent reference for practitioners. The first volume gives a thorough treatment of celestial mechanics and presents all the necessary mathematical details that a professional would need. The reader will appreciate the well-written chapters on numerical solution techniques for ordinary differential equations, as well as that on orbit determination. In the second volume applications to the rotation of earth and moon, to artificial earth satellites and to the planetary system are presented. The author addresses all aspects that are of importance in high-tech applications, such as the detailed gravitational fields of all planets and the earth, the oblateness of the earth, the radiation pressure and the atmospheric drag. The concluding part of this monumental treatise explains and details state-of-the-art professional and thoroughly-tested software for celestial mechanics. |
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... interval. Multistep methods, but also the famous Gaussian methods for numerical quadrature, were recognized as special cases of collocation methods. Numerical integration techniques are the basis of the computer programs ERDROT, SATORB ...
... interval between the two observations should be significantly shorter than the revolution period of the object considered). The most important perturbations (planetary perturbations in the case of minor planets and comets, gravitational ...
... interval between two subsequent passes of the Sun through the Moon's nodal line is called an eclipse year. The W-component is thus negative for 0◦ <u< 180◦ and positive for 180◦ <u< 360◦. This pattern also explains the differences ...
... 2.8, documenting a time interval of two. Fig. 2.7. Semi-major axis a − 380000 km of lunar orbit 1981-1983 Fig. 2.8. Eccentricity of the lunar orbit 1981-1983 Fig. 2.10. 2.2 The Rotation of a Rigid Earth and a Rigid Moon 25.
... interval of two years, the eccentricity of the lunar orbit varies roughly within the limits 0.025 ≤ e ≤ 0.075. The principal period is of the order of one month (according to a spectral analysis of 31.5 days), which is modulated by a ...
Inhalt
3 | |
6 | |
14 | |
Artificial Earth Satellites | 123 |
Evolution of the Planetary System | 211 |
Variational Equations | 272 |
5 | 301 |
The ComputerPrograms NUMINT and LINEAR | 311 |
The ComputerPrograms SATORB and LEOKIN | 323 |
The ComputerProgram ORBDET 355 | 354 |
The ComputerProgram ERDROT | 371 |
The ComputerProgram PLASYS | 387 |
Elements of Spectral Analysis | 394 |
References | 425 |
Abbreviations and Acronyms 433 | 432 |
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Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Eingeschränkte Leseprobe - 2004 |
Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Keine Leseprobe verfügbar - 2004 |