標(biāo)題: Titlebook: Analytical Techniques of Celestial Mechanics; Victor A. Brumberg Book 1995 Springer-Verlag Berlin Heidelberg 1995 Computeralgebra.Himmelsm [打印本頁] 作者: DUBIT 時(shí)間: 2025-3-21 16:34
書目名稱Analytical Techniques of Celestial Mechanics影響因子(影響力)
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書目名稱Analytical Techniques of Celestial Mechanics被引頻次
書目名稱Analytical Techniques of Celestial Mechanics被引頻次學(xué)科排名
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書目名稱Analytical Techniques of Celestial Mechanics讀者反饋
書目名稱Analytical Techniques of Celestial Mechanics讀者反饋學(xué)科排名
作者: COST 時(shí)間: 2025-3-21 22:29
Implications for Teaching and for Research,the motion of celestial bodies or at least to find corrections in a literal form to some approximate basic solution corresponding to specific initial numerical values and numerical values of the parameters. A series of power and trigonometric terms of the form ., with . = (.,…,.) and . = (.,…, .) be作者: 暗指 時(shí)間: 2025-3-22 02:06 作者: Constant 時(shí)間: 2025-3-22 08:06 作者: Handedness 時(shí)間: 2025-3-22 12:33 作者: 音的強(qiáng)弱 時(shí)間: 2025-3-22 14:29
Smart Innovation, Systems and Technologies rather large (of the order of 0.7, for example, for the pair Venus-Earth). Therefore, efficient expansions in powers of this ratio in satellite problems cannot be directly used here. They are given below to characterize the general structure of the expansions.作者: 易碎 時(shí)間: 2025-3-22 17:03 作者: 致詞 時(shí)間: 2025-3-22 23:53
https://doi.org/10.1007/978-981-13-3384-2er we consider methods applied to equations in elements whereas further on we shall deal with methods applied to equations in rectangular coordinates. But the differences between these two groups of methods are not of major significance. Their common features are of greater importance. In essence, a作者: defendant 時(shí)間: 2025-3-23 02:17
https://doi.org/10.1007/978-981-13-3384-2thod is similar to the von Zeipel technique of separation of short- and long- period perturbations in elements. The general solution of the homogeneous equations of variations for the two-body problem is presented here only on the basis of a transformation leading to a differential system with const作者: LATHE 時(shí)間: 2025-3-23 08:30 作者: Mingle 時(shí)間: 2025-3-23 10:28
https://doi.org/10.1007/978-981-13-3384-2he framework of the GPT. This framework is designed for small eccentricities and inclinations. For minor planets with large values of eccentricities and inclinations it is reasonable to use the expansion of the disturbing function of type (6.2.13), which involves Jacobi nomes and actual values of in作者: 膽汁 時(shí)間: 2025-3-23 15:30 作者: 使迷醉 時(shí)間: 2025-3-23 22:00 作者: CERE 時(shí)間: 2025-3-23 22:14
Defence and Disruptive Technologiesent argument or in pure trigonometric form with respect to some linear functions of this argument. We start with the first form. Let . (.),…, .(.) be the functions satisfying the differential polynomial system ., .(.) being power series with constant coefficients ..作者: animated 時(shí)間: 2025-3-24 05:24 作者: MIR 時(shí)間: 2025-3-24 07:04 作者: NAV 時(shí)間: 2025-3-24 13:15
Algorithms to Solve Polynomial Systems,ent argument or in pure trigonometric form with respect to some linear functions of this argument. We start with the first form. Let . (.),…, .(.) be the functions satisfying the differential polynomial system ., .(.) being power series with constant coefficients ..作者: cinder 時(shí)間: 2025-3-24 16:45 作者: Buttress 時(shí)間: 2025-3-24 21:27 作者: Mere僅僅 時(shí)間: 2025-3-25 00:23 作者: Progesterone 時(shí)間: 2025-3-25 05:56 作者: 兒童 時(shí)間: 2025-3-25 10:14 作者: 大吃大喝 時(shí)間: 2025-3-25 15:32 作者: 大方不好 時(shí)間: 2025-3-25 17:25 作者: 四海為家的人 時(shí)間: 2025-3-25 20:17
The General Planetary Theory,red his technique to be only an existence theorem although he actually used Newton- type quadratic iterations underlying the present KAM theory (Section 8.4). Later on the trigonometric representation of GPT was advanced by Dziobek (1888), Poincaré (1905) and Charlier (1902, 1907).作者: GUEER 時(shí)間: 2025-3-26 00:35
Book 1995e essence of any algorithm with its particular program implementation. For these reasons, the analytical techniques of this book are to be regarded as algorithms to be implemented in different ways depending on the hardware and software available. The book was preceded by Analytical Algorithms of Ce作者: nonsensical 時(shí)間: 2025-3-26 07:57 作者: 單調(diào)性 時(shí)間: 2025-3-26 08:50 作者: Expand 時(shí)間: 2025-3-26 12:37 作者: reject 時(shí)間: 2025-3-26 16:50
Disarmament, Arms Control and Arms Racered his technique to be only an existence theorem although he actually used Newton- type quadratic iterations underlying the present KAM theory (Section 8.4). Later on the trigonometric representation of GPT was advanced by Dziobek (1888), Poincaré (1905) and Charlier (1902, 1907).作者: 航海太平洋 時(shí)間: 2025-3-26 23:41 作者: Opponent 時(shí)間: 2025-3-27 04:08 作者: paradigm 時(shí)間: 2025-3-27 05:19
The Keplerian Processor,one confines oneself only to the case of elliptic motion, which is the most important for practical applications. The Keplerian processor may be developed on the basis of a PS processor or some general CAS. It illustrates the application of these software tools to the derivation of the formulae desc作者: BUST 時(shí)間: 2025-3-27 13:02 作者: 逢迎白雪 時(shí)間: 2025-3-27 15:16 作者: Adornment 時(shí)間: 2025-3-27 20:45 作者: 遵循的規(guī)范 時(shí)間: 2025-3-28 01:24 作者: essential-fats 時(shí)間: 2025-3-28 04:11
Separation of Variables in Elements,er we consider methods applied to equations in elements whereas further on we shall deal with methods applied to equations in rectangular coordinates. But the differences between these two groups of methods are not of major significance. Their common features are of greater importance. In essence, a作者: Individual 時(shí)間: 2025-3-28 09:29
Separation of Variables in Rectangular Coordinates,thod is similar to the von Zeipel technique of separation of short- and long- period perturbations in elements. The general solution of the homogeneous equations of variations for the two-body problem is presented here only on the basis of a transformation leading to a differential system with const作者: Foregery 時(shí)間: 2025-3-28 14:22
The General Planetary Theory,nd valid, at least formally, for an indefinite interval of time, has always been considered one of the most important problems of celestial mechanics. Laplace was the first to propose solving the equations of planetary motion in a purely trigonometric form with respect to time. But technical difficu作者: 含水層 時(shí)間: 2025-3-28 17:36 作者: DENT 時(shí)間: 2025-3-28 22:38 作者: 新奇 時(shí)間: 2025-3-28 23:27 作者: BULLY 時(shí)間: 2025-3-29 04:12
AR Cloud-Based Indoor Navigation,nd inclinations (the secular system) and so on. Moreover, the differential equations of celestial mechanics may be reduced in typical cases to polynomial systems by introducing some extra unknown variables. To illustrate this let us consider the problem of the heliocentric motion of . planets.作者: Sinus-Node 時(shí)間: 2025-3-29 11:06
Book 1995 "techniques" is used here as a term intermediate between "methods" and "recipes". One often conceives some method of solution of a problem as a general mathematical tool, while not taking much care with its computa- tional realization. On the other hand, the word "recipes" may nowadays be understoo作者: 脫毛 時(shí)間: 2025-3-29 12:11 作者: CARK 時(shí)間: 2025-3-29 15:38
The Poisson-Series Processor,ing power and trigonometric variables, respectively, is called an (., .) Poisson series. The summation in (1.1.1) is performed over all integer (positive and negative) values of indices . (.,…, .) and . = (.,…, j.). Sometimes it is appropriate to consider the exponential form of the Poisson series, ..作者: 對(duì)手 時(shí)間: 2025-3-29 22:58 作者: Evacuate 時(shí)間: 2025-3-30 01:32
https://doi.org/10.1007/978-981-13-3384-2ticular, in the theory of secular resonances caused by the commensurabilities between the secular motions of perihelia and nodes of major planets and asteroids. Therefore, consideration of the motion of asteroids by the same technique as used in the major-planet theory may bring new insight to this problem.作者: gospel 時(shí)間: 2025-3-30 07:51 作者: perpetual 時(shí)間: 2025-3-30 12:11
