標(biāo)題: Titlebook: Chaos in Gravitational N-Body Systems; Proceedings of a Wor J. C. Muzzio,S. Ferraz-Mello,J. Henrard Conference proceedings 1996 Kluwer Acad [打印本頁(yè)] 作者: 根深蒂固 時(shí)間: 2025-3-21 18:05
書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems影響因子(影響力)
書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
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書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems讀者反饋
書(shū)目名稱(chēng)Chaos in Gravitational N-Body Systems讀者反饋學(xué)科排名
作者: 忘恩負(fù)義的人 時(shí)間: 2025-3-21 21:06
grability (the famous Argentine beef was, certainly, also an attraction!). All the papers of the present volume were refereed. Most were accepted after some revision, while some needed no change at all (compli- ments to their authors!) and, sadly, a few could not be included. About half a dozen authors did no978-94-010-6623-5978-94-009-0307-4作者: 出血 時(shí)間: 2025-3-22 02:56
A Note Concerning the 2:1 and the 3:2 Resonances in the Asteroid Belt, secular resonances. This path crosses a bridge, at moderate inclination and large amplitude of libration, between the two chaotic domains associated with these resonances..The 3:2 resonance being similar in many respects to the 2:1 resonance, one may wonder whether it contains also such a path. Ind作者: 誘騙 時(shí)間: 2025-3-22 04:53
Geometrodynamics, Chaos and Statistical Behaviour of N-Body Systems,are unjustified. Nevertheless, we point out that the geometrical transcription of hamiltonian systems, if carefully employed, . deep informations about the degree of stochasticity in the dynamics, and very interesting insights on its sources. To overcome some of the limitations of the approach, for 作者: 高調(diào) 時(shí)間: 2025-3-22 12:45
Geometrodynamics on Finsler Spaces,cribed by conservative potentials and 2) Bianchi IX Cosmological Model (.). This latter example is particularly enlightening, as the introduction of Finsler Geometry overcomes the critical problems which raised some criticisms against the use of the Jacobi (Riemannian) metric to study the chaotic pr作者: 咽下 時(shí)間: 2025-3-22 15:26
Port Cities and Global Legacies secular resonances. This path crosses a bridge, at moderate inclination and large amplitude of libration, between the two chaotic domains associated with these resonances..The 3:2 resonance being similar in many respects to the 2:1 resonance, one may wonder whether it contains also such a path. Ind作者: 咽下 時(shí)間: 2025-3-22 20:24 作者: Focus-Words 時(shí)間: 2025-3-22 21:42
Port Cities and Global Legaciescribed by conservative potentials and 2) Bianchi IX Cosmological Model (.). This latter example is particularly enlightening, as the introduction of Finsler Geometry overcomes the critical problems which raised some criticisms against the use of the Jacobi (Riemannian) metric to study the chaotic pr作者: BLANK 時(shí)間: 2025-3-23 04:06
Spectra of Stretching Numbers and Helicity Angles in Dynamical Systems,tions from a given orbit at times . and . + 1. Similarly we define a ”helicity angle” as the angle between the deviation ξ.and a fixed direction. The distributions of the stretching numbers and helicity angles (spectra) are invariant with respect to initial conditions in a connected chaotic domain. 作者: Ambulatory 時(shí)間: 2025-3-23 05:53
On the Measure of the Structure Around the Last KAM Torus Before and After its Break-Up,he standard map for the analysis of the hierarchical structure existing around invariant KAM tori applying two complementary methods: the Laskar’s frequency map analysis and the sup-map analysis. We recover and extend the theoretical prediction recently given by Morbidelli and Giorgilli about the ex作者: Ibd810 時(shí)間: 2025-3-23 10:56 作者: 壯麗的去 時(shí)間: 2025-3-23 15:28 作者: 高腳酒杯 時(shí)間: 2025-3-23 21:33
Sinking, Tidally Stripped, Galactic Satellites,onally bound, and one of them is much larger than the other, the latter can be regarded as a satellite of the former. The study of their dynamics is somewhat simplified in this case, which presents well observed examples in nature (e.g., globular clusters). Galactic satellites suffer orbital decay d作者: misshapen 時(shí)間: 2025-3-24 00:09
On the Satellite Capture Problem,ed Three-Body Problem. We show that a second integral of motion furnishes an accurate description for the stability limit of retrograde satellites..The distribution of heliocentric orbital elements is studied, and possible candidates to be temporary Jovian satellites are investigated..Previous resul作者: enhance 時(shí)間: 2025-3-24 03:22 作者: judicial 時(shí)間: 2025-3-24 08:48 作者: chastise 時(shí)間: 2025-3-24 12:27
Large Scale Chaos and Marginal Stability in the Solar System,s from the outer region of the solar system. All the inner planets probably experienced large scale chaotic behavior for their obliquities during their history. The Earth obliquity is presently stable only because of the presence of the Moon, and the tilt of Mars undergoes large chaotic variations f作者: 仔細(xì)閱讀 時(shí)間: 2025-3-24 18:25
Chaos in the Solar System,time for an orbit to make a close encounter with a perturbing planet, T., is a function of the Lyapunov time, ... The relation is log(....) = . + . log(....) where .. is a fiducial period which we have taken as the period of the principal perturber or the period of the asteroid. There are exceptions作者: 射手座 時(shí)間: 2025-3-24 21:49
Geometrodynamics, Chaos and Statistical Behaviour of N-Body Systems,the instability is driven by the fluctuations of some geometrical invariants, rather than by their average values; .) the most commonly used invariant has in general nothing to do with dynamic instability of realistic . systems; .) in order to evaluate correctly the relevant quantities entering thes作者: Chemotherapy 時(shí)間: 2025-3-25 01:47
Geometrodynamics on Finsler Spaces,locities (possibly, on time), using a geometrical description. The manifold in which the dynamical systems live is a Finslerian space in which the conformai factor is a positively homogeneous function of first degree in the velocities (the homogeneous Lagrangian of the system). This method is a gene作者: 集合 時(shí)間: 2025-3-25 05:26
Stability of Motion of ,-Body Systems,is leads us to revisit some of the old results concerning geodesic stability on Lagrangian manifolds. These cannot be applied directly but may be useful when properly reinterpreted. A method for doing that is described along with some tests of its validity and possible future applications.作者: 大猩猩 時(shí)間: 2025-3-25 08:29 作者: Favorable 時(shí)間: 2025-3-25 13:46 作者: 最有利 時(shí)間: 2025-3-25 19:28
On the Possibility of 2D Dynamical Chaos in Astrophysical Disks,uations. Derived necessary and sufficient conditions of 2-D description are fulfilled rather seldom in astrophysical disks. Under this conditions we derived the 2-D equation with scalar and vector nonlinearities describing the dynamics of gaseous disk rotating in solid-body manner. From our study it作者: 思考才皺眉 時(shí)間: 2025-3-25 22:00
The Observed Turbulent Spectrum of Cloudy Population of the Milky Way as an Evidence of a Weak Ross For small-scale perturbations the equation can be reduced to the well known nonlinear equation for Rossby waves — Charney-Obukhov equation. The spectrum of weak turbulence obtained from this equation leads to the observed by Mayers and Solomon et al. relations between the fundamental parameters of 作者: Factual 時(shí)間: 2025-3-26 01:27 作者: 不知疲倦 時(shí)間: 2025-3-26 07:33
Spectra of Stretching Numbers and Helicity Angles in Dynamical Systems,We study such spectra in conservative and dissipative mappings of 2 degrees of freedom and in conservative mappings of 3-degrees of freedom. In 2-D conservative systems we found that the lines of constant stretching number have a fractal form.作者: canvass 時(shí)間: 2025-3-26 12:17 作者: 太空 時(shí)間: 2025-3-26 16:10 作者: obeisance 時(shí)間: 2025-3-26 18:34
Conference proceedings 1996nd Geophysics of La Plata National University, best known as La Plata Observatory, was the host institution. The Observatory (cover photo) was founded in 1883, and it has nowadays about 120 faculty members and 70 non-faculty members devoted to teaching and research in different areas of astronomy an作者: 原諒 時(shí)間: 2025-3-26 22:05
stronomy and Geophysics of La Plata National University, best known as La Plata Observatory, was the host institution. The Observatory (cover photo) was founded in 1883, and it has nowadays about 120 faculty members and 70 non-faculty members devoted to teaching and research in different areas of as作者: misanthrope 時(shí)間: 2025-3-27 03:45 作者: arousal 時(shí)間: 2025-3-27 05:35 作者: 甜得發(fā)膩 時(shí)間: 2025-3-27 10:29
https://doi.org/10.1057/9781137283146e distribution of heliocentric orbital elements is studied, and possible candidates to be temporary Jovian satellites are investigated..Previous results, limited to orbits satisfying the Mirror Theorem, are extended in order to give a complete set of capture conditions in phase-space.作者: ascetic 時(shí)間: 2025-3-27 13:44
Brad Beaven,Karl Bell,Robert Jamesas the existence of periodic orbits are observed..We also considered ellipsoids embedded in rigid, homogeneous, spherical halos, obtaining evidence of the stabilizing effect of halos even in the case of finite-amplitude oscillations.作者: coagulate 時(shí)間: 2025-3-27 18:32 作者: 個(gè)人長(zhǎng)篇演說(shuō) 時(shí)間: 2025-3-27 23:46 作者: 人類(lèi) 時(shí)間: 2025-3-28 04:01
On the Satellite Capture Problem,e distribution of heliocentric orbital elements is studied, and possible candidates to be temporary Jovian satellites are investigated..Previous results, limited to orbits satisfying the Mirror Theorem, are extended in order to give a complete set of capture conditions in phase-space.作者: diabetes 時(shí)間: 2025-3-28 08:15
Numerical Exploration of the Dynamics of Self-Adjoint S-Type Riemann Ellipsoids,as the existence of periodic orbits are observed..We also considered ellipsoids embedded in rigid, homogeneous, spherical halos, obtaining evidence of the stabilizing effect of halos even in the case of finite-amplitude oscillations.作者: GLOOM 時(shí)間: 2025-3-28 12:34 作者: 呼吸 時(shí)間: 2025-3-28 15:00
Die Architektur der erweiterten Situationistence of a neighborhood almost completely full of slave tori around a chief torus. We then make tests about the diffusion in order to measure the barrier to diffusion which still remains after the break-up of the last KAM torus.作者: RECUR 時(shí)間: 2025-3-28 19:33 作者: Optic-Disk 時(shí)間: 2025-3-29 01:02 作者: Tortuous 時(shí)間: 2025-3-29 04:36 作者: Seizure 時(shí)間: 2025-3-29 09:57 作者: staging 時(shí)間: 2025-3-29 12:22 作者: 集中營(yíng) 時(shí)間: 2025-3-29 15:52
Chaos in the Solar System,ave a positive Lyapunov exponent and still be blocked from having a close approach to Jupiter by a “zero velocity curve”. Of more serious concern is whether the relation holds for purely secular resonances, and if it does, how to choose ... This is the case of interest for the planets in the solar system.作者: Mundane 時(shí)間: 2025-3-29 19:42 作者: In-Situ 時(shí)間: 2025-3-30 03:47 作者: VOK 時(shí)間: 2025-3-30 04:39 作者: 減弱不好 時(shí)間: 2025-3-30 09:39
http://image.papertrans.cn/c/image/223887.jpg作者: Malaise 時(shí)間: 2025-3-30 13:09
Die Architektur der erweiterten Situationtions from a given orbit at times . and . + 1. Similarly we define a ”helicity angle” as the angle between the deviation ξ.and a fixed direction. The distributions of the stretching numbers and helicity angles (spectra) are invariant with respect to initial conditions in a connected chaotic domain. 作者: 組裝 時(shí)間: 2025-3-30 16:58 作者: fatuity 時(shí)間: 2025-3-30 21:32 作者: LATE 時(shí)間: 2025-3-31 02:59 作者: Erythropoietin 時(shí)間: 2025-3-31 05:22
Die Architektur der erweiterten Situationonally bound, and one of them is much larger than the other, the latter can be regarded as a satellite of the former. The study of their dynamics is somewhat simplified in this case, which presents well observed examples in nature (e.g., globular clusters). Galactic satellites suffer orbital decay d作者: 無(wú)情 時(shí)間: 2025-3-31 13:04
https://doi.org/10.1057/9781137283146ed Three-Body Problem. We show that a second integral of motion furnishes an accurate description for the stability limit of retrograde satellites..The distribution of heliocentric orbital elements is studied, and possible candidates to be temporary Jovian satellites are investigated..Previous resul作者: 鼓掌 時(shí)間: 2025-3-31 14:16
Port Cities and Global Legaciessystems are not integrable, the motion modes are not separated and one orbit may transit from one mode to another. In some cases, as in the 3/1 resonance, these transitions may lead, in a relatively short time scale, to eccentricities so high that the asteroid may approach the Sun and be destroyed. 作者: CLASP 時(shí)間: 2025-3-31 21:11
Port Cities and Global Legaciesalytical or numerical, point out that the two resonances have a very similar dynamical behavior. In spite of that, the 3:2 resonance, a little outside the main belt, hosts a family of asteroids, called the Hildas, while the 2:1, inside the main belt, is associated to a gap (the Hecuba gap) in the di作者: 草率女 時(shí)間: 2025-3-31 21:45 作者: Outshine 時(shí)間: 2025-4-1 03:31 作者: Curmudgeon 時(shí)間: 2025-4-1 08:52
Port Cities and Global Legaciesthe instability is driven by the fluctuations of some geometrical invariants, rather than by their average values; .) the most commonly used invariant has in general nothing to do with dynamic instability of realistic . systems; .) in order to evaluate correctly the relevant quantities entering thes作者: 有權(quán)威 時(shí)間: 2025-4-1 12:42
Port Cities and Global Legacieslocities (possibly, on time), using a geometrical description. The manifold in which the dynamical systems live is a Finslerian space in which the conformai factor is a positively homogeneous function of first degree in the velocities (the homogeneous Lagrangian of the system). This method is a gene作者: 最低點(diǎn) 時(shí)間: 2025-4-1 14:47 作者: 壓碎 時(shí)間: 2025-4-1 18:29 作者: 不能根除 時(shí)間: 2025-4-2 02:37
Brad Beaven,Karl Bell,Robert JamesSection, which reveal a rich and complex dynamical behaviour..Both the occurrence of chaos for certain values of the parameters of the system as well as the existence of periodic orbits are observed..We also considered ellipsoids embedded in rigid, homogeneous, spherical halos, obtaining evidence of作者: heart-murmur 時(shí)間: 2025-4-2 03:56 作者: 蛛絲 時(shí)間: 2025-4-2 08:08
Criteria for transportable algol libraries, For small-scale perturbations the equation can be reduced to the well known nonlinear equation for Rossby waves — Charney-Obukhov equation. The spectrum of weak turbulence obtained from this equation leads to the observed by Mayers and Solomon et al. relations between the fundamental parameters of
