Titlebook: Dynamical Chaos in Planetary Systems; Ivan I. Shevchenko Book 2020 Springer Nature Switzerland AG 2020 planetary systems.dynamical chaos.p

JAZZ

書目名稱Dynamical Chaos in Planetary Systems影響因子(影響力)




書目名稱Dynamical Chaos in Planetary Systems影響因子(影響力)學(xué)科排名




書目名稱Dynamical Chaos in Planetary Systems網(wǎng)絡(luò)公開度




書目名稱Dynamical Chaos in Planetary Systems網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Dynamical Chaos in Planetary Systems被引頻次




書目名稱Dynamical Chaos in Planetary Systems被引頻次學(xué)科排名




書目名稱Dynamical Chaos in Planetary Systems年度引用




書目名稱Dynamical Chaos in Planetary Systems年度引用學(xué)科排名




書目名稱Dynamical Chaos in Planetary Systems讀者反饋




書目名稱Dynamical Chaos in Planetary Systems讀者反饋學(xué)科排名

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0067-0057 ynamics in a unified framework.Provides a description of mos.This is the first monograph dedicated entirely to problems of stability and chaotic behaviour in planetary systems and its subsystems. The author explores the three rapidly developing interplaying fields of resonant and chaotic dynamics of

喧鬧

光明正大

Discrete

不幸的人

Contested Waters: Dividing or Sharing? are being developed and improved. Current and perspective studies of chaotic behaviour in exoplanetary systems comprise investigations of various clearing effects. Developments of analytical criteria of stability of planetary systems are warranted.

不幸的人

Book 2020lores the three rapidly developing interplaying fields of resonant and chaotic dynamics of Hamiltonian systems, the dynamics of Solar system bodies, and the dynamics of exoplanetary systems. The necessary concepts, methods and tools used to study dynamical chaos (such as symplectic maps, Lyapunov ex

Confirm

Chaotic Behaviourymplectic maps in general, the standard and separatrix maps, generalized separatrix maps, geometry of chaotic layers. These tools are necessary for estimating the diffusion and clearing rates, Lyapunov timescales, and extents of chaotic zones in various dynamical applications, exposed further on in the book.

BOLT

Keshan-disease

Multiplanet Systems of Single Starsharacterized in various dynamical models, in particular, if the perturber is in outer orbit in the system, and if it is in an inner orbit. We discuss actual resonant and formally chaotic exoplanet systems.