Titlebook: Chaos in Astrophysics; J. R. Buchler,J. M. Perdang,E. A. Spiegel Book 1985 D. Reidel Publishing Company, Dordrecht, Holland 1985 astrophys

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V. Gupta,M. D. Lechner,R. Guptaovern the temporal, regular or chaotic modulations of the amplitudes of the excited modes. These amplitude equations have been calculated and solved for realistic population I (Classical) Cepheid models, which have an internal resonance of the type Ω. ≃ 2 Ω. and exhibit a secondary bump on their lig

聋子

Grievance

鄙视读作

R. Gupta,V. Gupta,M. D. Lechner,R. Gupta with the second law of thermodynamics, (ii) the relation between the information flow rate ( = Kolmogorov entropy), Lyapunov exponents, and dimensions of the attractor, (iii) the discussion of generalized dimensions and entropies related to the flow of Renyi informations, (iv) the measurements of t

freight

R. Gupta,V. Gupta,M. D. Lechner,R. Gupta presence of a mean magnetic field, limited by a of large magnetic Reynolds number R. An asymptotic procedure relying on a presumed geometry of flux ropes and sheets is used. Our results suggest that alpha has a finite nonzero limit as R → ∞. We express this limit in terms of the geometry of certain

CAB

originality

R. Gupta,V. Gupta,M. D. Lechner,R. Guptan applied to obtain a Hamiltonian formalism. The numerical results presented here show that the nonradial modes can cause a much more irregular motion than the radial modes. First, there are many near-resonant nonradial frequencies, and second, there is a nonlinear velocity-dependent term in the Ham

jumble

小溪

https://doi.org/10.1007/978-3-642-41556-2rate limit cycles are identified, one of which is responsible for shell flashes in red giants and the second provides the underlying mechanism for X-ray burst sources..When the impact of the burst luminosity on the accretion rate is introduced, the system is shown to exhibit a complex temporal behav

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