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Titlebook: Nonlinear Physics of Complex Systems; Current Status and F Jürgen Parisi,Stefan C. Müller,Walter Zimmermann Conference proceedings 1996 Spr

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樓主: Stimulant
41#
發(fā)表于 2025-3-28 15:36:42 | 只看該作者
Bounds for properties of complex systems,ns describing turbulent flows in arbitrary geometrical configurations. Based on energy type balances, bounds on transport quantities can be derived rigorously. In many cases of turbulent fluid flow the extremalizing vector fields show surprising similarities with the observed turbulent velocity fields.
42#
發(fā)表于 2025-3-28 18:48:30 | 只看該作者
43#
發(fā)表于 2025-3-29 00:11:49 | 只看該作者
44#
發(fā)表于 2025-3-29 03:10:50 | 只看該作者
45#
發(fā)表于 2025-3-29 07:50:08 | 只看該作者
Conditional probability distributions of a turbulent cascade,e turbulent cascade is described by a drift and diffusion coefficient and the joint probability distributions obey a Fokker-Planck equation. We calculate the drift and diffusion coefficients and discuss their relationship to universal behaviour in the scaling region of the turbulent cascade.
46#
發(fā)表于 2025-3-29 14:55:28 | 只看該作者
47#
發(fā)表于 2025-3-29 16:48:05 | 只看該作者
48#
發(fā)表于 2025-3-29 20:36:03 | 只看該作者
Time series analysis of scalar time-delay systems, function . can be recovered. There are no restrictions to the dimensionality of the chaotic attractor. The method turns out to be insensitive to noise. We successfully apply the method to various time series taken from a computer experiment and two different electronic oscillators.
49#
發(fā)表于 2025-3-30 01:30:19 | 只看該作者
Conference proceedings 1996overview of recent developments and perspectives. Particular attention is given to the so-far unsolved problem of how to capture the mutual interplay between the microscopic and macroscopic dynamics that extend over various length and time scales. The book addresses researchers as well as graduate students.
50#
發(fā)表于 2025-3-30 06:06:37 | 只看該作者
Why air bubbles in water glow so easily,a of Putterman’s UCLA group. We can quantitatively account for heretofore unexplained results. In particular, we understand why the argon percentage in air is so essential for the observation of stable SL.
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