By Dieter Biskamp
Publisher: Cambridge University Press
Print Publication Year: 2003
Online Publication Date:August 2009
Online ISBN:9780511535222
Hardback ISBN:9780521810111
Paperback ISBN:9780521052535
Chapter DOI: http://dx.doi.org/10.1017/CBO9780511535222.004
Subjects: Plasma Physics and Fusion Physics, Astrophysics
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One important aspect of turbulence theory is the need to understand how obviously random motions are generated from a smooth flow. There are essentially three approaches to this problem: the dynamic systems approach; the development of singular solutions of the ideal fluid equations, in particular the question of finite-time singularities; and the excitation of instabilities and their effects. The dynamic systems approach, i.e., the transition to a chaotic temporal behavior in some low-order nonlinear dynamic model such as the Lorentz model of thermal convection, had once been considered a very promising way to describe also the transition to turbulence in a fluid. However, these expectations have largely been frustrated, mainly because the low-order approximations of the fluid equations ignore the most important aspect of turbulence, namely the excitation and interactions of a broad range of different spatial scales. We will therefore not discuss dynamic systems theory in this treatise.
The problem of finite-time singularities has evoked considerable discussion. This is primarily a mathematical problem concerning the nature of the solution of the ideal fluid equations, whose relevance for the generation of turbulence in dissipative systems might be debatable. However, similarly to the theory of absolute equilibrium states of the ideal system considered in Section 5.2, which provides valuable information about the cascade dynamics in dissipative turbulence, the way in which the ideal solution becomes singular gives some indication of the spatial structure of eddies encountered in the dissipative system.
pp. i-vi
pp. vii-x
pp. xi-xii
pp. 1-9
2 - Magnetohydrodynamics : Read PDF
pp. 10-32
3 - Transition to turbulence : Read PDF
pp. 33-64
4 - Macroscopic turbulence theory : Read PDF
pp. 65-85
5 - Spectral properties and phenomenology : Read PDF
pp. 86-112
6 - Two-point-closure theory : Read PDF
pp. 113-130
pp. 131-160
8 - Two-dimensional turbulence : Read PDF
pp. 161-182
9 - Compressible turbulence and turbulent convection : Read PDF
pp. 183-216
10 - Turbulence in the solar wind : Read PDF
pp. 217-232
11 - Turbulence in accretion disks : Read PDF
pp. 233-255
12 - Interstellar turbulence : Read PDF
pp. 256-274
pp. 275-276
pp. 277-292
pp. 293-297