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Topological ideas are relevant to fluid dynamics (including magnetohydrodynamics) at the kinematic level, since any fluid flow involves continuous deformation of any transported scalar or vector field. Problems of stirring and mixing are particularly susceptible to topological techniques. Thus, for example, the Thurston–Nielsen classification has been fruitfully applied to the problem of stirring in two-dimensions by any number of stirrers following a time-periodic 'stirring protocol' (Boyland, Aref & Stremler 2000). Other studies are concerned with flows having chaotic particle paths, and associated exponential rates of mixing (Ottino 1989). At the dynamic level, the fact that vortex lines are transported by any flow governed by the classical Euler equations implies conservation of any vortical structure within the flow. Such structures are characterised at least in part by the helicity of certain sub-regions of the flow field, a topological invariant of the equations. Helicity plays a central role in dynamo theory, the theory of spontaneous generation of magnetic fields in stars and planets (Moffatt 1978, Parker 1979, Krause & Rädler 1980). It is known that, with few exceptions, any statistically homogeneous turbulent flow having nonzero mean helicity in a sufficiently large expanse of conducting fluid will generate a large-scale magnetic field through dynamo action. Such fields themselves exhibit magnetic helicity, reflecting their own topologically nontrivial structure. Much interest attaches to the determination of states of minimum energy, subject to prescribed topology. Many problems of fluid dynamics and magnetohydrodynamics fall within this category. Recent developments in topological fluid dynamics include also applications to magnetic braids in the solar corona, DNA knotting by topoisomerases, polymer entanglement in chemical physics and chaotic behavior in dynamical systems. A mathematical introduction to this subject is given by Arnold & Khesin (1998) and recent survey articles and contributions may be found in Ricca (2009), and Moffatt, Bajer & Kimura (2013). ==References== *Arnold, V. I. & Khesin, B. A. (1998) ''(Topological Methods in Hydrodynamics )''. Applied Mathematical Sciences 125, Springer-Verlag. ISBN 9780387949475 *Boyland, P.L., Aref, H. & Stremler, M.A. (2000) (Topological fluid mechanics of stirring ). ''J.Fluid Mech.'' 403, pp. 277-304. *Krause, F. & Rädler, K.-H. (1980) ''Mean-field Magnetohydrodynamic and Dynamo Theory''. Pergamon Press, Oxford. ISBN 9780080250410 * Moffatt, H.K. (1978) (''Magnetic Field Generation in Electrically Conducting Fluids'' ). Cambridge Univ. Press. ISBN 9780521216401 * Moffatt, H.K., Bajer, K., & Kimura, Y. (Eds.) (2013) (''Topological Fluid Dynamics, Theory and Applications'' ). Kluwer. *Ottino, J. (1989) (''The Kinematics of Mixing: Stretching, Chaos and Transport'' ). Cambridge Univ. Press. ISBN 9780521368780 * Parker, E.N. (1979) ''Cosmical Magnetic Fields: their Origin and their Activity''. Oxford Univ. Press. ISBN 9780198512905 *Ricca, R.L. (Ed.) (2009) (''Lectures on Topological Fluid Mechanics'' ). Springer-CIME Lecture Notes in Mathematics 1973. Springer-Verlag. Heidelberg, Germany. ISBN 9783642008368 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「topological fluid dynamics」の詳細全文を読む スポンサード リンク
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