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Magnetohydrodynamic Turbulence
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  • Cited by 209
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    This book has been cited by the following publications. This list is generated based on data provided by CrossRef.

    Akbas, M. Kaya, S. and Rebholz, L. G. 2016. On the stability at all times of linearly extrapolated BDF2 timestepping for multiphysics incompressible flow problems. Numerical Methods for Partial Differential Equations,

    Banerjee, Supratik and Galtier, Sébastien 2016. Chiral exact relations for helicities in Hall magnetohydrodynamic turbulence. Physical Review E, Vol. 93, Issue. 3,

    Chernyshov, A A and Petrosyan, A S 2016. Discrete filters for large-eddy simulation of forced compressible magnetohydrodynamic turbulence. Physica Scripta, Vol. 91, Issue. 6, p. 064002.

    Giovannini, Massimo 2016. Spectrum of anomalous magnetohydrodynamics. Physical Review D, Vol. 93, Issue. 10,

    Grappin, Roland Müller, Wolf-Christian and Verdini, Andrea 2016. Alfvén-dynamo balance and magnetic excess in magnetohydrodynamic turbulence. Astronomy & Astrophysics, Vol. 589, p. A131.

    Jurčišinová, E. Jurčišin, M. and Remecký, R. 2016. Turbulent Prandtl number in theAmodel of passive vector admixture. Physical Review E, Vol. 93, Issue. 3,

    KC, Amar and Chandy, Abhilash J. 2016. Assessment of Five SGS Models for Low-R e m MHD Turbulence. Flow, Turbulence and Combustion, Vol. 96, Issue. 3, p. 693.

    Lingam, Manasvi and Bhattacharjee, Amitava 2016. A heuristic model for MRI turbulent stresses in Hall MHD. Monthly Notices of the Royal Astronomical Society, Vol. 460, Issue. 1, p. 478.

    Mamatsashvili, George Dong, Siwei Khujadze, George Chagelishvili, George Jiménez, Javier and Foysi, Holger 2016. Homogeneous shear turbulence – bypass concept via interplay of linear transient growth and nonlinear transverse cascade. Journal of Physics: Conference Series, Vol. 708, p. 012001.

    Schaffner, D. A. Brown, M. R. and Rock, A. B. 2016. Possible signatures of dissipation from time-series analysis techniques using a turbulent laboratory magnetohydrodynamic plasma. Physics of Plasmas, Vol. 23, Issue. 5, p. 055709.

    Semikoz, V. B. Smirnov, A. Yu. and Sokoloff, D. D. 2016. Generation of hypermagnetic helicity and leptogenesis in the early Universe. Physical Review D, Vol. 93, Issue. 10,

    Seshasayanan, Kannabiran and Alexakis, Alexandros 2016. Critical behavior in the inverse to forward energy transition in two-dimensional magnetohydrodynamic flow. Physical Review E, Vol. 93, Issue. 1,

    Shebalin, John V. 2016. Dynamo action in dissipative, forced, rotating MHD turbulence. Physics of Plasmas, Vol. 23, Issue. 6, p. 062318.

    Subramanian, Kandaswamy 2016. The origin, evolution and signatures of primordial magnetic fields. Reports on Progress in Physics, Vol. 79, Issue. 7, p. 076901.

    Vlaykov, Dimitar G. Grete, Philipp Schmidt, Wolfram and Schleicher, Dominik R. G. 2016. A nonlinear structural subgrid-scale closure for compressible MHD. I. Derivation and energy dissipation properties. Physics of Plasmas, Vol. 23, Issue. 6, p. 062316.

    Xu, Siyao and Zhang, Bing 2016. INTERPRETATION OF THE STRUCTURE FUNCTION OF ROTATION MEASURE IN THE INTERSTELLAR MEDIUM. The Astrophysical Journal, Vol. 824, Issue. 2, p. 113.

    Zhdankin, Vladimir Boldyrev, Stanislav and Uzdensky, Dmitri A. 2016. Scalings of intermittent structures in magnetohydrodynamic turbulence. Physics of Plasmas, Vol. 23, Issue. 5, p. 055705.

    Zhdankin, Vladimir Boldyrev, Stanislav and Chen, Christopher H. K. 2016. Intermittency of energy dissipation in Alfvénic turbulence. Monthly Notices of the Royal Astronomical Society: Letters, Vol. 457, Issue. 1, p. L69.

    Chen, C. H. K. Matteini, L. Burgess, D. and Horbury, T. S. 2015. Magnetic field rotations in the solar wind at kinetic scales. Monthly Notices of the Royal Astronomical Society: Letters, Vol. 453, Issue. 1, p. L64.

    Dallas, V. and Alexakis, A. 2015. Self-organisation and non-linear dynamics in driven magnetohydrodynamic turbulent flows. Physics of Fluids, Vol. 27, Issue. 4, p. 045105.

  • Dieter Biskamp, Max-Planck-Institut für Plasmaphysik, Garching, Germany

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Book description

This book presents an introduction to, and modern account of, magnetohydrodynamic (MHD) turbulence, an active field both in general turbulence theory and in various areas of astrophysics. The book starts by introducing the MHD equations, certain useful approximations and the transition to turbulence. The second part of the book covers incompressible MHD turbulence, the macroscopic aspects connected with the different self-organization processes, the phenomenology of the turbulence spectra, two-point closure theory, and intermittency. The third considers two-dimensional turbulence and compressible (in particular, supersonic) turbulence. Because of the similarities in the theoretical approach, these chapters start with a brief account of the corresponding methods developed in hydrodynamic turbulence. The final part of the book is devoted to astrophysical applications: turbulence in the solar wind, in accretion disks, and in the interstellar medium. This book is suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.


‘… this new book by Biskamp presents hydromagnetic turbulence as a very accessible and highly interesting topic both for students and professionals … an ideal reference both for beginners and experts … This book should certainly belong to the compulsory literature of any graduate student working in hydromagnetic turbulence.’

Source: Journal of Fluid Mechanics

‘… recommended to anybody working in the field, including graduate students.’

Source: Geophysical and Astrophysical Fluid Dynamics

'… I would recommend this book to all those who would like to undertake a serious study of MHD turbulence, be it from a theoretical point of view or because they are interested in applications.'

Source: Journal of Plasma Physics

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