Home page Hans Goedbloed


Prof. Dr. J.P. Goedbloed

Advisor, FOM-Institute for Plasma Physics, Edisonbaan 14, 3439 MN Nieuwegein, the Netherlands

Professor emeritus Theoretical Plasma Physics, Astronomy Department, Utrecht University


E-mail: goedbloed@rijnh.nl

Tel.: +31 (0) 30 609 6999

Fax: +31 (0) 30 603 1204

http://www.rijnh.nl/users/goedbloed

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(charcoal by Henk van der Vorst)


Principles of Magnetohydrodynamics

·  Principles of Magnetohydrodynamics; with Applications to Laboratory and Astrophysical Plasmas,

by Hans Goedbloed and Stefaan Poedts (Cambridge University Press, 2004):

This textbook provides a modern and accessible introduction to magnetohydrodynamics (MHD). It describes the two main applications of plasma physics -- laboratory research on thermo-nuclear fusion energy and plasma-astrophysics of the solar system, stars and accretion disks -- from the single viewpoint of MHD. This approach provides effective methods and insights for the interpretation of plasma phenomena on virtually all scales, from the laboratory to the Universe. It equips the reader with the necessary tools to understand the complexities of plasma dynamics in extended magnetic structures. The classical MHD model is developed in detail without omitting steps in the derivations, and problems are included at the end of each chapter. This text is ideal for senior-level undergraduate and graduate courses in plasma physics and astrophysics.

ISBN 0521 6 2347 2 (hardback);

ISBN 0 521 62607 2 (paperback).

·  Book review by Prof. Eugene Parker: J. Fluid Mechanics (2004), 519, p. 377-379.

·  A workshop with the same name was held 21-24 March 2005 at Leiden University: Lorentz Center


Advanced Magnetohydrodynamics (to appear April 2010)

·  Advanced Magnetohydrodynamics; with Applications to Laboratory and Astrophysical Plasmas,

by Hans Goedbloed, Rony Keppens, and Stefaan Poedts (to be published with Cambridge University Press):

In this volume the restrictions to ideal dissipationless plasmas, in static equilibrium and with inhomogeneity in only one direction, that had to be made in Principles of Magnetohydrodynamics for educational purposes, are relaxed one by one. The analysis now allows for stationary background flows, resistivity and reconnection, two-dimensional toroidal geometry, linear and nonlinear computational techniques, and transonic flows and shocks. These topics transform the subject into a vital new area with numerous applications in laboratory (thermonuclear fusion), space (space weather), and astrophysical plasmas (stellar winds, accretion discs and jets).


[Errata] [Lectures] [Publications]


·  Errata on Principles of Magnetohydrodynamics:

ErrataPrMHD.pdf (updated 10 August 2009)


·  Lectures at Astronomy Department, University of Sao Paulo, March-May 2007:

AdvancedMHD.pdf (Description of the course)

MHD1.pdf (Introduction)

MHD2.pdf (Elements of plasma physics)

MHD4.pdf (The MHD model)

MHD5.pdf (Waves and characteristics)

MHD6.pdf (Spectral theory)

MHD7.pdf (Waves and instabilities in inhomogeneous plasmas)

MHD8.pdf (Magnetic structures and dynamics)

MHDF.pdf (Flow: Waves and instabilities in stationary plasmas)

MHDR.pdf (Resistive plasmas)

MHDT.pdf (Toroidal plasmas)

MHDS.pdf (Transonic MHD flows and shocks)

MHDapp.pdf (Appendices: Vector identies and Tables)

RT.tar.bz2 (Exercise of MHD7: Fortran files for Rayleigh-Taylor instability)

Solo.tar.bz2 (Exercise of MHDT: Fortran files for Soloviev equilibrium)


·  Publications Goedbloed et al.:

Publications.pdf (updated 29 January 2010)