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Lectures in Magnetohydrodynamics: With an Appendix on Extended MHD

Posted By: AvaxGenius
Lectures in Magnetohydrodynamics: With an Appendix on Extended MHD

Lectures in Magnetohydrodynamics: With an Appendix on Extended MHD by Dalton D. Schnack
English | PDF (True) | 2009 | 317 Pages | ISBN : 3642006876 | 5.5 MB

Magnetohydrodynamics, or MHD, is a theoretical way of describing the statics and dynamics of electrically conducting uids. The most important of these uids occurring in both nature and the laboratory are ionized gases, called plasmas. These have the simultaneous properties of conducting electricity and being electrically charge neutral on almost all length scales. The study of these gases is called plasma physics. MHD is the poor cousin of plasma physics. It is the simplest theory of plasma dynamics. In most introductory courses, it is usually afforded a short chapter or lecture at most: Alfven ´ waves, the kink mode, and that is it. (Now, on to Landau damping!) In advanced plasma courses, such as those dealing with waves or kinetic theory, it is given an even more cursory treatment, a brief mention on the way to things more profound and interesting. (It is just MHD! Besides, real plasma phy- cists do kinetic theory!) Nonetheless, MHD is an indispensable tool in all applications of plasma physics.

Turbulence in Space Plasmas (Repost)

Posted By: AvaxGenius
Turbulence in Space Plasmas (Repost)

Turbulence in Space Plasmas by Peter Cargill, Loukas Vlahos
English | PDF | 2009 | 332 Pages | ISBN : 3642002099 | 7.6 MB

Over the years, many leading European graduate schools in the field of astrophysical and space plasmas have operated within the framework of the research network, "Theory, Observations, and Simulations in Turbulence in Space Plasmas." This text is a set of lectures and tutorial reviews culled from the relevant work of all those schools. It emphasizes applications on solar coronae, solar flares, and the solar wind.