An Introduction To Plasma Astrophysics And Magnetohydrodynamics


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An Introduction to Plasma Astrophysics and Magnetohydrodynamics


An Introduction to Plasma Astrophysics and Magnetohydrodynamics

Author: M. Goossens

language: en

Publisher: Springer Science & Business Media

Release Date: 2012-12-06


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Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion. This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties. The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics.

An Introduction to Plasma Astrophysics and Magnetohydrodynamics


An Introduction to Plasma Astrophysics and Magnetohydrodynamics

Author: Marcel Goossens

language: en

Publisher:

Release Date: 2014-01-15


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Basics of Plasma Astrophysics


Basics of Plasma Astrophysics

Author: Claudio Chiuderi

language: en

Publisher: Springer

Release Date: 2014-11-22


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This book is an introduction to contemporary plasma physics that discusses the most relevant recent advances in the field and covers a careful choice of applications to various branches of astrophysics and space science. The purpose of the book is to allow the student to master the basic concepts of plasma physics and to bring him or her up to date in a number of relevant areas of current research. Topics covered include orbit theory, kinetic theory, fluid models, magnetohydrodynamics, MHD turbulence, instabilities, discontinuities, and magnetic reconnection. Some prior knowledge of classical physics is required, in particular fluid mechanics, statistical physics, and electrodynamics. The mathematical developments are self-contained and explicitly detailed in the text. A number of exercises are provided at the end of each chapter, together with suggestions and solutions.