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This is an advanced text on electromagnetic theory, presenting a
systematic discussion of electromagnetic waves and radiation
processes in a wide variety of media. The treatment, taken from the
field of plasma physics, is based on the dielectric tensor, and
this permits the discussion of media outside the scope of the usual
approach adopted in most textbooks on electromagnetism. The
approach taken also has notable advantages when applied to the
conventional emission processes of electromagnetic theory. The
authors have thus unified the approaches used in plasma physics and
astrophysics on the one hand, and in optics on the other. The book
has been written clearly and pedagogically, and will be therefore
of value to senior undergraduates, graduate students, lecturers and
researchers. Students will find the exercises provided at the end
of each chapter particularly useful.
This introductory account of instabilities in plasmas concentrates
on laboratory plasmas, such as those encountered in fusion
research, and the space plasmas studied in physics of the
magnetosphere and solar atmosphere. This account bridges the gap
between a graduate textbook on plasma physics, and specialized
similarities between astrophysical and laboratory plasmas that are
traditionally regarded as quite separate. The author, an expert in
plasma astrophysics who has written a two-volume book on the
subject, treats the material naturally, lending a broader
perspective to the subject. This is an instructional text for
graduate students and professionals in magnetospheric and
mathematical physics, radiophysics, solar and theoretical
astrophysics and radio astronomy.
This is an advanced text on electromagnetic theory, presenting a
systematic discussion of electromagnetic waves and radiation
processes in a wide variety of media. The treatment, taken from the
field of plasma physics, is based on the dielectric tensor, and
this permits the discussion of media outside the scope of the usual
approach adopted in most textbooks on electromagnetism. The
approach taken also has notable advantages when applied to the
conventional emission processes of electromagnetic theory. The
authors have thus unified the approaches used in plasma physics and
astrophysics on the one hand, and in optics on the other. The book
has been written clearly and pedagogically, and will be therefore
of value to senior undergraduates, graduate students, lecturers and
researchers. Students will find the exercises provided at the end
of each chapter particularly useful.
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