Plasma physics for astrophysics, Kulsrud Russell M.

Автор: Juhan Frank
Название: Accretion Power in Astrophysics
ISBN: 0521629578 ISBN-13(EAN): 9780521629577
Издательство: Cambridge Academ
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Цена: 11563.00 р.
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Описание: Accretion Power in Astrophysics examines accretion as a source of energy in both binary star systems containing compact objects, and in active galactic nuclei. It describes the physical processes in accretion discs and other accretion flows. This expanded and updated edition is suitable for advanced undergraduates, graduate students and researchers.

Автор: Melia, Fulvio
Название: High-energy astrophysics
ISBN: 0691140294 ISBN-13(EAN): 9780691140292
Издательство: Wiley
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Цена: 13939.00 р.
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Описание: High-energy astrophysics involves the study of exceedingly dynamic and energetic phenomena occurring near the most extreme celestial objects known to exist, such as black holes, neutron stars, white dwarfs, and supernova remnants. This title introduces topics at the forefront of research, including relativistic particles, and energetic radiation.

Автор: Leblanc, Francis
Название: An introduction to stellar astrophysics
ISBN: 0470699566 ISBN-13(EAN): 9780470699560
Издательство: Wiley
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Цена: 7278.00 р.
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Описание: Fundamental to our understanding of the universe, stellar astrophysics deals with observations, theoretical understanding, classification, computer simulations and modeling of stars and their evolution.

Автор: Goossens M.
Название: An Introduction to Plasma Astrophysics and Magnetohydrodynamics
ISBN: 1402014295 ISBN-13(EAN): 9781402014291
Издательство: Springer
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Цена: 19591.00 р.
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Описание: 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.