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The twentieth century has witnessed the transformation of astronomy from celestial mechanics to astrophysics. While optical telescopes may have presented a peek into the structure of the constituents of the universe, such as stars and galaxies, new windows of observation have revealed far more amorphous objects, from nebulae and sheets to filaments and voids, whose “violent” processes include flares, shocks, accretion disks and jets. In these processes, plasma is often the constituent matter—as well as the medium through which the astrophysical setting becomes so violent. In this graduate-level text, Tajima and Shibata offer a new synthesis starting where the classic works on plasma physics left off. Beginning with a view of plasma astrophysics through fundamental processes of quasi-magnetostatic equilibria, quasi-hydrostatic equilibria, and non-equilibria, the authors go on to develop unique approaches to violent astrophysical plasmas—as opposed to the more quiescent ones.
This text investigates the role of plasma physics in driving the violent, non-equilibrium processes observed in celestial phenomena such as flares, shocks, and accretion disks. The authors, Kazunari Shibata and Toshiki Tajima, leverage their expertise in plasma dynamics to bridge the gap between classical celestial mechanics and modern astrophysical observation. By establishing a framework that moves beyond static models, they provide a rigorous mathematical and physical basis for understanding the energetic behavior of matter in the universe.
What You Will Find
Experts recognize this work as a foundational graduate-level text that successfully integrates plasma theory with observational astrophysics. Readers frequently note the high level of mathematical density and the specialized focus on non-equilibrium processes as key features of the volume.
Page Count:
512
Publication Date:
1997-09-22
Publisher:
Basic Books
ISBN-10:
020140642X
ISBN-13:
9780201406429
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