A01=Kazunari Shibata
A01=Toshi Tajima
Accretion Disks
AGN
astrophysical plasma dynamics
Author_Kazunari Shibata
Author_Toshi Tajima
Average Field Strength
Category=PHFP
Category=PHVB
celestial
Celestial Objects
Coronal Loops
cosmic structure formation
disk
Dynamo Action
Energy Density
Energy Source
eq_bestseller
eq_isMigrated=1
eq_isMigrated=2
eq_nobargain
eq_non-fiction
eq_science
fields
Fluctuation Dissipation Theorem
fluctuations
flux
Flux Tube
galactic
Galactic Disk
Galactic Dynamo
graduate level physics
high-energy astrophysics
K. Shibata
Kink Instability
magnetic
Magnetic Buoyancy
Magnetic Diffusion Time
Magnetic Field Evolution
Magnetic Fields
Magnetic Fluctuations
Magnetic Flux Tube
Magnetic Force
magnetohydrodynamics theory
Molecular Clouds
objects
Plasma Astrophysics
plasma instability mechanisms
Plasma Physics
Solar Corona
Supermassive Black Hole
T. Tajima
tube
violent plasma processes in cosmology
Product details
- ISBN 9780813339962
- Weight: 453g
- Dimensions: 152 x 229mm
- Publication Date: 25 Jan 2002
- Publisher: Taylor & Francis Inc
- Publication City/Country: US
- Product Form: Paperback
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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 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 laboratory variety-- and their processes. The text continues with an exploration of the fundamental processes in hydrostatic, magnetostatic, and gravitational objects. The final chapter is devoted to a discussion of the applications of plasma astrophysics to cosmology, anticipating future developments in this exciting field.This text will be of enormous use to graduate-- and some advanced undergraduate-- students, as well as to physicists entering the field of plasma physics.
Toshiki Tajima is Director General at the Kansai Research Establishment, Japan Atomic Energy Research Institute in Kyoto. He was formerly the Jane and Roland Blumberg Professor in Theoretical Physics at the University of Texas at Austin. His research interests include accelerator physics and computational physics. He is co-author with Kazunari Shibata, of Plasma Astrophysics. Toshiki Tajima is professor of physics and computational and applied mathematics at The University of Texas at Austin, where he is also a member of the Institute for Fusion Studies. His research interests include accelerator physics and computational physics. Kazunari Shibata is associate professor of Astronomy at the National Astronomical Observatory in Tokyoo. He has taught a series of lectures on plasma astrophysics at Osaka University, the University of Tokyo, and Kyoto University. His interests include solar physics, X-ray astronomy, and magnetohydrodynamic astrophysics.
