Plasma Physics for Astrophysics / / Russell M. Kulsrud.
In this book, a distinguished expert introduces plasma physics from the ground up, presenting it as a comprehensible field that can be grasped largely on the basis of physical intuition and qualitative reasoning, similar to other fields of physics. Plasmas are ionized gases that can be found in a hy...
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Superior document: | Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Backlist 2000-2013 |
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Place / Publishing House: | Princeton, NJ : : Princeton University Press, , [2020] ©2005 |
Year of Publication: | 2020 |
Language: | English |
Online Access: | |
Physical Description: | 1 online resource (496 p.) :; 140 line illus. |
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100 | 1 | |a Kulsrud, Russell M., |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
245 | 1 | 0 | |a Plasma Physics for Astrophysics / |c Russell M. Kulsrud. |
264 | 1 | |a Princeton, NJ : |b Princeton University Press, |c [2020] | |
264 | 4 | |c ©2005 | |
300 | |a 1 online resource (496 p.) : |b 140 line illus. | ||
336 | |a text |b txt |2 rdacontent | ||
337 | |a computer |b c |2 rdamedia | ||
338 | |a online resource |b cr |2 rdacarrier | ||
347 | |a text file |b PDF |2 rda | ||
505 | 0 | 0 | |t Frontmatter -- |t CONTENTS -- |t List of Figures -- |t Foreword -- |t Preface -- |t Chapter 1. Introduction -- |t Chapter 2. Particle Motions -- |t Chapter 3. Magnetohydrodynamics -- |t Chapter 4. Conservation Relations -- |t Chapter 5. MHD Waves -- |t Chapter 6. Nonlinear Steepening and Shocks -- |t Chapter 7. The Energy Principle and Instabilities -- |t Chapter 8. Collisions and the Braginski Equations -- |t Chapter 9. Collisionless Plasmas -- |t Chapter 10. Collisionless Plasmas:Thermal Effects -- |t Chapter 11. Nonlinear Phenomena -- |t Chapter 12. Cosmic Rays -- |t Chapter 13. Astrophysical Dynamos -- |t Chapter 14. Magnetic Reconnection -- |t Suggested Further Reading -- |t Index |
506 | 0 | |a restricted access |u http://purl.org/coar/access_right/c_16ec |f online access with authorization |2 star | |
520 | |a In this book, a distinguished expert introduces plasma physics from the ground up, presenting it as a comprehensible field that can be grasped largely on the basis of physical intuition and qualitative reasoning, similar to other fields of physics. Plasmas are ionized gases that can be found in a hydrogen bomb explosion, the confinement chamber of an experimental fusion reactor, the solar corona, the aurora borealis, the interstellar medium, and the immediate vicinity of a gravitational black hole. Not surprisingly, plasma physics appears to consist of numerous topics arising independently from astrophysics, fusion physics, and other practical applications, and hence it remains a field poorly understood even by many astrophysicists. But, in fact, most of these topics can be approached from the same perspective, with a simple, physical intuition. Selecting simple examples and presenting them in a simultaneously intuitive and rigorous manner, Russell Kulsrud guides readers through a careful derivation of the results and allows them to think through the physics for themselves. Thus, they are better prepared for complex cases and more general results. The first eleven chapters present topics by their importance to plasma physics while the last three chapters emphasize the field's astrophysical applications, applying the results accrued earlier. Throughout, many problems illustrate the field's applications. Based on a course the author taught for many years, Plasma Physics for Astrophysics is intended for graduate students as well as for working astrophysicists. | ||
538 | |a Mode of access: Internet via World Wide Web. | ||
546 | |a In English. | ||
588 | 0 | |a Description based on online resource; title from PDF title page (publisher's Web site, viewed 30. Aug 2021) | |
650 | 0 | |a Plasma astrophysics. | |
650 | 7 | |a SCIENCE / Physics / General. |2 bisacsh | |
653 | |a Accretion disk. | ||
653 | |a Alfven time. | ||
653 | |a Bessel function. | ||
653 | |a Braginski equations. | ||
653 | |a Charge neutrality. | ||
653 | |a Compression. | ||
653 | |a Contour integration. | ||
653 | |a Critical drift velocity. | ||
653 | |a Dalembertian solution. | ||
653 | |a Debye length. | ||
653 | |a Downstream region. | ||
653 | |a Earth's magnetic field. | ||
653 | |a Entropy. | ||
653 | |a Faraday rotation. | ||
653 | |a Flux freezing. | ||
653 | |a Guide field. | ||
653 | |a Helicity spectrum. | ||
653 | |a Impact parameter. | ||
653 | |a Ion acoustic mode. | ||
653 | |a Jump conditions. | ||
653 | |a Laplace transform. | ||
653 | |a Magnetic reconnection. | ||
653 | |a Magnetic tension. | ||
653 | |a Maxwell distribution. | ||
653 | |a Ohm's law. | ||
653 | |a Parallel viscosity. | ||
653 | |a Quasi neutrality. | ||
653 | |a Shocks. | ||
653 | |a Solar flare. | ||
653 | |a Topology. | ||
700 | 1 | |a Bahcall, John N., |e contributor. |4 ctb |4 https://id.loc.gov/vocabulary/relators/ctb | |
773 | 0 | 8 | |i Title is part of eBook package: |d De Gruyter |t Princeton University Press eBook-Package Backlist 2000-2013 |z 9783110442502 |
856 | 4 | 0 | |u https://doi.org/10.1515/9780691213354?locatt=mode:legacy |
856 | 4 | 0 | |u https://www.degruyter.com/isbn/9780691213354 |
856 | 4 | 2 | |3 Cover |u https://www.degruyter.com/cover/covers/9780691213354.jpg |
912 | |a 978-3-11-044250-2 Princeton University Press eBook-Package Backlist 2000-2013 |c 2000 |d 2013 | ||
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