Book Description
Designed as a text for upper-level undergraduate and first-year graduate students, this volume attempts to establish the curriculum for the modern student entering the fledgling field of space physics. The book provides a broad, yet selective, treatment of the subject, covering virtually all aspects of space plasmas in the solar system. There are sections on the sun and solar wind, the magnetized and unmagnetized planets, and the fundamental process of space plasmas including shocks, plasma waves, ULF waves, wave-particle interactions, and auroral processes. In addition to emphasizing analysis, the authors also place importance on underlying phenomenology with extensive attention to observations.
Customer Reviews:
Space Physics? OH YEAH!.......2007-02-24
When I'm in the mood for a little exploration of stellar structure or maybe some light magnetohydrodynamics, this is the first thing I grab off the shelf. It's kept me interested and not at all wanting to gouge my eyeballs out for weeks!
Introduction to Space Physics.......2000-05-02
This is a very comprehensive book. It is excellent if you are beginer who knows basic electricity and magnetism, but have not dealt with space plasmas.
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Plasma Astrophysics and Space Physics
Manufacturer: Springer
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Binding: Hardcover
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ASIN: 0792360028 |
Book Description
In May 1998 a hundred renowned scientists from 20 different countries met at the Max-Planck-Institut für Aeronomie to communicate their latest results and ideas in astrophysical and space plasma, as a follow-up to previous similar meetings which were held in Varenna, Abastumai, Potsdam, Toki and Guaruja. The main papers emerging from this meeting are collected in this volume.
They deal with fundamental plasma phenomena, particle and radiation processes in astrophysics and space physics as the origin of magnetic activity, the basic mechanisms of particle acceleration and plasma heating common to plasma in galaxies and at the sun as well as in planetary magnetospheres. New observational results from YOHKOH, SOHO and other missions are presented. Using these, the basic physical processes leading to coronal heating and solar/stellar wind acceleration are discussed. Other topics are the microphysics of shock waves and transport phenomena in collisionless plasmas and the physics of thin plasma boundaries.
The volume also treats the ionic composition of plasma and dust in the Universe and their observability in the solar system. A CD-ROM is attached which adds a valuable multimedia component, illuminating results of observations, theory and simulations.
Everyone interested in astrophysical plasmas, its radiation and charged particle aspects, and advanced or even beginning students will find references to nearly all modern aspects of plasma astrophysics and space physics as well as an overview of current research results.
Book Description
The raw numbers of high-energy-density physics are amazing: shock waves at hundreds of km/s (approaching a million km per hour), temperatures of millions of degrees, and pressures that exceed 100 million atmospheres. This book introduces the reader to the fundamental tools and discoveries of high-energy-density physics. It surveys the production of high-energy-density conditions, the fundamental plasma and hydrodynamic models that can describe them and the problem of scaling from the laboratory to the cosmos. Connections to astrophysics will be discussed throughout. The book is intended to support coursework in high-energy-density physics, to meet the needs of new researchers in this field, and also to serve as a useful reference on the fundamentals.
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Turbulence, Current Sheets and Shocks in Cosmic Plasma (The Fluid Mechanics of Astrophysics and Geophysics, Vol 6)
S. Vainshtein
Manufacturer: Routledge
ProductGroup: Book
Binding: Hardcover
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ASIN: 2881248772 |
Book Description
This volume is devoted to the principal problems of cosmic electrodynamics: current sheets, turbulence, magnetic field generation, shock, and particle acceleration. By including the general concepts of magnetohydrodynamics and plasma physics, and the methods and results of modern investigations, along with their own unique ideas, the authors have provided an invaluable tool for graduate students and scientists in the field of cosmic electrodynamics.
Average customer rating:
- Good book for the field, but...
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Cosmic Ray Astrophysics
Reinhard Schlickeiser
Manufacturer: Springer
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Cosmic Rays and Particle Physics
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High Energy Astrophysics
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High Energy Astrophysics
ASIN: 3540664653 |
Book Description
This book provides an exhaustive account of the origin and dynamics of cosmic rays. Divided into three parts, it first gives an up-to-date summary of the observational data, then -- in the following theory section -- deals with the kinetic description of cosmic ray plasma. The underlying diffusion-convection transport equation, which governs the coupling between cosmic rays and the background plasma, is derived and analyzed in detail. In the third part, several applications of the solutions of the transport equation are presented and how key observations in cosmic ray physics can be accounted for is demonstrated. The applications include cosmic ray modulation, acceleration near shock waves and the galactic propagation of cosmic rays. While the book is primarily of interest to scientists working at the forefront of research, the very careful derivations and explanations make it suitable also as an introduction to the field of cosmic rays for graduate students.
Customer Reviews:
Good book for the field, but..........2002-12-13
Covers cosmic ray astrophysics pretty well, but I've opted to stick with volume 1 of Longair for the grad class is cosmic rays which I'm teaching this Spring. Why? This book seems to have huge gaps in its coverage and too much of a European focus with references. Still, it's a good book, and anyone working in cosmic rays is bound to buy it in the end...
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Auroral Plasma Physics (Space Sciences Series of ISSI)
Manufacturer: Springer
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Binding: Hardcover
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ASIN: 1402009631 |
Book Description
This volume gives a broad synthesis of the current knowledge and understanding of the plasma physics behind the aurora. The aurora is not only one of the most spectacular natural phenomena on Earth, but the underlying physical processes are expected to be ubiquitous in the plasma universe. Recognizing the enormous progress made over the last decade) through in situ and groundbased measurements as well as theoretical modelling, it seemed timely to write the first comprehensive and integrated book on the subject. Recent advances concern the clarification of the nature of the acceleration process of the electrons that are responsible for the visible aurora, the recognition of the fundamental role of the large-scale current systems in organizing the auroral morphology, and of the interplay between particles and electromagnetic fields.
Average customer rating:
- They call this a computational book?????
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Computational Plasma Physics: With Applications To Fusion And Astrophysics (Frontiers in Physics)
TAJIMA Tajima
Manufacturer: Westview Press
ProductGroup: Book
Binding: Paperback
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Plasma Physics via Computer Simulation (Series in Plasma Physics)
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Computer Simulation Using Particles
ASIN: 0813342112 |
Book Description
The physics of plasmas is an extremely rich and complex subject as the variety of topics addressed in this book demonstrates. This richness and complexity demands new and powerful techniques for investigating plasma physics. An outgrowth from his graduate course teaching, now with corrections, Tajima's text provides not only a lucid introduction to computational plasma physics, but also offers the reader many examples of the way numerical modeling, properly handled, can provide valuable physical understanding of the nonlinear aspects so often encountered in both laboratory and astrophysical plasmas. Included here are computational methods for modern nonlinear physics as applied to hydrodynamic turbulence, solitons, fast reconnection of magnetic fields, anomalous transports, dynamics of the sun, and more. The text contains examples of problems now solved using computational techniques including those concerning finite-size particles, spectral techniques, implicit differencing, gyrokinetic approaches, and particle simulation.
Customer Reviews:
They call this a computational book?????.......2006-02-21
Collection of theoretical background for computational methods. Poor description of the methods themselves. This book is difficult to read. You better be a top notch expert in plasma physics to get anything out of this one. I was able to learn a few bits here and there, save your money and buy something else.
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Magnetic Reconnection: MHD Theory and Applications
Eric Priest , and
Terry Forbes
Manufacturer: Cambridge University Press
ProductGroup: Book
Binding: Paperback
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Plasma Physics for Astrophysics (Princeton Series in Astrophysics)
ASIN: 0521033942 |
Book Description
Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak disruptions. Written by two world leaders on the subject, this volume provides a comprehensive overview of this fundamental process. Coverage gives both a pedagogical account of the basic theory and a wide-ranging review of the physical phenomena created by reconnection--from laboratory machines, the Earth's magnetosphere, and the Sun's atmosphere to flare stars and astrophysical accretion disks. It also includes a succinct account of particle acceleration by electric fields, stochastic fields and shock waves, and how reconnection can be important in these mechanisms. Clearly written and highly accessible, this volume serves as an essential introduction for graduate students in solar physics, astrophysics, plasma physics and space science. Researchers in these fields also will find Magnetic Reconnection an authoritative reference.
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Coronal Mass Ejections (Space Sciences Series of ISSI)
Manufacturer: Springer
ProductGroup: Book
Binding: Hardcover
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ASIN: 0387450866 |
Product Description
It is well known, that the Sun as central star of our solar system gravitationally controls the orbits of planets and minor bodies. Much less known is the domain of plasma, fields and charged particles, however, in which the Sun with a radius of less than 0.7 Million km governs the heliosphere out to about 15 Billion km, an area about 2000 times bigger in radius or nearly 10
10 times bigger in volume. What forces activates the Sun to maintain this power? Coronal Mass Ejections (CMEs) and their descendants are the troops serving the Sun during high solar activity periods.
This volume offers a comprehensive and integrated overview of our present knowledge and understanding of Coronal Mass Ejections (CMEs) and their descendants, Interplanetary CMEs (ICMEs). It results from a series of workshops held between 2000 and 2004. An international team of about sixty experimenters involved e.g. in the SOHO, ULYSSES, VOYAGER, PIONEER, HELIOS, WIND, IMP, and ACE missions, ground observers, and theoreticians worked jointly on interpreting the observations and developing new models for CME initiations, development, and interplanetary propagation.
The book is intended to provide scientists active in space physics research a with an up-to-date status of the current understanding of CMEs and ICMEs and their effects in the heliosphere, and also to serve the advanced graduate student with introductory material on this active field of research.
Book Description
Graduate students and researchers in astrophysics and cosmology need a solid grasp of a wide range of physical processes. This authoritative textbook helps readers develop the necessary toolkit of theory. The book is modular in design, allowing the reader to pick and chose a selection of chapters, if necessary. After reviewing the basics of dynamics, electromagnetic theory, and statistical physics, the book carefully develops a solid understanding of radiative processes, spectra, fluid mechanics, plasma physics and MHD, dynamics of gravitating systems, general relativity, nuclear physics, and other key concepts. Throughout, the reader's understanding is developed and tested with problems and helpful hints. This welcome volume provides graduate students with an indispensable introduction to and reference on all the physical processes they will need to successfully tackle cutting-edge research in astrophysics and cosmology. It can be used alone or in conjunction with two companion volumes, which cover stars and stellar systems, and galaxies and cosmology (both forthcoming).
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