Plasma physics Books

Book Synopsis''This book is an important contribution, and I hope it will open many minds. What is particularly important in it are the discussions of David Bohm, of bioplasma, biophotons, and bioelectronics.'' - PROFESSOR ZBIGNIEW WOLKOWSKI, Sorbonne University, ParisAnswers so many questions, scientific and esoteric, about the true nature of our reality... A seminal work... Will revolutionise how we frame reality and the thinking of everyone on this planet. Kudos to Professor Temple for striking the first match to light the fire. - NEW DAWNThe story of the science of plasma and its revolutionary implications for the way we understand the universe and our place in it.Histories of science in the 20th century have focused on relativity and quantum mechanics. But, quietly in the background, there has been a third area of exploration which has equally important implications for our understanding of the universe. It is unknown to the general public despite the fact tha

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Book SynopsisThe beautiful aurorae, or northern lights, are the stuff of legends. The ancient stories of the Sami people warn that if you mock the lights they will seize you, and their mythical appeal continues to capture the hearts and imagination of people across the globe.Aurora explores the visual beauty, ancient myths and science of the northern lights and challenges the popular theory of how the lights are formed. Plasma physicist Melanie Windridge explains this extraordinary and evocative phenomenon, a scientific marvel unlike any other in which the powers of astronomy, geology, magnetism and atomic physics combine to create one of the wonders of the natural world.As Melanie travels in search of the perfect aurora, she uncovers the scientific realities of this plasmic phenomenon full of natural power. She combines the science behind the lights with a fascinating travelogue as she pursues the aurora across the northern hemisphere from the Arctic Circle to Scotland.Trade Review‘Captivating’ Nature ‘Spell-binding … a brilliant blend of auroral science, polar exploration, Sami heritage and folklore … full of wonders.’ The Simple Things ‘Her greatest strength is her ability to illuminate science for the lay person.’ Literary Review ‘Her enthusiasm for all things aurora is, ultimately, infectious and there will be something of interest here for anyone with even a passing curiosity in this remarkable natural phenomenon’ The Times Literary Supplement

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Book SynopsisFor over 60 years, scientists and engineers have been trying to crack a seemingly intractable problem: how to build practical devices that exploit nuclear fusion. Access to electricity has facilitated a standard of living that was previously unimaginable, but as the world’s population grows and developing nations increasingly reap the benefits of electrification, we face a serious global problem: burning fossil fuels currently produces about eighty percent of the world's energy, but it produces a greenhouse effect that traps outgoing infrared radiation and warms the planet, risking dire environmental consequences unless we reduce our fossil fuel consumption to near zero in the coming decades. Nuclear fusion, the energy-producing process in the sun and stars, could provide the answer: if it can be successfully harnessed here on Earth, it will produce electricity with near-zero CO2 byproduct by using the nuclei in water as its main fuel. The principles behind fusion are understood, but the technology is far from being fully realized, and governments, universities, and venture capitalists are pumping vast amounts of money into many ideas, some highly speculative, that could lead to functioning fusion reactors. This book puts all of these attempts together in one place, providing clear explanations for readers who are interested in new energy technologies, including those with no formal training in science or engineering. For each of the many approaches to fusion, the reader will learn who pioneered the approach, how the concept works in plain English, how experimental tests were engineered, the future prospects, and comparison with other approaches. From long-established fusion technologies to emerging and exotic methods, the reader will learn all about the idea that could eventually constitute the single greatest engineering advance in human history.Trade Review“Moynihan contributed his expertise as a ‘fusioneer’ – with a background in fusion-related doctoral work … and, critically, his limitless enthusiasm. … ‘Fusion’s Promise’ is a book with a clear mission. … we are now starting to see the ‘promise’ of Moynihan and Bortz’s book title, thanks to a number of convergent factors.” (Nick Smith, E&T Engineering and Technology, eandt.theiet.org, July 12, 2023)Table of Contents1. Introduction: Fusion Basics.- 2. Exciting Fusion Developments.- 3. Pinches.- 4. Mirrors.- 5. Cusps.- 6. Tokamaks & Stellarators.- 7. Field Reversed Configuration.- 8. Inertial Electrostatic Confinement.- 9. Ion Beams.- 10. Plasma Cannons.- 11. Inertial Confinement Fusion.- 12. Liquid Metal.- 13. Conclusion: Achieving a Fusion-Powered Future.

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Book SynopsisChapter 1: Introduction.- Chapter 2: Ball Lightning: Observers’ Tales.- Chapter 3: The Search for Photographic Evidence.- Chapter 4: A Bit of Philosophy, or What Has a Razor to Do with Ball Lightning?.- Chapter 5: Organizing and Analyzing The Observations.- Chapter 6: Electrical Discharges, Coronas, and Streamers.- Chapter 7: Thunderstorms and Lightning.- Chapter 8: BL: Well Documented Cases of Copious Production.- Chapter 9: The Link Between Lightning Physics and Ball Lightning.- Chapter 10: Some People Just Won’t Believe It: The Skeptic’s View.- Chapter 11: Ball Lightning Theories.- Chapter 12: BL Experiments.- Chapter 13: Wrapping It All Up.

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Book SynopsisThis book gives an accessible overview of the 70-year history of nuclear fusion research and the vain attempts to construct an energy-generating nuclear fusion reactor. It shows that even in the most optimistic scenario nuclear fusion, despite the claims of its proponents and the billions being spent on research, will not be able to make a sizable contribution to the energy mix in this century. The important consequence is that nuclear fusion will not be a factor in combating climate change, since the race for carbon-free energy will have been won or lost long before the first nuclear fusion power station comes on line. Table of ContentsPreface.- What is nuclear fusion?.- Stellar processes and quantum mechanics.- Nuclear fusion of light elements.- Plasma.- Plasma in nuclear fusion devices.- Early history and declassification.- Birth of the tokamak.- The tokamak stampede and further developments.- The Big Tokamaks: TFTR, JET, JT-60.- The International Thermonuclear Experimental Reactor.- Problems, problems, problems….- Post-ITER: Demo and fusion power plants.- Spherical tokamaks.- Stellarators and other alternative approaches.- Privately funded research.- Criticism of the fusion enterprise.- Economics and sustainability.- Environment and safety.- Summary and final conclusion.

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Book SynopsisThis rigorous explanation of plasmas is relevant to diverse plasma applications. More thorough than previous texts, it exploits new powerful techniques to develop deeper insights into plasma behavior. Written for advanced students, it explores a host of essential and advanced topics while emphasizing the fundamentals that apply to all plasmas.Trade ReviewReview of the hardback: 'A conscientious and elegantly produced textbook … single-particle orbit theory and linearized waves in unbounded plasma are particularly well done … A lot can be learned from it. Picking up the text and reading it at random is often rewarding.' D. C. Montgomery, Theoretical and Computational Fluid Dynamics'Gives an exceptionally lucid and compelling overview of recent progress in this broad branch of physics. The unique organization of the book and straightforward writing style reflect the extensive teaching background of the author … A welcome addition to the library of both the expert and the newcomer to the field.' Geophysical and Astrophysical Fluid Dynamics'The book will undoubtedly be valued by those doing postgraduate work in this field, for whom it provides a useful bridge to the scientific literature. It is also highly recommended to researchers looking to widen their horizons to other areas of plasma physics outside their area of expertise.' Zulfikar Najmudin, The Times Higher Education SupplementTable of ContentsPreface; 1. Basic concepts; 2. The Vlasov, two-fluid, and MHD models of plasma dynamics; 3. Motion of a single plasma particle; 4. Elementary plasma waves; 5. Streaming instabilities and the Landau problem; 6. Cold plasma waves in a magnetized plasma; 7. Waves in inhomogeneous plasmas and wave energy relations; 8. Vlasov theory of warm electrostatic waves in a magnetized plasma; 9. MHD equilibria; 10. Stability of static MHD equilibria; 11. Magnetic helicity interpreted and Woltjer–Taylor relaxation; 12. Magnetic reconnection; 13. Fokker–Planck theory of collisions; 14. Wave-particle nonlinearities; 15. Wave-wave nonlinearities; 16. Non-neutral plasmas; 17. Dusty plasmas; Appendix A. Intuitive method for vector calculus identities; Appendix B. Vector calculus in orthogonal curvilinear coordinates; Appendix C. Frequently used physical constants and formulae; Bibliography; References; Index.

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Book SynopsisA good working knowledge of fluid mechanics and plasma physics is essential for the modern astrophysicist. This graduate textbook provides a clear, pedagogical introduction to these core subjects. Assuming an undergraduate background in physics, this book develops fluid mechanics and plasma physics from first principles. This book is unique because it presents neutral fluids and plasmas in a unified scheme, clearly indicating both their similarities and their differences. Also, both the macroscopic (continuum) and microscopic (particle) theories are developed, establishing the connections between them. Throughout, key examples from astrophysics are used, though no previous knowledge of astronomy is assumed. Exercises are included at the end of chapters to test the reader's understanding. This textbook is aimed primarily at astrophysics graduate students. It will also be of interest to advanced students in physics and applied mathematics seeking a unified view of fluid mechanics and plaTrade Review'I'd not hesitate to recommend [this] book to anybody with an interest in fluids or plasmas … superbly written … [an] original textbook which should quickly become a bestseller.' Uriel Frisch, CNRS, Observatoire de Nice'[This] book provides a comprehensive introduction both to fluid dynamics and to plasma physics, with many astrophysical examples. Here at last is an excellent textbook for a theoretical course, at graduate level, in plasma astrophysics.' Nigel O. Weiss, FRS, University of Cambridge'The text is unique in combining the essential formal calculations with the simple physical concepts to give the reader an intuitive grasp of the dynamical phenomena of the active astonomical universe … The new student, as well as the experienced research worker, will find this textbook useful and instructive.' Eugene Parker, University of Chicago'… it is rare to find a textbook that is such a pleasure to read.' S. M. Tobias, Journal of Fluid Mechanics'This is a delightful book, largely because of the author's evident enthusiasm for the subject. It is a pleasure to find such potentially messy subjects as plasma physics and hydrodynamics presented as a unified whole with the grand themes well brought out. The text is strong on physical insight and clarity of exposition … this is an excellent book … A copy should be available on the bookshelves of every astrophysics research group.' A. R. Bell, Blackett Laboratory, Imperial College'This is an excellent book. The author has that rare gift of being able to make a complex subject seem not only straightforward but also fascinating … an absolute bargain at the price.' Moira Jardine, The Observatory'I enjoyed reading this book, and found the author's viewpoints fresh and interesting. He manages to entertain the reader and succeeds in conveying the essentials of the subject simultaneously. It is a rare textbook that is as well written and presented as this.' Current Science'The book is well written, covering quite a large number of topics in a clear and pleasant style which makes enjoyable reading … The student who reads this book will successfully gain a very good understanding of many, often referred to, astrophysical topics.' R. M. Kulsrud, Nuclear FusionTable of ContentsIntroduction; Part I. Neutral Fluids: 2. Boltzmann equation; 3. March towards hydrodynamics; 4. Properties of ideal fluids; 5. Viscous flows; 6. Gas dynamics; 7. Linear theory of waves and instabilities; 8. Turbulence; 9. Rotation and hydrodynamics; Part II. Plasmas: 10. Plasma orbit theory; 11. Dynamics of many charged particles; 12. Collisionless processes in plasmas; 13. Collisional processes and the one-fluid model; 14. Basic magnetohydrodynamics; 15. Theory of magnetic topologies; 16. Dynamo theory; Appendices: A. Useful vector relations; B. Integrals in kinetic theory; C. Formulae and equations in cylindrical and spherical coordinates; D. Values of various quantities; E. Basic parameters pertaining to plasmas; Suggestions for further reading; References.

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Book SynopsisThis textbook, derived from courses given by three leading researchers, provides advanced undergraduates and graduates with up-to-date coverage of space physics, from the Sun to the interstellar medium. Clear explanations of the underlying physical processes are presented alongside major new discoveries and knowledge gained from space missions, ground-based observations, theory, and modelling to inspire students. Building from the basics to more complex ideas, the book contains enough material for a two-semester course but the authors also provide suggestions for how the material can be tailored to fit a single semester. End-of-chapter problems reinforce concepts and include computer-based exercises specially developed for this textbook package. Free access to the software is available via the book''s website and enables students to model the behavior of magnetospheric and solar plasma. An extensive glossary recaps new terms and carefully selected further reading sections encourage stuTrade Review'[This book] provides a significant update of scientific material in the rapidly changing field of space plasma physics while maintaining a level appropriate for seniors and beginning graduate students. I look forward to using this text the next time I teach my course.' Mary Hudson, Dartmouth College, New Hampshire'This is a very welcome update, which makes excellent use of recent advances in simulation techniques to illustrate concepts, and each chapter ends with a valuable set of problems, many of which are linked to online resources and applications. I have no doubt that this volume will rapidly become the standard recommended textbook for those teaching both basic and advanced courses in space plasmas.' Christopher Owen, University College London'Space Physics boasts clear and thorough discussions of the physics and phenomenology of our space environment, illustrated by a wealth of diagrams and examples from spacecraft observations. It is an ideal launch pad for students new to space physics with web-based software complementing many of the problems at the end of each chapter, enabling students to explore interactively the physics of our space environment.' Gregory Howes, University of Iowa'Providing a complete and in-depth coverage of space physics, this refreshing new contribution to teaching in space physics is well written, simple and clear. It's an excellent textbook for introductory courses and a valuable reference for any space physics researcher.' Hui Zhang, University of Alaska, Fairbanks'As this is an update to an earlier text published in 1995, some chapters have been thoroughly revised while others replaced but the essence is still the same. The authors have designed it to include all the required material, enough for a two-semester graduate course. Each chapter comes with a set of carefully selected additional readings with reasons why they are of interest given; and problem sets, some of which are in the form of lab exercises that are entirely online. The book does not stop at solar-terrestrial problems; the effects of solar wind on other planets and planetary aurora are discussed as well. Apart from graduate students, other parties that will find it a good investment are new lecturers of advanced undergraduate plasma physics course looking to get their hands on a comprehensive text for their lectures or existing ones needing to update their repertoire.' B. Ishak, Contemporary PhysicsTable of ContentsPreface; 1. Solar terrestrial physics: the evolution of a discipline; 2. The upper atmosphere and ionosphere; 3. Physics of magnetized plasmas; 4. The Sun and its atmosphere; 5. The solar wind and heliosphere; 6. Collisionless shocks; 7. Solar wind interaction with magnetized obstacles; 8. Plasma interactions with unmagnetized bodies; 9. Solar wind magnetosphere coupling; 10. The terrestrial magnetosphere; 11. The aurora; 12. Planetary magnetospheres; 13. Plasma waves; Appendix 1. Notation, vector identities, and differential operators; Appendix 2. Fundamental constants and plasma parameters of space physics; Appendix 3. Geophysical coordinate transformations; Appendix 4. Time series analysis techniques; Glossary; References; Index.

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Book SynopsisThis book is based on Valery Zagrebaev's original papers and lecture materials on nuclear physics with heavy ions, which he prepared and extended through many years for the students of nuclear physics specialties.Thе book outlines the main experimental facts on nuclear reactions involving heavy ions at low energies. It focuses on discussions of nuclear physics processes that are a subject of active, modern research and it gives illustrative explanations of these phenomena in the framework of up-to-date theoretical concepts.This textbook is intended for students in physics who have completed a standard course of quantum mechanics and have basic ideas of nuclear physics processes.It is designed as a kind of lifeboat that, at the end of the course, will allow students to navigate the modern scientific literature and to understand the goals and objectives of current, on-going research.Table of Contents1. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62. Nuclear interactions and classes of nuclear reaction . . . . . . . . . 122.1. Nucleon-nucleon and nucleon-nucleus interactions, nuclear mean field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122.2. Nucleus-nucleus interaction: folding and phenomenological potentials. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162.2.1. Folding potentials . . . . . . . . . . . . . . . . . . . . . 172.2.2. Woods-Saxon potential . . . . . . . . . . . . . . . . . . 202.2.3. Proximity potential . . . . . . . . . . . . . . . . . . . . 212.2.4. Bass potential . . . . . . . . . . . . . . . . . . . . . . . 222.2.5. Comparison of diabatic potentials for the nucleus-nucleusinteraction . . . . . . . . . . . . . . . . . . . . . . . . . 232.2.6. Dependence of potential energy on nuclear orientation . 232.2.7. Dependence of potential energy on dynamical deformations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 252.3. Classification of nuclear reactions, experimental procedures, cross sections and kinematics . . . . . . . . . . . . . . . 273. Elastic scattering of nucleons and heavy ions . . . . . . . . . . . . . 343.1. Scattering in a Coulomb field . . . . . . . . . . . . . . . . . . . 343.2. Elastic scattering of protons and neutrons. Optical model . . . 373.3. Elastic scattering of light ions . . . . . . . . . . . . . . . . . . 433.4. Applicability of classical mechanics and trajectory analyses . . 453.5. Nuclear rainbow and diffraction scattering . . . . . . . . . . . . 493.6. Elastic scattering of heavy ions . . . . . . . . . . . . . . . . . . 564. Quasi-elastic scattering of heavy ions and few-nucleon transfer reactions. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 584.1. Direct process of light-particle transfer . . . . . . . . . . . . . . 594.2. Distorted-wave description of direct reactions . . . . . . . . . . 614.3. Single-particle states and cluster states, spectroscopic factors . 624.4. Inelastic excitation of vibrational and rotational states . . . . . 654.5. Quasi-elastic scattering of heavy ions . . . . . . . . . . . . . . 684.6. Reactions of few-nucleon transfer . . . . . . . . . . . . . . . . . 745. Deep-inelastic scattering of nuclei . . . . . . . . . . . . . . . . . . . 785.1. Experimental systematics of deep-inelastic scattering and quasifission. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 795.2. Potential energy of heavy nuclear systems, diabatic and adiabatic driving potentials . . . . . . . . . . . . . . . . . . . . . . 855.2.1. Nucleon transfer and driving potentials . . . . . . . . . 855.2.2. Macro-microscopic model and the adiabatic potential energy. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 865.3. Transport equations for deep-inelastic nuclear collisions: Frictional forces . . . . . . . . . . . . . . . . . . . . . . . . . . . . 915.4. Calculation of deep-inelastic cross sections . . . . . . . . . . . 965.5. Analysis of deep-inelastic scattering and quasi-fission . . . . . . 995.6. Multi-nucleon transfer reactions. Synthesis of heavy neutronrich nuclei . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1046. Fusion of atomic nuclei . . . . . . . . . . . . . . . . . . . . . . . . . 1136.1. Detecting fission fragments and evaporation residues from the compound nucleus . . . . . . . . . . . . . . . . . . . . . . . . . 1146.2. Statistical model for the decay of an excited nucleus . . . . . . 1166.3. Fusion at above-barrier energies . . . . . . . . . . . . . . . . . 1256.4. Sub-barrier fusion. Hill–Wheeler formula . . . . . . . . . . . . 1276.5. Coupled channels. Empirical and quantum description of fusion 1296.6. Barrier distribution function . . . . . . . . . . . . . . . . . . . 1346.7. Neutron transfer in the process of sub-barrier fusion . . . . . . 1356.8. Synthesis of superheavy elements in fusion reactions . . . . . . 1426.9. Radiative capture of light nuclei . . . . . . . . . . . . . . . . . 160References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166

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Book SynopsisThis didactic book uses a data-driven approach to connect measurements made by plasma instruments to the real world. This approach makes full use of the instruments’ capability and examines the data at the most detailed level an experiment can provide. Students using this approach will learn what instruments can measure, and working with real-world data will pave their way to models consistent with these observations. While conceived as a teaching tool, the book contains a considerable amount of new information. It emphasizes recent results, such as particle measurements made from the Cluster ion experiment, explores the consequences of new discoveries, and evaluates new trends or techniques in the field. At the same time, the author ensures that the physical concepts used to interpret the data are general and widely applicable. The topics included help readers understand basic problems fundamental to space plasma physics. Some are appearing for the first time in a space physics textbook. Others present different perspectives and interpretations of old problems and models that were previously considered incontestable. This book is essential reading for graduate students in space plasma physics, and a useful reference for the broader astrophysics community. Table of Contents1 Basic Equations and Concepts 11.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11.2 Fundamental Equations . . . . . . . . . . . . . . . . . . . . . . . 21.3 Statistical Equations . . . . . . . . . . . . . . . . . . . . . . . . . 41.4 Electric and Magnetic Field in Space . . . . . . . . . . . . . . . . 71.5 Transformation of E and B Fields . . . . . . . . . . . . . . . . . 111.6 Macroscopic Equations . . . . . . . . . . . . . . . . . . . . . . . . 181.7 Plasma Measurements . . . . . . . . . . . . . . . . . . . . . . . . 221.8 Examples of Plasma Distributions . . . . . . . . . . . . . . . . . 311.9 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 342 Charged Particle Acceleration 392.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 392.2 Motion in Uniform E and B Field . . . . . . . . . . . . . . . . . 402.3 E ⇥ B Acceleration . . . . . . . . . . . . . . . . . . . . . . . . . 452.4 Motion in Inhomogeneous Magnetic Field . . . . . . . . . . . . . 572.5 Other Particle Acceleration Mechanisms . . . . . . . . . . . . . . 632.6 Waves and Wave-Particle Interaction . . . . . . . . . . . . . . . . 682.7 Cyclotron Resonance Theory . . . . . . . . . . . . . . . . . . . . 722.8 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 783 Escaping Solar Particles 813.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 813.2 Observations of Solar Wind Ions . . . . . . . . . . . . . . . . . . 833.3 Observations of Solar Wind Electrons . . . . . . . . . . . . . . . 913.4 Solar Wind Models . . . . . . . . . . . . . . . . . . . . . . . . . . 963.5 Kinetic Models of the SW . . . . . . . . . . . . . . . . . . . . . . 993.6 Heuristic Interpretation of the Solar Wind . . . . . . . . . . . . . 1043.7 Electrostatic Solitary Waves . . . . . . . . . . . . . . . . . . . . . 1083.8 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 1104 Collisionless Shocks 1174.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1174.2 Observations of Earth’s Bow Shock . . . . . . . . . . . . . . . . . 1194.3 Entropy Across Earth’s Bow Shock . . . . . . . . . . . . . . . . . 1254.4 ICME Shock . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1334.5 Nonlinear Structures Upstream of Bow Shock . . . . . . . . . . . 1404.6 Growth of Nonlinear Structure . . . . . . . . . . . . . . . . . . . 1584.7 Acceleration of Particles at the Bow Shock . . . . . . . . . . . . 1614.8 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 1655 Current Sheets and Boundaries 1835.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1835.2 Magnetic Reconnection on Earth . . . . . . . . . . . . . . . . . . 1845.3 SW Entry into Magnetosphere through Cusps . . . . . . . . . . . 1915.4 Particle Motions in Magnetic Neutral Regions . . . . . . . . . . . 1985.5 Kinetic Models of Current Sheets . . . . . . . . . . . . . . . . . . 2045.6 Kinetic Equations for Boundaries . . . . . . . . . . . . . . . . . . 2085.7 Tearing Mode Instability . . . . . . . . . . . . . . . . . . . . . . . 2145.8 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 2186 Current and Electric Field 2256.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2256.2 Observations of Electron and Ion Beams . . . . . . . . . . . . . . 2266.3 Motion Parallel to E and B Fields . . . . . . . . . . . . . . . . . 2316.4 Electric Potential . . . . . . . . . . . . . . . . . . . . . . . . . . . 2366.5 A Model of Double Layer . . . . . . . . . . . . . . . . . . . . . . 2466.6 Currents in the Magnetosphere and Ionosphere . . . . . . . . . . 2516.7 Ring Current in Magnetospheres . . . . . . . . . . . . . . . . . . 2566.8 Magnetosphere-Ionosphere Coupling . . . . . . . . . . . . . . . . 2646.9 Auroral Kilometric Radiation . . . . . . . . . . . . . . . . . . . . 2726.10 Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . 2757 Topics for Further Studies 2817.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2817.2 Large-scale Current Structures . . . . . . . . . . . . . . . . . . . 2817.3 Heating Space Plasmas . . . . . . . . . . . . . . . . . . . . . . . . 2847.4 Boltzmann Collisional Term (@f/@t)c . . . . . . . . . . . . . . . 2867.5 Runaway Electrons . . . . . . . . . . . . . . . . . . . . . . . . . . 2927.6 Collective Interactions . . . . . . . . . . . . . . . . . . . . . . . . 295

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Book SynopsisThis book explores several key issues in beam phase space dynamics in plasma-based wakefield accelerators. It reveals the phase space dynamics of ionization-based injection methods by identifying two key phase mixing processes. Subsequently, the book proposes a two-color laser ionization injection scheme for generating high-quality beams, and assesses it using particle-in-cell (PIC) simulations. To eliminate emittance growth when the beam propagates between plasma accelerators and traditional accelerator components, a method using longitudinally tailored plasma structures as phase space matching components is proposed. Based on the aspects above, a preliminary design study on X-ray free-electron lasers driven by plasma accelerators is presented. Lastly, an important type of numerical noise—the numerical Cherenkov instabilities in particle-in-cell codes—is systematically studied.Table of Contents Chapter 1 Introduction 1.1 Introduction 1.2 Plasma Based Acceleration 1.3 Particle-in-Cell Simulations 1.4 Motivation and Outline Chapter 2 Phase Space Dynamics of Injected Electron Beams in Ionization Injection 2.1 Introduction 2.2 The Photoionization Process 2.3 The Residual Momentum 2.3.1 Initial Momentum from the Tunneling Ionization 2.3.2 The Momentum from the Lasers: Longitudinal Injection 2.3.3 The Momentum from the Lasers: Transverse Injection 2.3.4 The Thermal Emittance 2.4 Single Particle Motion in the Nonlinear Wake 2.5 Transverse Phase Mixing 2.5.1 Emittance Evolution: Growth and Oscillation in the Injection Stage 2.5.2 Emittance Evolution: Decrease and Regrowth in the Acceleration Stage 2.5.3 A Phenomenological Model 2.5.4 Comparisons with PIC Simulations 2.6 Longitudinal Phase Mixing 2.6.1 The Trapping Condition 2.6.2 Longitudinal Phase Mixing 2.7 Space Charge Effects 2.8 The Two-Color Ionization Injection 2.8.1 The Emittance in A Single Laser Case 2.8.2 The Two-Color Ionization Injection: Longitudinal Injection 2.8.3 The Two-Color Ionization Injection: Transverse Injection 2.9 Intrinsic Phase Space Discretization in Laser Triggered Ionization Injection 2.9.1 Single Laser Pulse Case 2.9.2 Beam Driver with a Laser Injector 2.10 Summary 3.1 Introduction 3.2 The Emittance Growth between Stages 3.2.1 Emittance Growth in Free Space Drifting 3.2.2 Emittance Growth in A Uniform Focusing Field 3.3 Theoretical Analysis of A Matching Plasma 3.3.1 How to Design the Matching Plasma? 3.3.2 The Effect of the Energy Spread 3.4 Verification by PIC Simulations 3.4.1 Matching Between Two-Stage LWFAs 3.4.2 Matching in External Injection 3.4.3 Matching between LWFAs and the Quadrupoles 3.5 Summary Chapter 4 X-FELs Driven by Plasma Based Accelerators 4.1 Introduction 4.1.1 The Basic Principles of FELs< 4.1.2 The Challenges and Opportunities of X-FELs Driven by plasma Based Accelerators 4.2 X-FEL Driven by A Two-Stage LWFA 4.2.1 Simulation of the Injector Stage 4.2.2 Simulation of the Accelerator Stage 4.2.3 Simulation of the Undulator Stage 4.3 Conclusions Chapter 5 Numerical Instability due to Relativistic Plasma Drift in EM-PIC Simulations 5.1 Introduction 5.1.1 The Boosted Frame Simulations of LWFA 5.1.2 Numerical Noise Induced by Relativistic Plasma Drift in PIC Codes 5.2 Numerical Dispersion Relation for Cold Plasma Drift 5.2.1 Derivation of Dispersion Relation 5.2.2 Elements of Dispersion Relation Tensor 5.2.3 EM Modes, and Wave-Particle Resonance 5.3 Numerical Instability Induced by Relativistic Plasma Drift for the Yee Solver 5.3.1 Theoretical Analysis of the 2D Dispersion Relation 5.3.2 Simulation Study of the Instability 5.4 Asymptotic Expression for Instability Growth Rate 5.4.1 Derivation of Asymptotic Expression 5.4 2 Parameter Scans for Minimal Instability Growth Rate 5.5 Elimination of the Numerical Cerenkov Instability for Spectral EM-PIC codes 5.5.1 The NCI Modes For the Spectral Solver 5.5.2 The Positions and the Growth Rates of the NCI Modes for the Spectral Solver 5.53 LWFA Simulation in the Lorentz Boosted Frame with Spectral Solver 5.6 Conclusions Chapter 6 Summary 6.1 Concluding Remarks 6.2 Future Work Reference Acknowledgement Appendix A A.1 Derivation of the Emittance Evolution in the Acceleration Stage A.2 Interpolation Tensor and Finite Difference Operator

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Book SynopsisThis book provides for the first time an insider’s view into ITER, the biggest fusion reactor in the world, which is currently being constructed in southern France. Now in its second edition, it updates readers on all developments at ITER and those at competing fusion initiatives worldwide, at the National Ignition Facility (US), the Joint European Torus (EU) and the tens of start-ups funded by private ventures. The author also shares his personal experience with this unique big science project.Aimed at bringing the “energy of the stars” to earth, ITER is funded by the major economic powers (China, the EU, India, Japan, Korea, Russia and the USA). Often presented as a “nuclear but green” energy source, fusion could play an important role in the future electricity supply. But as delays accumulate and budgets continue to grow, ITER is currently a star partially obscured by clouds. Will ITER save humanity by providing a clean, safe and limitless source of energy, or is it merely a political showcase of cutting-edge technology? Is ITER merely an ambitious research project and partly a PR initiative driven by some politically connected scientists? In any case, ITER has already helped spur on rival projects in the USA, Canada and the UK. This book offers readers a behind-the-scenes look at this controversial project, which France snatched from Japan, and introduces them to a world of superlatives: with the largest magnets in the world, the biggest cryogenic plant and tremendous computing power, ITER is one of the most fascinating, and most international, scientific and technological endeavours of our time.Table of Contents

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Book SynopsisOn the centenary of the International Union of Geodesy and Geophysics, this book reviews the state-of-the-art research in geomagnetism, aeronomy and space weather. Written by eminent researchers from these fields, it summarises the advances in research over the past 100 years, and looks ahead to current and emerging studies on Earth''s magnetic field. It provides a comprehensive overview of the generation of Earth''s magnetic field, its history and its response to external forces. Starting at the centre of the Earth, the reader is taken on a journey from the interior core and mantle, through the upper atmosphere and magnetosphere, before reaching the Sun''s atmosphere and corona. The applications of this research are also discussed, particularly the societal impact of solar activity on critical infrastructures in our increasingly technologically dependant society. This book provides a valuable resource and reference to academic researchers and students in geomagnetism and aeronomy.Trade Review'This impressive book, published in conjunction with the 100th anniversary of the International Union of Geodesy and Geophysics (IUGG), was commissioned by the International Association of Geomagnetism and Aeronomy, one of eight constituent bodies within IUGG. The goal of the project was to provide a thorough review of current knowledge and research in the fields, considering their contribution to our understanding of the earth and inter­planetary space and the effects magnetic field variations have on our technological society. It will undoubtedly be an essential reference for researchers and advanced students in these fields for many years.' William Green, The Leading EdgeTable of ContentsPart I. Introduction: 1. Objectives of geomagnetic and aeronomy studies David Kerridge; 2. Why study the geomagnetic field? Steven Constable, Rob Van der Voo, Trond Torsvik, Harald Böhnel, Jacques Zlotnicki, Malcolm J. S. Johnston, Yoichi Sasai, Jean-Louis LeMouёl, Mangalathayil Ali Abdu, David Boteler and Jean-Pierre Valet; 3. Major scientific contributions of the International Association of Geomagnetism and Aeronomy (IAGA) during the past 100 years Ed Cliver and Eduard Petrovsky; Part II. Geomagnetic Field: Sources and Observations: 4. Geomagnetic field sources – from Earth's core to the sun Daniel Baker; 5. Can paleomagnetism distinguish dynamo regimes? Stuart Gilder and Florian Lhuillier; 6. Geomagnetic and electromagnetic observations at ground level Arnaud Chulliat, Ute Weckmann, Oliver Ritter, Stuart Gilder, Michael Wack, Elena Kronberg and Ameya Prabhu; 7. Modelling internal and external geomagnetic fields using satellite data Ingo Wardinski and Erwan Thébault; 8. New insights in far space measurements: large-scale structures and processes in the solar wind and terrestrial magnetosphere Aurelie Marchaudon; Part III. Spatial and Temporal Variations of the Geomagnetic Field: 9. Insights from forward and inverse core field models Nicolas Gillet; 10. The global lithospheric magnetic field: world magnetic anomaly maps and models Vincent Lesur and Erwan Thébault; 11. The ionospheric field Robert Strangeway, Nanan Balan, Robert Clauer and Yusuke Ebihara; 12. The magnetosphere Stephen Fuselier, Robert McPherron, Daniel Baker, Craig Kletzing, Craig Kletzing and Viviane Pierrand; 13. Temporal field variations Catherine Constable, Ian Mann, Louis G. Ozeke, Alex Degeling, Kyle R. Murphy, Robert Rankin and Colin Waters; Part IV. Space Weather: 14. Physical processes of space weather Bogdan Hnat and Robert McPherron; 15. Space weather effects in the ionosphere, thermosphere and at Earth's surface Ian Mann, Hermann Lühr and Ari Viljanen; 16. Technological impacts of space weather Michael Hapgood; Part V. Magnetic Fields Beyond the Earth and Beyond Today: 17. Magnetic field evolution in terrestrial bodies from planetesimals to exoplanets Doris Breuer; 18. Solar variability: causes, current understanding, prospects for the future Andre Balogh; 19. Long and short geomagnetic prediction Weijia Kuang, Andrew Tangborn, Terence Sabaka and Robert Tyler; Index.

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Book SynopsisPlasma is one of the four fundamental states of matter; the other three being solid, liquid and gas. Several components, such as molecular clouds, diffuse interstellar gas, the solar atmosphere, the Earth''s ionosphere and laboratory plasmas, including fusion plasmas, constitute the partially ionized plasmas. This book discusses different aspects of partially ionized plasmas including multi-fluid description, equilibrium and types of waves. The discussion goes on to cover the reionization phase of the universe, along with a brief description of high discharge plasmas, tokomak plasmas and laser plasmas. Various elastic and inelastic collisions amongst the three particle species are also presented. In addition, the author demonstrates the novelty of partially ionized plasmas using many examples; for instance, in partially ionized plasma the magnetic induction is subjected to the ambipolar diffusion and the Hall effect, as well as the usual resistive dissipation. Also included is an obserTrade Review'Professor Krishan is to be congratulated for such a mathematically detailed presentation of her material, which allows the reader to follow the developments step by step. Make no mistake, this is a challenging book, but it is also an extremely rewarding one for anyone who wants to acquire a thorough grounding in the theory of partially ionized plasmas.' Terry Robinson, The ObservatoryTable of ContentsFigures; Preface; 1. Partially ionized plasmas here and everywhere; 2. Multifluid description of partially ionized plasmas; 3. Equilibrium of partially ionized plasmas; 4. Waves in partially ionized plasmas; 5. Advanced topics in partially ionized plasmas; 6. Research problems in partially ionized plasmas; Supplementary matter; Index.

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Book SynopsisWith ninety per cent of visible matter in the universe existing in the plasma state, an understanding of magnetohydrodynamics is essential for anyone looking to understand solar and astrophysical processes, from stars to accretion discs and galaxies; as well as laboratory applications focused on harnessing controlled fusion energy. This introduction to magnetohydrodynamics brings together the theory of plasma behavior with advanced topics including the applications of plasma physics to thermonuclear fusion and plasma- astrophysics. Topics covered include streaming and toroidal plasmas, nonlinear dynamics, modern computational techniques, incompressible plasma turbulence and extreme transonic and relativistic plasma flows. The numerical techniques needed to apply magnetohydrodynamics are explained, allowing the reader to move from theory to application and exploit the latest algorithmic advances. Bringing together two previous volumes: Principles of Magnetohydrodynamics and Advanced MagTable of ContentsPreface; Part I. Plasma Physics Preliminaries: 1. Introduction; 2. Elements of plasma physics; 3. 'Derivation' of the macroscopic equations; Part II. Basic Magnetohydrodynamics: 4. The MHD model; 5. Waves and characteristics; 6. Spectral theory; Part III. Standard Model Applications: 7. Waves and instabilities of inhomogeneous plasmas; 8. Magnetic structures and dynamics of the solar system; 9. Cylindrical plasmas; 10. Initial value problem and wave damping; 11. Resonant absorption and wave heating; Part IV. Flow and Dissipation: 12. Waves and instabilities of stationary plasmas; 13. Shear flow and rotation; 14. Resistive plasma dynamics; 15. Computational linear MHD; Part V. Toroidal Geometry: 16. Static equilibrium of toroidal plasmas; 17. Linear dynamics of static toroidal plasmas; 18. Linear dynamics of toroidal plasmas with flow; Part VI. Nonlinear Dynamics: 19. Turbulence in incompressible magneto-fluids; 20. Computational nonlinear MHD; 21. Transonic MHD flows and shocks; 22. Ideal MHD in special relativity; Appendices: A. Vectors and coordinates; B. Tables of physical quantities; References; Index.

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Book SynopsisAn up-to-date comprehensive text useful for graduate students and academic researchers in the field of energy transfers in fluid flows. The initial part of the text covers discussion on energy transfer formalism in hydrodynamics and the latter part covers applications including passive scalar, buoyancy driven flows, magnetohydrodynamic (MHD), dynamo, rotating flows and compressible flows. Energy transfers among large-scale modes play a critical role in nonlinear instabilities and pattern formation and is discussed comprehensively in the chapter on buoyancy-driven flows. It derives formulae to compute Kolmogorov's energy flux, shell-to-shell energy transfers and locality. The book discusses the concept of energy transfer formalism which helps in calculating anisotropic turbulence.Trade Review'This book is an outcome of the author's life-long obsession with the mechanism of energy transfers in turbulent flows.' Jayant Bhattacharjee, Indian Association for the Cultivation of Science'Nicely organized in parts devoted to increasingly complex flows, it is a perfect book to explore the theoretical description of Navier-Stokes turbulence as well as flows with scalars, vectors and more exotic systems.' Daniele Carati, Université Libre de Bruxelles'This comprehensive book discusses an impressive array of applications from a unified point of view.' Arnab Rai Choudhuri, Indian Institute of Science'The monograph will be an invaluable resource to students and researchers interested in the application of energy transfer theory to fluids and magnetofluids.' Melvyn Goldstein, NASA'This book is an outstanding achievement whose many examples and illustrations make the reading as fluid as the subject matter.' Franck Plunian, Université Grenoble Alpes'It is a self-contained monograph which will certainly be of direct use to a large audience, from graduate students to scholars and researchers.' Annick Pouquet, University of Colorado, Boulder'This book, addressed to graduate students and researchers, covers vast areas of fluid dynamics and presents each domain in a precise manner.' Maurice Rossi, Université Pierre et Marie Curie, Paris'This monograph clearly articulates the multiscale energy transfer perspectives for turbulent flows, advanced prominently by the author and his co-workers.' K. R. Sreenivasan, New York University'This impressive monograph will serve as a highly valuable reference to researchers in turbulence and other fields for many years to come.' P. K. Yeung, Georgia Institute of TechnologyTable of ContentsPreface; Acknowledgement; Dedication; Part I: 1. Introduction; 2. Basics of Hydrodynamics; 3. Fourier space description of hydrodynamics; 4. Energy transfers in hydrodynamic flows; 5. Energy spectrum and flux of 3D hydrodynamics; 6. Enstrophy transfers in hydrodynamics; 7. Two-dimensional turbulence; 8. Helical turbulence; 9. Craya-Herring and helical basis; 10. Field-theoretic treatment of energy transfers; 11. Energy transfers in anisotropic flows'; 12. Energy transfers in real space; Part II: 13. Energy transfers in passive scalar; 14. Stably stratified turbulence; 15. Thermal convection; 16. Rotating turbulence; 17. Magnetohydrodynamic turbulence: Formalism; 18. Magnetohydrodynamic turbulence: applications; 19. Magnetic Field Generation in MHD; 20. Energy transfers in compressible turbulence; 21. Shell modes of turbulence; 22. Miscellaneous applications of energy transfers; Appendix A. Power lay physics; Appendix B. Money or wealth transfers in economy; Appendix C. Renormalization group analysis of hydrodynamic turbulence; Notes; References; Subject Index.

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Book SynopsisThe field of high-power laser-plasma interaction has grown in the last few decades, with applications ranging from laser-driven fusion and laser acceleration of charged particles to laser ablation of materials. This comprehensive text covers fundamental concepts including electromagnetics and electrostatic waves, parameter instabilities, laser driven fusion,charged particle acceleration and gamma rays. Two important techniques of laser proton interactions including target normal sheath acceleration (TNSA) and radiation pressure acceleration (RPA) are discussed in detail, along with their applications in the field of medicine. An analytical framework is developed for laser beat-wave and wakefield excitation of plasma waves and subsequent acceleration of electrons. The book covers parametric oscillator model and studies the coupling of laser light with collective modes.Table of ContentsPreface; Acknowledgement; Dedication; 1. Introduction; 2. Linear waves; 3. Resonance absorption and Brunel absorption; 4. Plasmonics: surface plasma wave and its coupling to laser; 5. Motion in large amplitude EM wave: ponderomotive force and self-generated magnetic field; 6. Laser electron acceleration; 7. Laser acceleration of ions; 8. Coherent radiation generation; 9. Self -focusing and filamentation; 10. Parametric instabilities in homogeneous plasma; 11. Parametric instabilities in inhomogeneous plasma; 12. Nonlinear Schrodinger equation; 13. Vlasov and particle in cell simulations; 14. Quantum electrodynamic effects in plasma; Reference; Index.

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Book SynopsisPhysics of Ionized Gases

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Book SynopsisAdvances in Plasma Physics Research

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Book SynopsisAdvances in Plasma Physics Research

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Book Synopsis

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Book SynopsisAdvances in Plasma Physics Research

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Book SynopsisThis book presents state-of-the-art analysis of developments in plasma physics.

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Book SynopsisThis series includes within its scope equilibria, linear waves, and instabilities; nonlinear behaviour, including turbulent and stochastic phenomena and associated transport, and solitons and shock waves. It also includes plasma physics of lasers and particle beams and charged-particle acceleration and transport as well as radiation generation, transport, propagation, and interaction with plasmas. Low-temperature plasmas, including sources. plasma chemistry and processing and covered as are geophysical, planetary, solar, and astrophysical plasmas and plasma confinement by magnetic fields. Inertial confinement physics, the physics of dense plasmas or matter under extreme conditions and dusty plasmas are further subsumed. This volumes includes the latest research from around the globe.

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Book SynopsisThis monograph contains all aspects of plasma physics for plasma confinement in stellarator and heliotron devices. Present achievements and prospects for next generation devices are included.Trade ReviewFor the laboratory plasma physicist, for whom it is written, this volume will surely be of great value...It is also salutory to be reminded just how sophisticated fusion research as become, driven by the combination of theory and experiment. * Leon Mestel, The Observatory Magazine, Feb 1999 *Table of Contents1. Introduction ; 2. Design Principles of Coil Systems in Stellarator and Heliotron Devices ; 3. Description of Magnetically Confined Plasmas ; 4. MHD Equillibrium of Toroidal Plasma in Three-Dimensional Geometry ; 5. MHD Instabilites in Heliotrons ; 6. Particle Orbit in Heliotrons ; 7. Neoclassical Transport in Stellarator/Heliotron ; 8. Heating and Confinement of Heliotron Plasmas ; 9. Steady State Fusion Reactor

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Book SynopsisThis is a coherent and updated comprehensive treatise on the field of atomic physics in hot plasmas, which can be used both for tutorial and professional purposes, and which summarizes the central subjects in the field today.Table of Contents1. Modeling of the ionic potential ; 2. Ionic properties in hot plasmas ; 3. Ionic properties and processes in hot plasmas ; 4. The charge and excited state distributions in hot plasmas ; 5. The emission spectrum and its components ; 6. Spectral line broadening ; 7. The emission spectrum as a means of plasma diagnostics ; 8. Radiation absorbing processes and radiation transport ; 9. Applications

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Book SynopsisDeals with the propagation and absorption of high frequency waves in plasmas (hot fully ionized gases), a subject on which work is very active in controlled fusion research and in astrophysics. This book could therefore be useful as a source for courses on electromagnetism or classical kinetic theory at a medium to advanced level.Trade ReviewThis well organised text on hot plasma theory is written for fusion physicists researching high frequency heating and current drive.Table of ContentsPreface ; Index ; Introduction ; 1. Plasma Electrodynamics ; 2. Elementary plasma kinetic theory ; 3. The hot plasma dielectric tensor ; 4. Waves in cold plasma ; 5. Waves in hot plasma ; 6. The electrostatic and fluid approximations ; 7. Linear wave-particle interactions ; 8. Collisionless stochacity ; 9. Quasilinear theory and current drive ; 10. Nonlinear effects associated with H.F. Heating

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Book SynopsisGives a physical treatment of the kinetic theory of gases and magnetoplasmas, using mean-free-path arguments when possible and identifying problem areas where received theory has either failed or fallen short of expectations. L.C. Woods has also written "The Thermodynamics of Fluid Systems".Trade Reviewthe book presents a treatment of the kinetic theory of gases and magnetoplasmas in such a way that it covers the standard material in a way as simple as possible .,.. The book seems to radiate a deep conviction - which is appreciated by the reviewer - that the development of the kinetic theory needs not only calculational skills and computational magic in evaluating the content of the theory in model arrangements, but equally, if not in excess, deep insight into the physical processes. * I. Abonyi, Besprechungsbelege, February 1994 *Table of Contents1. Basic concepts ; 2. The Maxwellian velocity distribution ; 3. Elementary kinetic theory ; 4. Particle diffusion ; 5. Intermediate kinetic theory ; 6. Advanced kinetic theory ; 7. Boltzmann's kinetic equation ; 8. Second-order kinetic theory ; 9. Dynamics of charged particles ; 10. Kinetic theory for magnetoplasmas ; 11. Transport across strong magnetic fields ; Appendix ; References ; Index

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a huge range and FREE tracked UK delivery on ALL orders.

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Book Synopsis1. Introduction.- 2. Charged Particle Motion in Constant and Uniform Electromagnetic Fields.- 3. Charged Particle Motion in Nonuniform Magnetostatic Fields.- 4. Charged Particle Motion in Time-Varying Electromagnetic Fields.- 5. Elements of Plasma Kinetic Theory.- 6. Average Values and Macroscopic Variables.- 7. The Equilibrium State.- 8. Macroscopic Transport Equations.- 9. Macroscopic Equations for a Conducting Fluid.- 10. Plasma Conductivity and Diffusion.- 11. Some Basic Plasma Phenomena.- 12. Simple Applications of Magnetohydrodynamics.- 13. The Pinch Effect.- 14. Electromagnetic Waves in Free Space.- 15. Magnetohydrodynamic Waves.- 16. Waves in Cold Plasmas.- 17. Waves in Warm Plasmas.- 18. Waves in Hot Isotropic Plasmas.- 19. Waves in Hot Magnetized Plasmas.- 20. Particle Interactions in Plasmas.- 21. The Boltzmann and the Fokker-Planck Equations.- 22. Transport Processes in Plasmas.- Appendix A Useful Vector Relations.- Appendix B Useful Relations in Cartesian and in CurvilineaTrade ReviewFrom the reviews of the third edition: "This is an excellent introductory textbook of plasma physics, especially recommendable to those starting the study of the subject. … the book is an immense monography of 678 pages. Our impressions are good … ." (Iván Abonyi, Zentralblatt MATH, Vol. 1084, 2006)Table of ContentsCONTENTS 1. General Properties of Plasmas 1.1 Definition of a Plasma 1.2 Plasma as the Fourth State of Matter 1.3 Plasma Production 1.4 Particle Interactions and Collective Effects 1.5 Some Basic Plasma Phenomena 2. Criteria for the De.nition of a Plasma 2.1 Macroscopic Neutrality 2.2 Debye Shielding 2.3 The Plasma Frequency 3. The Occurrence of Plasmas in Nature 3.1 The Sun and its Atmosphere 3.2 The Solar Wind 3.3 The Magnetosphere and the Van Allen Radiation Belts 3.4 The Ionosphere 3.5 Plasmas Beyond the Solar System 4. Applications of Plasma Physics 4.1 Controlled Thermonuclear Fusion 4.2 The Magnetohydrodynamic Generator 4.3 Plasma Propulsion 4.4 Other Plasma Devices 5. Theoretical Description of Plasma Phenomena 5.1 General Considerations on a Self-Consistent Formulation 5.2 Theoretical Approaches Problems 1. Introduction 2. Energy Conservation 3. Uniform Electrostatic Field 4. Uniform Magnetostatic Field 4.1 Formal Solution of the Equation of Motion 4.2 Solution in Cartesian Coordinates 4.3 Magnetic Moment 4.4 Magnetization Current 5. Uniform Electrostatic and Magnetostatic Fields 5.1 Formal Solution of the Equation of Motion 5.2 Solution in Cartesian Coordinates 6. Drift Due to an External Force Problems 1. Introduction 2. Spatial Variation of the Magnetic Field 2.1 Divergence Terms 2.2 Gradient and Curvature Terms 2.3 Shear Terms 3. Equation of Motion in the First Order Approximation 4. Average Force Over One Gyration Period 4.1 Parallel Force 4.2 Perpendicular Force 4.3 Total Average Force 5. Gradient Drift 6. Parallel Acceleration of the Guiding Center 6.1 Invariance of the Orbital Magnetic Moment and of the Magnetic Flux 6.2 Magnetic Mirror Effect 6.3 The Longitudinal Adiabatic Invariant 7. Curvature Drift 8. Combined Gradient-Curvature Drift Problems 1. Introduction 2. Slowly Time-Varying Electric Field 2.1 Equation of Motion and Polarization Drift 2.2 Plasma Dielectric Constant 3. Electric Field with Arbitrary Time Variation 3.1 Solution of the Equation of Motion 3.2 Physical Interpretation 3.3 Mobility Dyad 3.4 Plasma Conductivity Dyad 3.5 Cyclotron Resonance 4. Time-Varying Magnetic Field and Space-Varying Electric Field 4.1 Equation of Motion and Adiabatic Invariants 4.2 Magnetic Heating of a Plasma 5. Summary of Guiding Center Drifts and Current Densities 5.1 Guiding Center Drifts 5.2 Current Densities Problems 1. Introduction 2. Phase Space 2.1 Single-Particle Phase Space 2.2 Many-Particle Phase Space 2.3 Volume Elements 3. Distribution Function 4. Number Density and Average Velocity 5. The Boltzmann Equation 5.1 Colisionless Boltzmann Equation 5.2 Jacobian of the Transformation in Phase Space 5.3 E.ects of Particle Interactions 6. Relaxation Model for the Collision Term 7. The Vlasov Equation Problems 1. Average Value of a Physical Quantity 2. Average Velocity and Peculiar Velocity 3. Flux 4. Particle Current Density 5. Momentum Flow Dyad or Tensor 6. Pressure Dyad or Tensor 6.1 Concept of Pressure 6.2 Force per Unit Area 6.3 Force per Unit Volume 6.4 Scalar Pressure and Absolute Temperature 7. Heat Flow Vector 8. Heat Flow Triad 9. Total Energy Flux Triad 10. Higher Moments of the Distribution Function Problems 1. The Equilibrium State Distribution Function 1.1 The General Principle of Detailed Balance and Binary Collisions 1.2 Summation Invariants 1.3 Maxwell-Boltzmann Distribution Function 1.4 Determination of the Constant Coe.cients 1.5 Local Maxwell-Boltzmann Distribution Function 2. The Most Probable Distribution 3. M

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Book Synopsis1. Introduction.- 2. Single-Particle Motions.- 3. Plasmas as Fluids.- 4. Waves in Plasmas.- 5. Diffusion and Resistivity.- 6. Equilibrium and Stability.- 7. Kinetic Theory.- 8. Nonlinear Effects.- Appendices.- Appendix A. Units, Constants and Formulas, Vector Relations.- Appendix B. Theory of Waves in a Cold Uniform Plasma.- Appendix C. Sample Three-Hour Final Exam.- Appendix D. Answers to Some Problems.- Index to Problems.Table of Contents1. Introduction.- 2. Single-Particle Motions.- 3. Plasmas as Fluids.- 4. Waves in Plasmas.- 5. Diffusion and Resistivity.- 6. Equilibrium and Stability.- 7. Kinetic Theory.- 8. Nonlinear Effects.- Appendices.- Appendix A. Units, Constants and Formulas, Vector Relations.- Appendix B. Theory of Waves in a Cold Uniform Plasma.- Appendix C. Sample Three-Hour Final Exam.- Appendix D. Answers to Some Problems.- Index to Problems.

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Book SynopsisThis energy source is inexhaustible and, although achieving fusion energy is difficult, the progress made in the past two decades has been remarkable.Trade ReviewFrom the reviews:“The ‘indispensable truth’ is that Chen … has written what may well be recognized as the definitive retrospective on the promise of endless supplies of cheap, clean nuclear energy from fusion, offering the prospect of realizing the promise at last. … It is stylishly written, designed, and illustrated to appeal to general readers … . Chen is in his comfort zone as he tells his story, and the indispensable truth is that it is just that–indispensable! Summing Up: Highly recommended. All levels/libraries.”­­­ (L. W. Fine, Choice, Vol. 49 (3), November 2011)"With An Indispensable Truth: How Fusion Power Can Save the Planet, Frank Chen has provided a sweeping perspective on fusion energy. He covers everything from climage change to plasma instabilities. On climate change and energy, the view is best from 30 000 feet: The book provides a good high-level overview of the issues at stake...On fusion plasma physics, Chen's area of expertise, An Indispensable Truth provides an intuitive, up-close explanation of exciting recent advances and future challenges...An Indispensable Truth provides an exciting whirlwind tour of energy issues and technologies, with particular insight into fusion. Chen is correct to emphasize the tremendous progress that has been made in fusion research. ITER will produce hundreds of millions of watts of thermal energy from fusion, for periods of up to an hours. However, it remains for the world, and in particular the US, to decide if we will develop fusion into a practical energy source. We will need it." (Physics Today, Volume 65, Issue 2, February 2012)Table of ContentsPreface.- Prologue.- The Evidence for Climate Change.- The Future of Energy I: Fossil Fuels.- The Future of Energy II: Renewable Energy.- Fusion: Energy from the Seawater.- Perfecting the Magnetic Bottle.- The Remarkable Tokamak.- Evolution and Physics of the Tokamak.- A Half-century of Progress.- Engineering: The Big Challenge.- Fusion Concepts for the Future.- Conclusions.- Epilogue.

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Book SynopsisThis open access book serves as a concise primer introducing the non-specialist reader to the physics of solar energetic particles (SEP). It systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. This second edition contains two completely new chapters discussing element abundances and shock waves, reflecting new theoretical, modeling, and observational results. Existing chapters have been substantially expanded or updated with additions placed in a broader context.More specifically, the author discusses the timing of the onsets of SEPs, their longitude distributions, their high-energy spectral shapes, their correlations with other solar phenomena, as well as the all-important elemental and isotopic abundances. The book relates impulsive SEP events to magnetic reconnection in solar flares and jets. The concept of shock acceleration by scattering on self-amplified Alfvén waves is introduced, as is the evidence of reacceleration of impulsive-SEP material in the seed population accessed by the shocks in gradual events. The text then develops processes of transport of ions out to an observer. Finally, a technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated.The author also mentions the role of SEP events as a radiation hazard in space and briefly discusses the nature of the main particle telescope designs that have contributed to most of the SEP measurements.Trade Review“Donald V. Reames presents a clear contemporary account of observational and theoretical studies of the principal families of solar energetic particles (SEPs) … . A delightful sense that this lively presentation is drawn from Reames’ decades of experimental investigations of SEPs pervades the book. … This excellent primer by Reames is a thorough account of SEP events with parallel discussions of the solar wind. It deserves to be read by stellar astronomers.” (David L. Lambert, The Observatory, Vol. 142 (1287), April, 2022)Table of Contents

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Book SynopsisThis book introduces the traditional and novel techniques required to study the thermodynamic and transport properties of quark–gluon plasma. In particular, it reviews the construction of improved holographic models for QCD-like confining gauge theories and their applications in the physics of quark–gluon plasma. It also discusses the recent advances in the development of hydrodynamic techniques, especially those incorporating the effects of external magnetic fields on transport. The book is primarily intended for researchers and graduate students with a background in quantum field theory and particle physics but who may not be familiar with the theory of strong interactions and holographic and hydrodynamic techniques required to study said interactions.Table of ContentsIntroduction: AdS/CFT and heavy ion collisions.- Holographic QCD theories.- Improved holographic QCD - construction of the theory.- Thermodynamics and the confinement/deconfinement transition.- Flavor sector.- Hydrodynamics and transport coefficients.- Hard probes.- ihQCD at finite B.- Conclusion and a look ahead.

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Book SynopsisConstant and crossing-cubic vector fields.- Crossing-linear and crossing-cubic vector fields.- Crossing-quadratic and crossing-cubic Vector Field.- Two crossing-cubic vector fields.

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Book SynopsisScattering by One Electron.- Scattering by Many Electrons.- Dressed Particles.- The Fluctuation-Dissipation Theorem.- Transition to Turbulence.- Conclusions.

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Book SynopsisChapter 1. Introduction.- Chapter 2. Ion and Plasma Sources: Basic Science & Recent Trends.- Chapter 3. ION AND PLASMA DIAGNOSTICS.- Chapter 4. High Brightness, Low Energy Spread Ions for Fine Focused Beams and Applications.- Chapter 5. Ion and Plasma Interaction with Materials.- Chapter 6. Plasmas for the production of value-added chemicals.- Chapter 7. Reevaluating the Role of Water in Plasma-Assisted Nitrogen Fixation.- Chapter 8. Applications of the Heavy Ion Microbeam Technology for the Life Sciences Research.- Chapter 9. Plasma-assisted Hydrogel Synthesis.- Chapter 10. Plasma Chemistry and Applications of Atmospheric Pressure Transient Electrical Discharges.- Chapter 11. Spray Generated Ions: Principles, Processes, Pathways for Applications.- Chapter 12. Machine Learning: Basic Methodologies, Structures and Application Examples.- Chapter 13. Mathematical Foundation for Quantum Computing of Electromagnetic Wave Propagation in Dielectric Media.

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Book SynopsisIntroduction.- Basic Tools of Laser Plasma Physics.- Nonlinear Laser Plasma Optics.- Electron Acceleration.- Ion Acceleration.- An Outlook in the Quantum Regime.

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Book SynopsisThe 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 title 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 are 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. Specifically the book has been designed to enable academics in physics, astrophysics, applied physics and engineering departments to provide in a single-course, an introduction to fluid mechanics and radiative transfer, with dramatic applications in the field of high-energy-density systems. This second edition includes pedagogic improvements to the presentation throughout and additional material on equations of state, heat waves, and ionization fronts, as well as problem sets accompanied by solutions.Table of ContentsIntroduction to High-Energy-Density Physics.- Descriptions of Fluids and Plasmas.- Properties of High-Energy-Density Plasmas.- Shocks and Rarefactions.- Hydrodynamic Instabilities.- Radiative Transfer.- Radiation Hydrodynamics.- Creating High-Energy-Density Conditions.- Inertial Confinement Fusion.- Experimental Astrophysics.- Relativistic High-Energy-Density Systems.- Appendix A: Constants, Acronyms, and Standard Variables.- Appendix B: Sample Mathematica Code.- Appendix C: List of the Homework Problems and Solutions to Selected Problems.

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