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Stroth U: Plasmaphysik

Plasmaphysik

Phänomene, Grundlagen und Anwendungen

This text introduces readers to magnetohydrodynamics (MHD), the physics of ionised fluids. Traditionally MHD is taught as part of a graduate curriculum in plasma physics. By contrast, this text - one of a very few - teaches MHD exclusively from a fluid dynamics perspective, making it uniquely accessible to senior undergraduate students. Part I of the text uses the MHD Riemann problem as a focus to introduce the fundamentals of MHD: Alfvén's theorem; waves; shocks; rarefaction fans; etc. Part II builds upon this with presentations of broader areas of MHD: fluid instabilities; viscid hydrodynamics; steady-state MHD; and non-ideal MHD. Throughout the text, more than 125 problems and several projects (with solutions available to instructors) reinforce the main ideas. Optionally, large-font lesson plans for a 'flipped-style' class are also available to instructors. This book is suitable for advanced undergraduate and beginning graduate students, requiring no previous knowledge of fluid dynamics or plasma physics.

A First Course in Magnetohydrodynamics

Wer kennt das nicht: Für ein besonderes Gericht der asiatischen Küche eine Spezialzutat gekauft, die nun im Schrank steht. Früher stand sie dort so lange, bis man auch mit den besten Zugeständnissen an das MHD sie nicht mehr zum Kochen verwenden konnte und dies nicht nur, weil z.B. das Aroma komplett verflogen war - und diese wundervolle Zutat dann den Weg alles Irdischen ging. Doch das ist nicht nur in Zeiten nachhaltigen Kochens nun überhaupt keine Option. 60 überraschende und im besten Sinne Crossover-Rezepte zeigen, was man aus diesen leckeren südostasiatischen Zutaten noch alternativ alles zaubern kann. Eine übersichtliche Warenkunde hilft zudem, sich in dem Zutatenangebot der spannenden Asia-Shops zurechtzufinden und mutig zu sein, auch einmal etwas Neues oder Exotisches auszuprobieren.

Wer kennt das nicht: Für ein besonderes Gericht der asiatischen Küche eine Spezialzutat gekauft, die nun im Schrank steht. Früher stand sie dort so lange, bis man auch mit den besten Zugeständnissen an das MHD sie nicht mehr zum Kochen verwenden konnte und dies nicht nur, weil z.B. das Aroma komplett verflogen war – und diese wundervolle Zutat dann den Weg alles Irdischen ging. Doch das ist nicht nur in Zeiten nachhaltigen Kochens nun überhaupt keine Option. 60 überraschende und im besten Sinne Crossover-Rezepte zeigen, was man aus diesen leckeren südostasiatischen Zutaten noch alternativ alles zaubern kann. Eine übersichtliche Warenkunde hilft zudem, sich in dem Zutatenangebot der spannenden Asia-Shops zurechtzufinden und mutig zu sein, auch einmal etwas Neues oder Exotisches auszuprobieren.

Asiatische Zutaten neu entdecken

Shop Suey

The second edition of Applied Mechanics of Solids provides a concise description of all the concepts needed to predict how solid materials deform and fail under stress. With its companion volume of solved example problems, it is an invaluable class textbook or reference for personal study or review.

Applied Mechanics of Solids

This comprehensive volume &nbsp;navigates through the complexities of Earth's ionosphere and its intricate relationship with GNSS spread-spectrum signals. The book delineates the nuanced structures and dynamics of Earth's atmosphere, offering profound insights into signal propagation, including a meticulous analysis of various ionospheric models.

&nbsp;

Delving into the instruments of choice, it encapsulates the facets of the GNSS space segment, its theoretical background, and practical applications. The ground and user segments discussed provide readers with a deep understanding of satellite dynamics and navigation data.

&nbsp;

Further chapters explore the intricacies of GNSS Software Defined Radio (SDR), offering a detailed examination of signal acquisition and tracking, and presenting innovative approaches to baseband data application without data decoding. A significant portion is devoted to manufacturing front-end hardware, providing guidance from specifications to testing, enabling readers to navigate the world of hardware design with ease.

&nbsp;

Lastly, the book ventures into the applications of GNSS receivers for ionospheric study, highlighting the construction of advanced observables and their practical applications in navigation processors. This section also elucidates the role of multi-station observables in extracting critical ionospheric information.

&nbsp;

A pivotal resource for researchers and professionals alike, this book stands as a testament to comprehensive research and innovation in the field of GNSS and SDR, fostering a deeper understanding of the Earth's ionosphere.

&nbsp;

This book serves as a natural progression from Dr.Petrocski's prior contributions, offering readers actionable insights grounded in theoretical understanding.

Specialized Software-Defined Radio for In-Depth Ionospheric Research

The Ionosphere with GNSS SDR

Chemical Industries

The third edition of Bubbles, Drops, and Particles in Non-Newtonian Fluids provides comprehensive coverage of the scientific foundations and latest advances in particle motion in non-Newtonian media.

The third edition of Bubbles, Drops, and Particles in Non-Newtonian Fluids provides comprehensive coverage of the scientific foundations and latest advances in particle motion in non-Newtonian media.

Bubbles, Drops, and Particles in Non-Newtonian Fluids

Embarking on a journey into the realm of quantum mechanics can be a daunting task for anyone. Its puzzling mathematics and bewildering predictions often leave individuals feeling confused and disheartened. But what if there was a different approach-one aimed to cultivate an understanding of quantum mechanics from its very foundations?

Inception or Conception? A Classical Preamble to Quantum Mechanics

Quantum Mechanics

This book introduces the physics of stars. It covers observational methods, star formation, and the life cycles of stars. In this book, you will find a comprehensive overview of the physical properties of stars. The current state of knowledge regarding star structure and evolution is summarized here, and a glimpse into exciting, open questions in astrophysics is offered.

Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.

The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.

Mathias Scholz&nbsp;is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986. &lt;  ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.   ed from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.

Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it. 
The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future. Mathias Scholz&nbsp;is hobby astronomer. He&nbsp;studied physics at the University of Rostock from 1981 to 1986.Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it. 
The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.

Structure, Evolution and Properties

The Physics of Stars

This book delves into the analysis and application of the dimensions, units, and unit conversions in engineering practical use. It demonstrates the importance of dimensional homogeneity and unit consistency and presents detailed portrayals of various unit systems in both the English system and the SI system.

This book delves into the analysis and application of the dimensions, units, and unit conversions in engineering practical use. It demonstrates the importance of dimensional homogeneity and unit consistency and presents detailed portrayals of various unit systems in both the English system and the SI system.

Engineering Dimensions, Units, and Conversions

Proceedings of the International Astronomical Union Symposia and Colloquia

Impressive events of magnetic energy release, such as solar and stellar flares and coronal mass ejections, take place in the atmospheric layers above a star's photosphere. These magnetic-activity events are closely related to the dynamics of subsurface convection zones inside the star. IAU Symposium 365 was devoted to observational and theoretical aspects of solar and stellar hydrodynamics and magnetohydrodynamics, both global and local, including numerical studies. The last few decades have been marked by substantial progress in our understanding of the physics of internal and external processes in the Sun and solar-type stars, but the scientific communities making this progress have not traditionally worked closely together. This symposium, delayed due to the COVID pandemic, brought together specialists in the physics of convection zones and atmospheres, to stimulate the emergence of new ideas and to develop new techniques in this dynamic field of active research.

Dynamics of Solar and Stellar Convection Zones and Atmospheres (IAU S365)

Classical Dynamics of Linear and Nonlinear Systems

Springer Aerospace Technology

Proceedings of the 33rd International Symposium

Rarefied Gas Dynamics

Springer Proceedings in Physics

This book presents articles from the 5th Chinese Conference on High Voltage and Discharge Plasmas, held in Xi'an, China by the Special Committee on Plasma and Its Applications of the Chinese Electrotechnical Society from November 29 to December 1, 2024. It facilitates the exchange and sharing of the latest research advances and major outcomes in the fields of high voltage technology, pulsed power, plasma, and related applications over the past two years. It is dedicated to enhancing academic exchanges between various disciplines, promoting interdisciplinary integration, and thereby advancing the development and technological progress in high voltage and discharge plasma technology sectors.&nbsp;

This book presents articles from the 5th Chinese Conference on High Voltage and Discharge Plasmas, held in Xi'an, China by the Special Committee on Plasma and Its Applications of the Chinese Electrotechnical Society from November 29 to December 1, 2024. It facilitates the exchange and sharing of the latest research advances and major outcomes in the fields of high voltage technology, pulsed power, plasma, and related applications over the past two years. It is dedicated to enhancing academic exchanges between various disciplines, promoting interdisciplinary integration, and thereby advancing the development and technological progress in high voltage and discharge plasma technology sectors.

HVDP 2024, 29 Nov-1 Dec, Xi'an, China

Proceedings of the 5th Chinese Conference on High Voltage and Discharge Plasmas

Plasmaphysik

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