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  • 1
    Online Resource
    Online Resource
    Dordrecht : Springer Netherlands
    UID:
    b3kat_BV042410826
    Format: 1 Online-Ressource (XVII, 309 p)
    Edition: Second Edition
    ISBN: 9780306477195 , 9781402006951
    Series Statement: Astrophysics and Space Science Library 279
    Note: This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena – such as one period of a high-frequency wave – or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star
    Language: English
    Keywords: Sonnenkorona ; Plasmaphysik ; Sternkorona ; Plasmaphysik
    Library Location Call Number Volume/Issue/Year Availability
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  • 2
    UID:
    almahu_9949199294502882
    Format: XVII, 309 p. 45 illus. , online resource.
    Edition: 2nd ed. 2002.
    ISBN: 9780306477195
    Series Statement: Astrophysics and Space Science Library, 279
    Content: This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena - such as one period of a high-frequency wave - or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star.
    Note: Basic Concepts -- Magnetohydrodynamics -- Waves in a Cold, Collisionless Plasma -- Kinetic Plasma and Particle Beams -- Astrophysical Electron Beams -- Ion Beams and Electromagnetic Instabilities -- Electrons Trapped in Magnetic Fields -- Electric Currents -- Collisionless Shock Waves -- Propagation of Radiation.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9789401750882
    Additional Edition: Printed edition: ISBN 9781402006951
    Additional Edition: Printed edition: ISBN 9789400739604
    Additional Edition: Printed edition: ISBN 9789400739246
    Language: English
    Library Location Call Number Volume/Issue/Year Availability
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  • 3
    UID:
    b3kat_BV014639893
    Format: XVII, 301 S. , Ill., graph. Darst.
    Edition: 2. ed.
    ISBN: 1402006950 , 9781402006951
    Series Statement: Astrophysics and space science library 279
    Note: Includes bibliographical references and indexes
    Language: English
    Subjects: Physics
    RVK:
    Keywords: Sternkorona ; Plasmaphysik ; Sonnenkorona ; Plasmaphysik
    Author information: Benz, Arnold 1945-
    Library Location Call Number Volume/Issue/Year Availability
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