Description du livre Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 332 pp. Englisch. N� de r�f. du vendeur 9781402006951

Plus d'informations sur ce vendeur | Contacter le vendeur

Acheter neuf

EUR 160,49

Autre devise

Ajouter au panier

Frais de port : EUR 23

De Allemagne vers Etats-Unis

Destinations, frais et d�lais

Image fournie par le vendeur

Plasma Astrophysics

Arnold O. Benz

Edit� par Springer Netherlands (2002)

ISBN 10 : 1402006950 ISBN 13 : 9781402006951

Neuf Couverture rigide Quantit� disponible : > 20

impression � la demande

Vendeur :

moluna
(Greven, Allemagne)

Evaluation vendeur

Evaluation du vendeur :

Description du livre Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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 physi. N� de r�f. du vendeur 4092037

Plus d'informations sur ce vendeur | Contacter le vendeur

Acheter neuf

EUR 136,16

Autre devise

Ajouter au panier

Frais de port : EUR 48,99

De Allemagne vers Etats-Unis

Destinations, frais et d�lais

Image fournie par le vendeur

Plasma Astrophysics : Kinetic Processes in Solar and Stellar Coronae

Arnold O. Benz

Edit� par Springer Netherlands (2002)

ISBN 10 : 1402006950 ISBN 13 : 9781402006951

Neuf Couverture rigide Quantit� disponible : 1

Vendeur :

AHA-BUCH GmbH
(Einbeck, Allemagne)

Evaluation vendeur

Evaluation du vendeur :

Description du livre Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - 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. N� de r�f. du vendeur 9781402006951

Plus d'informations sur ce vendeur | Contacter le vendeur

Acheter neuf

EUR 164,03

Autre devise

Ajouter au panier

Frais de port : EUR 32,99

De Allemagne vers Etats-Unis

Destinations, frais et d�lais

Image d'archives