0
Your cart

Your cart is empty

Books > Science & Mathematics > Physics > States of matter > Plasma physics

Buy Now

Plasma Astrophysics - Kinetic Processes in Solar and Stellar Coronae (Paperback, 2nd ed. 2002. Softcover reprint of the original 2nd ed. 2002) Loot Price: R4,495
Discovery Miles 44 950
Plasma Astrophysics - Kinetic Processes in Solar and Stellar Coronae (Paperback, 2nd ed. 2002. Softcover reprint of the...

Plasma Astrophysics - Kinetic Processes in Solar and Stellar Coronae (Paperback, 2nd ed. 2002. Softcover reprint of the original 2nd ed. 2002)

Arnold O. Benz

Series: Astrophysics and Space Science Library, 279

 (sign in to rate)
Loot Price R4,495 Discovery Miles 44 950 | Repayment Terms: R421 pm x 12*

Bookmark and Share

Expected to ship within 10 - 15 working days

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.

General

Imprint: Springer
Country of origin: Netherlands
Series: Astrophysics and Space Science Library, 279
Release date: April 2014
First published: 2002
Authors: Arnold O. Benz
Dimensions: 235 x 155 x 18mm (L x W x T)
Format: Paperback
Pages: 309
Edition: 2nd ed. 2002. Softcover reprint of the original 2nd ed. 2002
ISBN-13: 978-9401750882
Categories: Books > Science & Mathematics > Physics > Atomic & molecular physics
Books > Science & Mathematics > Astronomy, space & time > Solar system > General
Books > Science & Mathematics > Physics > States of matter > Plasma physics
Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
LSN: 9401750882
Barcode: 9789401750882

Is the information for this product incomplete, wrong or inappropriate? Let us know about it.

Does this product have an incorrect or missing image? Send us a new image.

Is this product missing categories? Add more categories.

Review This Product

No reviews yet - be the first to create one!

Partners