Shock Waves in Collisionless Plasmas
Author: Derek A. Tidman
Publisher: John Wiley & Sons
Published: 1971
Total Pages: 202
ISBN-13:
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Author: Derek A. Tidman
Publisher: John Wiley & Sons
Published: 1971
Total Pages: 202
ISBN-13:
DOWNLOAD EBOOKAuthor: André Balogh
Publisher: Springer Science & Business Media
Published: 2013-01-04
Total Pages: 503
ISBN-13: 1461460999
DOWNLOAD EBOOKThe present book provides a contemporary systematic treatment of shock waves in high-temperature collisionless plasmas as are encountered in near Earth space and in Astrophysics. It consists of two parts. Part I develops the complete theory of shocks in dilute hot plasmas under the assumption of absence of collisions among the charged particles when the interaction is mediated solely by the self-consistent electromagnetic fields. Such shocks are naturally magnetised implying that the magnetic field plays an important role in their evolution and dynamics. This part treats subcritical shocks which dissipate flow energy by generating anomalous resistance or viscosity. The main emphasis is, however, on super-critical shocks where the anomalous dissipation is insufficient to retard the upstream flow. These shocks, depending on the direction of the upstream magnetic field, are distinguished as quasi-perpendicular and quasi-parallel shocks which exhibit different behaviours, reflecting particles back upstream and generating high electromagnetic wave intensities. Particle acceleration and turbulence at such shocks become possible and important. Part II treats planetary bow shocks and the famous Heliospheric Termination shock as examples of two applications of the theory developed in part I.
Author: James M. Witting
Publisher:
Published: 1964
Total Pages: 366
ISBN-13:
DOWNLOAD EBOOKAuthor: David Burgess (Astrophysicist)
Publisher:
Published: 2015
Total Pages: 356
ISBN-13: 9781316356753
DOWNLOAD EBOOKAuthor: Lynn Mary Olson
Publisher:
Published: 1970
Total Pages: 176
ISBN-13:
DOWNLOAD EBOOKSmall amplitude near-steady oblique shock waves in a collisionless plasma are possible at Alfven Mach numbers 1 and cos theta. In the first case, either the magnetic pressure decreases monotonely or the head of the wave is near-periodic. In the second case, a main wavefront is followed by an oscillatory tail. (Author).
Author: David Burgess
Publisher: Cambridge University Press
Published: 2015-07-30
Total Pages: 367
ISBN-13: 0521514592
DOWNLOAD EBOOKAn engaging introduction to collisionless shocks in space plasmas, presenting a complete review, from first principles to current research.
Author: Mahmoud H. Ahmed
Publisher:
Published: 1972
Total Pages: 288
ISBN-13:
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Publisher:
Published: 1995
Total Pages: 10
ISBN-13:
DOWNLOAD EBOOKCollisionless shock waves are a very important heating mechanism for plasmas and are commonly found in space and astrophysical environments. Collisionless shocks were studied in the laboratory more than 20 years ago, and more recently in space via in situ satellite measurements. The authors propose a new laboratory shock wave experiment to address unresolved issues related to the differences in the partition of plasma heating between electrons and ions in space and laboratory plasmas, which can have important implications for a number of physical systems.
Author: R. Z. Sagdeev
Publisher:
Published: 1965
Total Pages: 80
ISBN-13:
DOWNLOAD EBOOKAuthor: Michael A. Liberman
Publisher: Springer
Published: 1986
Total Pages: 408
ISBN-13:
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