Physics of collisionless shocks
Read Online
Share

Physics of collisionless shocks proceedings of the D2.1 Symposium of COSPAR Scientific Commission D which was held during the Thirtieth COSPAR Scientific Assembly, Hamburg, Germany, 11-21 July, 1994 by COSPAR. Plenary Meeting

  • 26 Want to read
  • ·
  • 25 Currently reading

Published by Published for the Committee on Space Research [by] Pergamon Press in Oxford, Tarrytown, N.Y .
Written in English

Subjects:

  • Astrophysics -- Congresses.,
  • Shock waves -- Congresses.

Book details:

Edition Notes

Includes bibliographical references and index.

Statementedited by C.T. Russell.
SeriesAdvances in space research -- v. 15, no. 8-9
ContributionsRussell, C. T., COSPAR. Scientific Commission D.
Classifications
LC ClassificationsQB461 .C676 1994
The Physical Object
Paginationix, 544 p. :
Number of Pages544
ID Numbers
Open LibraryOL21345222M
ISBN 100080425585

Download Physics of collisionless shocks

PDF EPUB FB2 MOBI RTF

The 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 by: The 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 . Physics of Collisionless Shocks: Space Plasma Shock Waves André Balogh, Rudolf A. Treumann (auth.) The present book provides a contemporary systematic treatment of shock waves in high-temperature collisionless plasmas as are encountered in . The 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.

  Physics of Collisionless Shocks by Andre Balogh, , available at Book Depository with free delivery worldwide. springer, The 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 . adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86ACited by: Collisionless shocks occur in various fields of physics. In the context of space and astrophysics they have been investigated for many decades. However, a thorough understanding of shock formation and particle acceleration is still missing. Collisionless shocks can be distinguished into electromagnetic and electrostatic shocks.

Full particle-in-cell simulation of the interaction between two plasmas for laboratory experiments on the generation of magnetized collisionless shocks with high-power lasers. Physics of Plasmas, Vol. 26, Issue. 3, p. Cited by:   Shock waves are an important feature of solar system plasmas, from the solar corona out to the edge of the heliosphere. This engaging introduction to collisionless shocks in space plasmas presents a comprehensive review of the physics governing different types of shocks and processes of particle acceleration, from fundamental principles to current research. Physics of Collisionless Shocks: Space Plasma Shock Waves (Inglese) Copertina rigida – 3 gennaio di Andre Balogh (Autore), Rudolf A. Treumann (Autore) 5,0 su 5 stelle 2 votiReviews: 2. Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume Violent expansions of the solar corona cause transient shock waves which propagate outward from the sun at hundreds to thousands of kilometers per second; simple solar wind velocity gradients at the surface of the sun lead to high-speed streams overtaking slower .