Numerical Simulation of Interplanetary and Magnetospheric Phenomena: The Kelvin-Helmholtz Instability

  1. J. H. Waite Jr.,
  2. J. L. Burch and
  3. R. L. Moore
  1. Melvyn L. Goldstein1,
  2. D. Aaron Roberts1 and
  3. William H. Matthaeus2

Published Online: 18 MAR 2013

DOI: 10.1029/GM054p0113

Solar System Plasma Physics

Solar System Plasma Physics

How to Cite

Goldstein, M. L., Aaron Roberts, D. and Matthaeus, W. H. (1989) Numerical Simulation of Interplanetary and Magnetospheric Phenomena: The Kelvin-Helmholtz Instability, in Solar System Plasma Physics (eds J. H. Waite, J. L. Burch and R. L. Moore), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM054p0113

Author Information

  1. 1

    Code 692, Laboratory for Extraterrestrial Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771

  2. 2

    Bartol Research Institute, University of Delaware, Newark, DE 19716

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 1989

ISBN Information

Print ISBN: 9780875900742

Online ISBN: 9781118664315

SEARCH

Options for accessing this content:

  • If you have access to this content through a society membership, please first log in to your society website.
  • Login via other institutional login options http://onlinelibrary.wiley.com/login-options.
  • You can purchase online access to this Chapter for a 24-hour period (price varies by title)
    • If you already have a Wiley Online Library or Wiley InterScience user account: login above and proceed to purchase the article.
    • New Users: Please register, then proceed to purchase the article.

Login via OpenAthens

or

Search for your institution's name below to login via Shibboleth.

Please register to:

  • Save publications, articles and searches
  • Get email alerts
  • Get all the benefits mentioned below!

Register now >