Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Statistics
  • Help & Advice
University of Warwick

The Library

  • Login

Kelvin-Helmholtz multi-spacecraft studies at the Earth's magnetopause boundaries

Tools
- Tools
+ Tools

Foullon, C. (Claire), Farrugia, C. J. (Charles John), Owen, C. J. (Christopher J.), Fazakerley, A. N. and Gratton, F. T. (2010) Kelvin-Helmholtz multi-spacecraft studies at the Earth's magnetopause boundaries. In: 12th International Solar Wind Conference, St Milo, France, 21-26 Jun 2009. Published in: AIP Conference Proceedings, Vol.1216 (No.1). pp. 483-486.

Full text not available from this repository.
Official URL: http://dx.doi.org/10.1063/1.3395908

Abstract

The Kelvin-Helmholtz (KH) instability can operate in various situations in the solar wind, but at the boundaries of planetary obstacles, for example the Earth's magnetopause, it is most amenable to investigation. Reliable estimates of wave characteristics are essential for comparison with theoretical and numerical models and for understanding the non-linear development of KH waves and their role in the plasma entry into the magnetosphere. After discussing their typical conditions of appearance in KH unstable domains at the magnetopause, both theoretically and observationally, we outline recent results of multi-spacecraft analysis with Cluster giving accurate, albeit spatially limited, determination of surface wave characteristics. Those characteristics (wavelength and propagation direction), close to the terminator on the nightside, are likely to be prescribed by the 3-D geometry and the bending of field lines developed by the KH waves, rather than by the magnitude and the direction of the magnetosheath or background flow. An unprecedented number of satellites provides now the opportunity to extend the analysis of source regions of KH waves and their domains of development.

Item Type: Conference Item (Paper)
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Magnetopause, Magnetosphere, Magnetohydrodynamic waves, Solar wind
Series Name: AIP Conference Proceedings
Journal or Publication Title: AIP Conference Proceedings
Publisher: American Institute of Physics
ISBN: 978-0-7354-0759-6
ISSN: 0094-243X
Editor: Maksimovic, M and Issautier, K and MeyerVernet, N and Moncuquet, M and Pantellini, F
Date: 25 March 2010
Volume: Vol.1216
Number: No.1
Number of Pages: 4
Page Range: pp. 483-486
Identification Number: 10.1063/1.3395908
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Conference Paper Type: Paper
Title of Event: 12th International Solar Wind Conference
Type of Event: Conference
Location of Event: St Milo, France
Date(s) of Event: 21-26 Jun 2009
URI: http://wrap.warwick.ac.uk/id/eprint/5281

Data sourced from Thomson Reuters' Web of Knowledge

Request changes to a record

Actions (login required)

View Item View Item
twitter

Email us: publications@warwick.ac.uk
Contact Details
About Us