Generation of Whistler-Mode Radiation by Parametric Decay of Bernstein Waves

R. W. Boswell and M. Giles
Phys. Rev. Lett. 39, 277 – Published 1 August 1977
PDFExport Citation

Abstract

It is shown both experimentally and theoretically that a Bernstein wave can decay parametrically into another Bernstein wave and a whistler-mode wave. The process only occurs in a highly collisionless plasma and it is suggested that this is the dominant mechanism for producing whistler-mode noise in the auroral ionosphere.

  • Received 11 August 1976

DOI:https://doi.org/10.1103/PhysRevLett.39.277

©1977 American Physical Society

Authors & Affiliations

R. W. Boswell

  • Space Science Department, European Space Agency, Noordwijk, The Netherlands

M. Giles

  • Space and Plasma Physics Group, University of Sussex, Sussex, England

References (Subscription Required)

Click to Expand
Issue

Vol. 39, Iss. 5 — 1 August 1977

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×