NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Kelvin-Helmholtz instability in the magnetopause-boundary layer regionThe Kelvin-Helmholtz instability in the magnetopause-boundary layer region is studied on the basis of an idealized model which consists of three uniform plasma regions: the magnetosheath, the boundary layer, and the magnetosphere. There are two unstable modes in the magnetopause-boundary layer region: one is excited at the magnetopause (the magnetopause mode) and the other is excited at the inner surface of the boundary layer (the inner mode). The inner mode is found to be unstable most of the time, while the excitation of the magnetopause mode depends on the magnetic field in the magnetosheath. The observed variation of the boundary layer thickness can be attributed to the unstable inner mode. Possible relationships between the Pc 3-5 geomagnetic pulsations and the surface waves excited on the magnetospheric boundary are also discussed.
Document ID
19810038502
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lee, L. C.
(Alaska Univ. Fairbanks, AK, United States)
Albano, R. K.
(Alaska Univ. Fairbanks, AK, United States)
Kan, J. R.
(Alaska, University Fairbanks, Alaska, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Journal of Geophysical Research
Volume: 86
Subject Category
Geophysics
Accession Number
81A22906
Funding Number(s)
CONTRACT_GRANT: NSG-5409
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available