NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Plasma transport in the Io torus - The importance of microscopic diffusionThis paper considers the question of whether the distribution of mass in the Io plasma torus is consistent with the concept of interchange eddy transport. Specifically, the flux tube content exhibits a gradual decrease with increasing radial distance from the source near Io without any evidence for substantial density irregularity associated with the plasma source or loss. Using a simple one-dimensional numerical model to simulate macroscopic interchange eddy transport, it is demonstrated that this smooth equilibrium distribution of mass can occur but only with the inclusion of a minimal level of small scale microscopic mixing at a rate approaching Bohm diffusion. Otherwise, the system exhibits a chaotic appearance which never approaches an equilibrium distribution. Various physical mechanisms for the microscopic diffusion process which is required to provide a sufficiently rapid mixing of material between the macroscopic eddies are discussed.
Document ID
19910041653
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mei, YI
(California Univ. Los Angeles, CA, United States)
Thorne, Richard M.
(California, University Los Angeles, United States)
Date Acquired
August 14, 2013
Publication Date
February 1, 1991
Publication Information
Publication: Geophysical Research Letters
Volume: 18
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
91A26276
Funding Number(s)
CONTRACT_GRANT: NAGW-1639
CONTRACT_GRANT: NSF ATM-87-18108
Distribution Limits
Public
Copyright
Other

Available Downloads

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