NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A comparative study of plasma expansion events in the polar windThe temporal characteristics of the polar wind have been studied using a simplified set of collisionless equations and a full set of hydrodynamic equations which contained continuity, momentum, and energy equations for H(+), O(+), and electrons, including collisional conductivities and variable isotropic, ion and electron temperatures. The temporal evolution of the polar wind was modeled for initial, extended density depletions of factors of 3, 10, and 100 starting at several altitudes for each model. Comparison of the results from the two models showed the same temporal characteristics for the polar wind densities, flow velocities, and escape fluxes. The characteristics of plasma expansion are presented. It is found that the propagation velocities of the disturbance vary with the level of the depletion.
Document ID
19880060324
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gombosi, Tamas I.
(Michigan, University Ann Arbor, United States)
Schunk, Robert W.
(Utah State University Logan, United States)
Date Acquired
August 13, 2013
Publication Date
August 1, 1988
Publication Information
Publication: Planetary and Space Science
Volume: 36
ISSN: 0032-0633
Subject Category
Geophysics
Accession Number
88A47551
Funding Number(s)
CONTRACT_GRANT: NSF ATM-85-08753
CONTRACT_GRANT: NAG5-472
CONTRACT_GRANT: NAGW-77
Distribution Limits
Public
Copyright
Other

Available Downloads

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