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Study plasma interactions in the auroral ionosphereAnalyzed data from rocket flight, 29.007UE is presented. In a discrete electron arc the measured upward moving electrons are well accounted for by secondaries produced in collisional scattering of the measured downcoming electrons. No collective mechanisms need to invoke. The low energy downcoming electrons are accounted for by thermal plasma accelerated through a potential drop of a few kV that specularly reflects upward-moving lower energy electrons. No low altitude collective effects need to invoke in the arc. Simultaneous measurements of electric field by double probes on 29.007 and the Chatanika Radar allow one to infer that there are upward drifting ions above the discrete electron arc, and there is a westward neutral wind in the discrete arc. Two rocket payloads were built to investigate plasma effects in the pulsating aurora.
Document ID
19840008630
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Anderson, H. R.
(Science Applications, Inc., Bellevue Wash., United States)
Wolf, R. A.
(Rice Univ. Houston, TX, United States)
Date Acquired
September 4, 2013
Publication Date
September 1, 1983
Subject Category
Geophysics
Report/Patent Number
NASA-CR-175352
SAI/NW-83-428-06
NAS 1.26:175352
Report Number: NASA-CR-175352
Report Number: SAI/NW-83-428-06
Report Number: NAS 1.26:175352
Accession Number
84N16698
Funding Number(s)
CONTRACT_GRANT: NAG6-5
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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