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Synthesis of data obtained at Jicamarca, Peru, during the September 11, 1969, eclipse.Results of continuous measurements of electron temperatures, electron concentrations, and vertical plasma drift made at Jicamarca during the Sept. 11, 1969, solar eclipse and of control measurements made on Sept. 13, 1969. Synthesis of the observed electron concentrations was made, using a model that solved the time-dependent electron-ion continuity equations. Ions O(-), NO(+), O2(+), and N2(+) were treated. Physical and chemical processes pertinent to the F region were considered in a realistic way. At noon, 300 km above Jicamarca, the values q = 290 per cu cm per sec for the O(+) production rate, beta = 1.94 x 0.0001 per sec for the loss coefficient, and H = 59 km for the atomic oxygen scale height were obtained. All large-scale features observed in the F2 region were synthesized by the model. This synthesis was not sensitive to a simultaneous 30% reduction of q and beta.
Document ID
19720039852
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sterling, D. L.
Hanson, W. B.
(Texas, University Dallas, Tex., United States)
Woodman, R. F.
(Jicamarca Radar Observatory Lima, Peru)
Date Acquired
August 6, 2013
Publication Date
February 1, 1972
Publication Information
Publication: Radio Science
Volume: 7
Subject Category
Space Sciences
Accession Number
72A23518
Funding Number(s)
CONTRACT_GRANT: NGL-44-004-001
CONTRACT_GRANT: NGR-52-158-001
Distribution Limits
Public
Copyright
Other

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