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ISEE-C solar wind plasma experimentTwo 135 deg spherical section electrostatic analyzers furnish electron and ion measurements of the solar wind on ISEE-C. Each of these instruments utilizes a divided secondary emitter system to intercept the analyzed particles. Secondary electrons selected from all of the emitters simultaneously provide fast two-dimensional measurements of the particle fluxes integrated over polar angle; at a slower rate secondary electrons are successively selected from individual emitters to provide three-dimensional measurements. Speed of the ion measurements is increased by a factor of two by using an active proton peak tracking system to reduce the total range of energy per charge which has to be covered.
Document ID
19780065144
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bame, S. J.
(Los Alamos Scientific Lab. NM, United States)
Asbridge, J. R.
(Los Alamos Scientific Lab. NM, United States)
Felthauser, H. E.
(Los Alamos Scientific Lab. NM, United States)
Glore, J. P.
(California, University Los Alamos Scientific Laboratory, Los Alamos, N. Mex., United States)
Hawk, H. L.
(Los Alamos Scientific Lab. NM, United States)
Chavez, J.
(Sandia Laboratories Albuquerque, N. Mex., United States)
Date Acquired
August 9, 2013
Publication Date
July 1, 1978
Publication Information
Publication: IEEE Transactions on Geoscience Electronics
Volume: GE-16
Subject Category
Spacecraft Instrumentation
Accession Number
78A49053
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-54496-A
Distribution Limits
Public
Copyright
Other

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