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A cosmic ray isotope spectrometerThe paper describes a new instrument to be flown on ISEE-C which is optimized to measure the isotopic composition of solar and galactic cosmic rays in the 5-250 MeV/nucleon range. A mass resolution of not greater than 0.3 AMU should be achieved for all elements with charge Z not exceeding 30.
Document ID
19780065153
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Althouse, W. E. (California Inst. of Tech. Pasadena, CA, United States)
Cummings, A. C. (California Inst. of Tech. Pasadena, CA, United States)
Garrard, T. L. (California Inst. of Tech. Pasadena, CA, United States)
Mewaldt, R. A. (California Inst. of Tech. Pasadena, CA, United States)
Stone, E. C. (California Inst. of Tech. Pasadena, CA, United States)
Vogt, R. E. (California Institute of Technology Pasadena, Calif., 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
78A49062
Funding Number(s)
CONTRACT_GRANT: NAS5-20721
CONTRACT_GRANT: NGR-05-002-160
Distribution Limits
Public
Copyright
Other

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