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The medium energy cosmic ray experiment for ISEE-CA description is provided of the medium energy cosmic ray experiment on board the ISEE-C spacecraft. This experiment is designed to measure the charge composition of nuclear energetic particles over wide ranges in energy (1-500 MeV/nucleon) and in charge (Z equals 1-28). Individual isotopes are resolvable for Z equals 1-7 over a restricted energy range. Electrons of 2-10 MeV are measured as well. These measurements are accomplished using all solid-state detector telescopes with detectors ranging in thickness from 15-3000 microns. The scientific goals of the experiment are also described. These include study of the composition of energetic particles from the sun and from the galaxy, the acceleration and flow of particles in the interplanetary medium, and electrons from Jupiter. Heliospheric gradients and other characteristics of solar modulation will be measured in conjunction with identical telescopes flown on the Voyager 1 and 2 spacecraft and similar telescopes on Pioneer 10 and 11.
Document ID
19780065154
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Von Rosenvinge, T. T.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mcdonald, F. B.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Trainor, J. H.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Van Hollebeke, M. A. I.
(NASA Goddard Space Flight Center Greenbelt; Maryland, University, College Park, Md., United States)
Fisk, L. A.
(New Hampshire, University Durham, N.H., 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
78A49063
Distribution Limits
Public
Copyright
Other

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