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The cosmic ray and solar flare isotope experiments in the CRRES, NOAA-I and Ulysses'' satellites

Conference · · AIP Conference Proceedings (American Institute of Physics); (USA)
OSTI ID:6808010
 [1]
  1. Laboratory for Astrophysics and Space Research Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637 (USA)
The ONR-604 instrument has been designed to measure the energy spectra and the isotopic composition at 1 AU of the elements Hydrogen to Nickel in the energy range 40--500 MeV/n and will be carried by the Combined Release and Radiation Effects Satellite (CRRES) to be launched July, 1990 in a highly eccentric orbit between a low perigee and a synchronous orbit point. It will measure galactic cosmic rays, solar energetic particles, and trapped and pseudo-trapped particles in the Earth magnetosphere. Also at 1 AU, the Energetic Heavy Ion Composition (EHIC) instrument, designed to study mainly the elemental and isotopic composition of solar energetic particles over the charge range H to Ni, in the energy range 0.5 to 200 MeV/n, will be placed in a Sun-synchronous circular polar orbit of 833 or 870 km altitude by a NOAA-I satellite scheduled to be launched late 1990 or early 1991. The University of Chicago High Energy Telescope (HET) experiment which is part of the COSPIN consortium on the Ulysses'' mission will measure the energy spectra and the isotopic composition of the elments Hydrogen to Nickel in the energy interval 20--450 MeV/n in the heliosphere, both the ecliptic plane and at high heliographic latitudes in an orbit around the Sun that will have an aphelion near a Jupiter orbit point and a perhelion of about 1.4 AU. It will be launched October 1990.
OSTI ID:
6808010
Report Number(s):
CONF-8911161--
Conference Information:
Journal Name: AIP Conference Proceedings (American Institute of Physics); (USA) Journal Volume: 203:1
Country of Publication:
United States
Language:
English