The Cosmic Ray Isotope Spectrometer for the Advanced Composition Explorer

@inproceedings{Stone1998TheCR,
  title={The Cosmic Ray Isotope Spectrometer for the Advanced Composition Explorer},
  author={Edward C. Stone and Christina M. S. Cohen and Walter R. Cook and Alan C. Cummings and B. Gauld and Branislav Kecman and RA. LESKE and Richard A. Mewaldt and Matt Thayer and Brian L. Dougherty and R. L. Grumm and B. D. Milliken and Robert G. Radocinski and Mark E. Wiedenbeck and Susan Shuman and H. Trexel and Tycho T. von Rosenvinge and W Robert Binns and Diana Crary and Paul Dowkontt and Joyce Epstein and P. L. Hink and Joshua Klarmann and Michal Lijowski and M. A. Olevitch},
  year={1998}
}
The Cosmic-Ray Isotope Spectrometer is designed to cover the highest decade of the Advanced Composition Explorer’s energy interval, from ∼50 to∼500 MeV nucl −1, with isotopic resolution for elements fromZ ' 2 to Z ' 30. The nuclei detected in this energy interval are predominantly cosmic rays originating in our Galaxy. This sample of galactic matter can be used to investigate the nucleosynthesis of the parent material, as well as fractionation, acceleration, and transport processes that these… CONTINUE READING
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