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Cosmic Ray Helium Isotopes From 0.2 to 3.6 GeV/nucleon

  • O. Reimer
  • , M. Hof
  • , W. Menn
  • , M. Simon
  • , L.M. Barbier
  • , E.R. Christian
  • , K.E. Krombel
  • , J.W. Mitchell
  • , J.F. Ormes
  • , R.E. Streitmatter
  • , A.J. Davis
  • , A.W. Labrador
  • , R.A. Mewaldt
  • , S.M. Schindler
  • , R.L. Golden
  • , S.J. Stochaj
  • , W.R. Webber
  • , Ib Lundgaard Rasmussen

    Research output: Contribution to journalJournal articleResearchpeer-review

    Abstract

    The abundances of cosmic ray helium isotopes were measured by the IMAX balloon-borne magnet spectrometer during a flight in July, 1992. A high-resolution time-of-flight system and two silica aerogel Cherenkov counters were used in conjunction with a drift-chamber/MWPC-tracking system to determine mass by means of the velocity vs. magnetic rigidity technique. A model of the instrument response was developed in order to unfold the species and rigidity-dependent effects. Measurements and astrophysical interpretation of the ^3He/^4He isotope ratio from 0.2 to 3.6 GeV/nucleon will be presented. The IMAX experiment was supported by NASA: RTOP 353-87-02 (GSFC), grants NAGW-1919 (Caltech) and NAGW-1418 (NMSU), and in Germany by the DFG and the BMFT. ^1currently at Max-Planck-Institut für Extraterrestrische Physik
    Original languageEnglish
    JournalAmerican Physical Society Meeting Abstracts
    Pages (from-to)K1003+
    Publication statusPublished - 1996

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