Isotopic analysis of cosmic rays by the Cerenkov-Cerenkov slowing-down method

Details Isotopic analysis of cosmic rays by the Cerenkov-Cerenkov slowing-down method Isotopic analysis of cosmic rays by the Cerenkov-Cerenkov slowing-down method

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stia...7532534m&link_type=abstract

(ESRO, Workshop on Research Goals for Cosmic-Ray Astrophysics in the 1980's, Frascati, Italy, Oct. 24, 25, 1974.) Revue Scientif

Astronomy and Astrophysics

Astrophysics

Cerenkov Counters, Cosmic Rays, Isotope Effect, Nuclear Interactions, Balloon Flight, Energy Spectra, Heavy Nuclei, Radiation Measurement

Scientific paper

The performance of a large-scale Cerenkov-Cerenkov slowing-down set-up for isotope analysis in the 1-2 GeV/n region is analysed. Such a setup should permit isotopic analysis of all nuclei between neon and nickel with rms mass errors less than 0.5 amu and less than 1 amu over, respectively, approximately 250 MeV/n and approximately 500 MeV/n energy ranges. The background associated with the very high rate of nuclear interactions in the instrument (75 percent) should be eliminated by a triple redundancy in the charge measurement. These estimates are based largely on experience gained from Danish-French balloon flights and from runs at the Berkeley Bevatron.

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