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Published 1995 | Version Published
Book Section - Chapter Open

Cosmic Ray Hydrogen Isotopes from 0.2 to 3.0 GeV/nucleon

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Abstract

We have measured the energy dependent abundances of the hydrogen isotopes by the IMAX balloon-borne magnet spectrometer during a flight in July, 1992. A high- resolution time-of-flight system was used in conjunction with a drift chamber/MWPC-tracking system to determine the mass by means of a velocity vs. magnetic rigidity technique. A model of the instrument response was developed in order to unfold the species and rigidity-dependent effects. Measurements of the ^2H/^1 H-ratio from 0.2 to 3.0 Ge V / n will be presented.

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© IUPAP. Provided by the NASA Astrophysics Data System.

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46359
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CaltechAUTHORS:20140619-114146710

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http://adsabs.harvard.edu/abs/1995ICRC....2..614R (URL)

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2014-06-26
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2020-03-09
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Space Radiation Laboratory
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Space Radiation Laboratory
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1995-29