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Cosmic Ray Hydrogen Isotopes from 0.2 to 3.0 GeV/nucleon

Reimer, O. and Davis, A. J. and Barbier, L. M. and Christian, E. R. and Golden, R. L. and Hof, M. and Krombel, K. E. and Labrador, A. W. and Menn, W. and Mewaldt, R. A. and Mitchell, J. W. and Ormes, J. F. and Rasmussen, I. L. and Schindler, S. M. and Simon, M. and Stochaj, S. J. and Stone, E. C. and Streitmatter, R. E. and Webber, W. R. (1995) Cosmic Ray Hydrogen Isotopes from 0.2 to 3.0 GeV/nucleon. In: Proceedings of the 24th International Cosmic Ray Conference. Vol.2. International Union of Pure and Applied Physics , pp. 614-617.

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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.

Item Type:Book Section
Related URLs:
URLURL TypeDescription
Christian, E. R.0000-0003-2134-3937
Hof, M.0000-0003-2884-3037
Labrador, A. W.0000-0001-9178-5349
Mewaldt, R. A.0000-0003-2178-9111
Stone, E. C.0000-0002-2010-5462
Additional Information:© IUPAP. Provided by the NASA Astrophysics Data System.
Group:Space Radiation Laboratory
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Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1995-29
Record Number:CaltechAUTHORS:20140619-114146710
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:46359
Deposited By: Deborah Miles
Deposited On:26 Jun 2014 20:56
Last Modified:09 Mar 2020 13:18

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