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Interpretation of the Helium Isotope Ratios Measured by IMAX

Davis, A. J. and Menn, W. and Barbier, L. M. and Christian, E. R. and Golden, R. L. and Hof, M. and Krombel, K. E. and Labrador, A. W. and Mewaldt, R. A. and Mitchell, J. W. and Ormes, J. F. and Rasmussen, I. L. and Reimer, O. and Schindler, S. M. and Simon, M. and Stochaj, S. J. and Streitmatter, R. E. and Webber, W. R. (1995) Interpretation of the Helium Isotope Ratios Measured by IMAX. In: Proceedings of the 24th International Cosmic Ray Conference. Vol.2. International Union of Pure and Applied Physics , pp. 622-625. https://resolver.caltech.edu/CaltechAUTHORS:20140618-144936615

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Abstract

We present here the IMAX^3He/He^4 ratios between 0.2 and 3.6 GeV /nucleon corrected to the top of the atmosphere, and a preliminary comparison with previous data. and the predictions of a standard 'Leaky Box' model of CR transport in the galaxy. We find no evidence of an excess of ^3He over that predicted by the model, in the energy range studied.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1995ICRC....2..622DADSArticle
ORCID:
AuthorORCID
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
Additional Information:© IUPAP. Provided by the NASA Astrophysics Data System. This work supported by NASA under grant NAGW-1919 and other grants
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAGW-1919
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1995-28
Record Number:CaltechAUTHORS:20140618-144936615
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140618-144936615
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:46346
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:26 Jun 2014 20:46
Last Modified:09 Mar 2020 13:18

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