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A new analysis of cosmic ray isotopes at 3 GeV/n from HEA03-C2 dataResults of mean masses of cosmic rays at energy about 3 GeV/n, for Ne, Al, Mg, Si, S, Ca, and Fe, derived from high energy astronomy observatory 3 data collected by the Danish-French experiment C2 on board (HEAO-3) are presented. A method based upon comparison between observed transmission function and a predicted one computed from a geomagnetic field model was used. Enhancement factors of 2.9 + or - .7 for 22Ne/20Ne, 2.1 + or - .4 for (25Mg+26Mg)/24Mg, and 1.6 + or - .8 for (29Si+30Si)/28Si at GCRS when compared to LG were found.
Document ID
19850025718
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ferrando, P. (Commissariat a l'Energie Atomique Saclay, France)
Goret, P. (Commissariat a l'Energie Atomique Saclay, France)
Koch-Miramond, L. (Commissariat a l'Energie Atomique Saclay, France)
Petrou, N. (Commissariat a l'Energie Atomique Saclay, France)
Soutoul, A. (Commissariat a l'Energie Atomique Saclay, France)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-4.3-6
Accession Number
85N34031
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025693Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 2
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