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The Elemental Composition of 4-30 MeV/nuc Cosmic Ray Nuclei with 1 ≤ Z ≤ 8

Mewaldt, R. A. and Stone, E. C. and Vidor, S. B. and Vogt, R. E. (1975) The Elemental Composition of 4-30 MeV/nuc Cosmic Ray Nuclei with 1 ≤ Z ≤ 8. In: Proceedings of the 14th International Cosmic Rays Conference. Max Planck Gesellschaft , pp. 798-803. http://resolver.caltech.edu/CaltechAUTHORS:20140410-134228705

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Abstract

Recent observations of low energy cosmic rays have shown enhanced fluxes of nitrogen and oxygen relative to other elements in the ~8-30 MeV/nuc energy interval. We have extended the measurements of lithium through oxygen down to ~ 4 MeV/nuc with the Caltech Electron/Isotope Spectrometers on IMP-7 and -8 during solar quiet periods from October 1972 to September 1974. We find no evidence for significant enhancements of Li, Be, B. or C, which are found to have energy spectra consistent with those expected from the adiabatic deceleration of higher energy galactic cosmic rays. The He, N, and O fluxes are greatly enhanced when compared to the other elements, with relative abundances of O/He ~ 0.25, O/B ~ 100, and O/C ~ 30 at ~ 5 to 12.5 MeV/nuc.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1975ICRC....2..798MADSArticle
Contact Email Address:dmiles@caltech.edu
Additional Information:© 1975 MPE. Provided by the NASA Astrophysics Data System. This work was supported in part by the National Aeronautics and Space Administration under Contract NAS5-11066 and Grant NGR 05-002-160.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAS5-11066
NASANGR 05-002-160
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1975-10
Record Number:CaltechAUTHORS:20140410-134228705
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140410-134228705
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:44866
Collection:CaltechAUTHORS
Deposited By: SWORD User
Deposited On:14 Apr 2014 22:51
Last Modified:15 Apr 2014 20:53

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