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Abundances and spectra for cosmic-ray nuclei from lithium to iron for 2 to 150 GeV per nucleon

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/156692· OSTI ID:6389184
We report measurements of the absolute and relative abundances, differential energy spectra, and spectral indices for cosmic-ray nuclei from Li to Fe for 2--150 GeV per nucleon. These measurements were made using a balloon-borne superconducting magnetic spectrometer with scintillators and optical spark chambers. The abundances of Li, Be, and B for rigidities below 10 GV/c are consistent with an energy-independent mean interstellar pathlength of 41/2 +- 1/2 g cm/sup -2/ for the ''leaky-box'' propagation model. The abundances of all elements above 10 GV/c are consistent with an interstellar path length that decreases with rigidity as R/sup -n/ with an index n=0.6(+0.4, -0.3). All differential source spectra can be fitted by power laws in total energy per nucleon with the same spectral index, which is between 2.5 and 2.6 depending on n. If n is near 0.5 (as for simple diffusion), the source index is 2.54 +- 0.03. Relative abundances at the sources are thus independent of energy, and have ratios to solar abundances as a function of first ionization potential which indicate a source temperature between 10/sup 4/ and 5 x 10/sup 4/ K depending on the equilibrium nature of the injection environment.
Research Organization:
Spaces Sciences Laboratory and Lawrence Berkeley Laboratory, University of California, Berkeley
OSTI ID:
6389184
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 226:3; ISSN ASJOA
Country of Publication:
United States
Language:
English