Energy dependence of Ti/Fe ratio in the Galactic cosmic rays measured by the ATIC-2 experiment

Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium has been separated. The energy dependence of the Ti to Fe flux ratio in the energy region from 5 GeV per nucleon to about 500 GeV per nucleon is presented.

Saved in:
Bibliographic Details
Published in:Astronomy letters 2009-05, Vol.35 (5), p.338-342
Main Authors: Zatsepin, V. I., Panov, A. D., Sokolskaya, N. V., Adams, J. H., Ahn, H. S., Bashindzhagyan, G. L., Chang, J., Christl, M., Fazely, A. R., Guzik, T. G., Isbert, J. B., Kim, K. C., Kouznetsov, E. N., Panasyuk, M., Seo, E. S., Watts, J., Wefel, J. P., Wu, J.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Astrophysics and Astroparticles
Cosmic rays
Observations and Techniques
Physics
Physics and Astronomy
Titanium
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium has been separated. The energy dependence of the Ti to Fe flux ratio in the energy region from 5 GeV per nucleon to about 500 GeV per nucleon is presented.
ISSN:1063-7737
1562-6873
DOI:10.1134/S1063773709050089