Co/Ni Ratio Between 0.8-5 GeV/nucleon from TIGER-2001

Creators: de Nolfo, G. A.; Barbier, L. M.; Binns, W. R.; Cummings, J. R.; Geier, S.; Israel, M. H.; Link, J. T.; Mewaldt, R. A.; Mitchell, J. W.; Rauch, B. F.; Schindler, S. M.; Scott, L. M.; Stone, E. C.; Streitmatter, R. E.

Others:: Acharya, B.; Gupta, S.; Jain, Atul; Karthikeyan, S.; Morris, S.; Tonwar, S.

Abstract

The 2001 flight of TIGER lasted 31.8 days and collected sufficient statistics to study the Co/Ni elemental ratio over a wide range in energies. We present the elemental ratio of Co/Ni in galactic cosmic rays between ~0.80-5 GeV /nucleon and compare our results with previous measurements and propagation models.

Additional Information

Copyright TATA Institute of Fundamental Research. This research was supported by the National Aeronautics and Space Administration under grant NAGS-5078.

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