Final Results of RUNJOB and Related Topics

Details Final Results of RUNJOB and Related Topics Final Results of RUNJOB and Related Topics

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..47..106h&link_type=abstract

Journal of Physics: Conference Series, Volume 47, Issue 1, pp. 106-112 (2006).

Physics

3

Scientific paper

This report presents the energy spectra of galactic cosmic rays with the energy ranges between 10 and 1000 TeV/particle based on the full data set obtained by RUNJOB (RUssia Nippon JOint Balloon) experiment. Our proton flux is consistent with the other past observations such as JACEE and SOKOL, but the fluxes of the other components are less than those of the past ones, particularly the RUNJOB helium intensity giving nearly half of those obtained by JACEE and SOKOL. The slope of individual spectra becomes gradually harder as heavier components, in sharp contrast to JACEE and SOKOL data. Comparing the RUNJOB results with the propagation models, it seems to support that the acceleration and the propagation mechanisms of cosmic rays depend simply on particle rigidity.

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