Abundance of very heavy components of primary cosmic rays over Alice Springs.

Details Abundance of very heavy components of primary cosmic rays over Alice Springs. Abundance of very heavy components of primary cosmic rays over Alice Springs.

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998hadjs..13...37b&link_type=abstract

Hadronic J. Suppl., Vol. 13, No. 1, p. 37 - 47

Physics

Cosmic Rays: Element Abundances

Scientific paper

An investigation has been made of the elemental abundance of primary cosmic rays over Alice Springs obtained from the 32 hours exposure of a plastic-emulsion chamber in a balloon. The long hour etched plastic track detector exhibited etch pits whose measured diameter distribution yields a charge abundance in the range of Z values from 10 to 28. The observed charge spectrum has been corrected to account for the loss of fluxes due to interactions and fragmentation by using the standard diffusion equation with fitted partial cross-section of Wilson et al. (1987). The observed charge spectrum has been extrapolated to source by adopting the steady state leaky box model.

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