The cosmic ray spectrum above 10(17) eV

Details The cosmic ray spectrum above 10(17) eV The cosmic ray spectrum above 10(17) eV

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icrc....9..499w&link_type=abstract

In NASA. Goddard Space Flight Center Nineteenth International Cosmic Ray Conference. Conference Papers: Invited Rapporteur, High

Physics

Cosmic Ray Showers, Energy Spectra, Particle Density (Concentration), Muons, Photomultiplier Tubes, Zenith

Scientific paper

The final analysis of the data obtained by the Sydney University Giant Airshower Recorder (SUGAR) is presented. The data has been reanalysed to take into account the effects of afterpulsing in the photomultiplier tubes. Event data was used to produce a spectrum of equivalent vertical muon number and from this a model dependent primary energy spectrum was obtained. These spectra show good evidence for the Ankle: a flattening at 10(19) eV. There is no sign of the cut-off which would be expected from the effects of the universal black body radiation.

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