High Energy Cosmic Rays Investigations by Cerenkov radiation Generated in the Upper Atmosphere.

Details High Energy Cosmic Rays Investigations by Cerenkov radiation Generated in the Upper Atmosphere. High Energy Cosmic Rays Investigations by Cerenkov radiation Generated in the Upper Atmosphere.

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2167p&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We discuss opportunities to study nuclei/antinuclei and electron/positron cosmic rays fluxes by Cerenkov radiation generated in the upper atmosphere. For balloon experiment (altitude of flights ~ 30-35 km) an ability to register nuclei/antinuclei cosmic rays fluxes at energies 0.4-4 TeV/n is revealed. Electron/positron spectra can be determined at energies 40 GeV 1 TeV.

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