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- W3150256050 abstract "S u m m a r y . A measurement of the p r imary spectrum of the cosmic radiat ion in the energy range of 5.1O 1~ cV to ~ 5.1O 15 eV has been made, employing the detcction of atmospheric (~erenkov-light pulses produced in extensive air showcrs. Through the use of an all l inear system and an extensive series of calibration, the uncertaint ies of previous measurements have been removed. The relation between the ~erenkov pulseheight spectrum and thc p r imary cosmic-ray spectrum was invest igated through the use of i~Ionte Carlo air shower simulations designed specifically for in terpreta t ion of the results of this experiment, covering prim~try eJmrgics from 10 ~ eV to 10 ~3 eV. These indicate that , due to large fluctuations in shower development, the technique is relat ively insensitive to the spcctrum of primaries at energies of l0 H eV to 1013 eV. The simulations also indicate a decrease in the importance of fluctuations with increasing pr imary energy. The measured spectral index shows an increase at ~ 1.5.10 ~5 eV. The physical implicat ions of this bending are discussed." @default.
- W3150256050 created "2021-04-13" @default.
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- W3150256050 date "2007-01-01" @default.
- W3150256050 modified "2023-09-27" @default.
- W3150256050 title "The Primary Cosmic-Radiation Spectrum from 1012 eV to 1015 eV from Atmospheric (~erenkov-Radiation Measurements" @default.
- W3150256050 hasPublicationYear "2007" @default.
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