Add to ORKGThe energy spectrum and composition of cosmic rays with primary energies between $10\sp{14}$ eV and $10\sp{16}$ eV have been studied with the CASA-MIA detector in order to provide experimental evidence to compare with competing models of cosmic ray acceleration. New measurements in this energy region are needed to understand previous contradictory experimental results. The CASA-MIA detector is a ground based air shower array, with 1089 surface detectors spaced 15 meters apart and 1024 buried muon detectors in 16 patches, used to measure the lateral distributions of the electromagnetic and muonic portions of air showers. The CASA-MIA measured differential energy spectrum is a power law with spectral indices of $2.68\pm.05$ below approximatel...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "k...
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10^15 and 10^16 eV, i.e., around the ...
The energy spectrum and composition of cosmic rays with primary energies between $10\sp{14}$ eV and ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "k...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "k...
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10^15 and 10^16 eV, i.e., around the ...
The energy spectrum and composition of cosmic rays with primary energies between $10\sp{14}$ eV and ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the ‘‘...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "k...
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "k...
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around th...
The cosmic ray primary composition in the energy range between 10^15 and 10^16 eV, i.e., around the ...