Add to ORKGThe size dependence of high energy muons and the size spectrum obtained in the air shower experiment suggest that the mean mass of cosmic rays remains nearly constant at approx 15 up to 5 x 1000,000 GeV and becomes one beyond. The composition model in which nuclei are removed spectrum steepens at 6.7 x 10 power GeV due to leakage from the galaxy, which explains the data which are consistent with data from other experiments
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
It is argued that above 10 to the 5th power GeV/nucleus, in the range where charge-resolved spectra ...
Recent results from the KASCADE extensive air shower experiment are presented. After briefly reviewi...
Abstract The evolution of the cosmic ray primary composition in the energy range 10 6 –10 7 GeV (...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground b...
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around th...
Estimation of the relative intensities of protons and heavy nuclei in primary cosmic rays in the ene...
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 10^15 and 10^16 eV, i.e., around the ...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
It is argued that above 10 to the 5th power GeV/nucleus, in the range where charge-resolved spectra ...
Recent results from the KASCADE extensive air shower experiment are presented. After briefly reviewi...
Abstract The evolution of the cosmic ray primary composition in the energy range 10 6 –10 7 GeV (...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
The cosmic ray primary composition in the energy range between 10(15) and 10(16) eV, i.e., around th...
Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground b...
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around th...
Estimation of the relative intensities of protons and heavy nuclei in primary cosmic rays in the ene...
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 10^15 and 10^16 eV, i.e., around the ...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
It is argued that above 10 to the 5th power GeV/nucleus, in the range where charge-resolved spectra ...
Recent results from the KASCADE extensive air shower experiment are presented. After briefly reviewi...