The energy spectrum of cascade showers induced by electromagnetic interactions of high energy muons of horizontal cosmic ray flux in iron absorber was measured. The total observation time exceeded 22,000 hours. Both the energy spectrum and angular distributions of cascade showers are fairly described in terms of the usual muon generation processes, with a single power index of the parent meson spectrum over the muon energy range from 150 GeV to 5 TeV
One of the uncertainties in ultrahigh energy cosmic ray (UHECR) observation derives from the hadroni...
We have studied how the energy spectrum of muons at production affects some of the most common measu...
Previous work on the muon component of extensive air showers is described and reviewed with particul...
Spectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle o...
An automated air shower array to investigate the properties of showers accompanied by high energy mu...
An experimental investigation of high energy muons above 200 GeV in extensive air showers has been m...
The Sydney University Giant Air-shower Recorder (SUGAR) measured the energy spectrum of ultra-high-e...
Results of analysis of experimental data on cascade showers with energies of 0.1 – 10 TeV initiated ...
The distribution of muons near shower cores was studied at sea level at Fermilab using the E594 neut...
A small air shower array has been used to measure the size spectrum of air showers at sea level in t...
In view of the interpretation of data collected by large, deep underground experiments in terms of p...
The KASCADE-Grande air shower experiment [1] consists of, among others, a large scintillator array f...
Measurements have been made on high-energy muons (>220 GeV and >640 GeV) in extensive air show...
Muon energy spectra and muon lateral distribution in EAS were investigated with the underground magn...
Two components of cosmic-ray-induced air showers are measured simultaneously at the Gran Sasso Labor...
One of the uncertainties in ultrahigh energy cosmic ray (UHECR) observation derives from the hadroni...
We have studied how the energy spectrum of muons at production affects some of the most common measu...
Previous work on the muon component of extensive air showers is described and reviewed with particul...
Spectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle o...
An automated air shower array to investigate the properties of showers accompanied by high energy mu...
An experimental investigation of high energy muons above 200 GeV in extensive air showers has been m...
The Sydney University Giant Air-shower Recorder (SUGAR) measured the energy spectrum of ultra-high-e...
Results of analysis of experimental data on cascade showers with energies of 0.1 – 10 TeV initiated ...
The distribution of muons near shower cores was studied at sea level at Fermilab using the E594 neut...
A small air shower array has been used to measure the size spectrum of air showers at sea level in t...
In view of the interpretation of data collected by large, deep underground experiments in terms of p...
The KASCADE-Grande air shower experiment [1] consists of, among others, a large scintillator array f...
Measurements have been made on high-energy muons (>220 GeV and >640 GeV) in extensive air show...
Muon energy spectra and muon lateral distribution in EAS were investigated with the underground magn...
Two components of cosmic-ray-induced air showers are measured simultaneously at the Gran Sasso Labor...
One of the uncertainties in ultrahigh energy cosmic ray (UHECR) observation derives from the hadroni...
We have studied how the energy spectrum of muons at production affects some of the most common measu...
Previous work on the muon component of extensive air showers is described and reviewed with particul...