Monte Carlo simulations of extensive air showers were performed using a couple of different nuclear interaction models and obtaining a variety of shower characteristics. The discussion of these shows that the sensitivity of observables to the primary mass spectrum is significantly stronger than to the interaction model, the latter being quite weak
Extensive Air Showers are still the only source of information on primary cosmic rays and their inte...
In view of the interpretation of data collected by large, deep underground experiments in terms of p...
The particle showers produced in the atmosphere due to the interactions of primary cosmic particles ...
This thesis describes the results of computer simulations of cosmic ray extensive air showers with p...
An analysis has been made of the present situation with respect to the high energy hadron-nucleus an...
We present a summary of recent tests and measurements of hadronic interaction properties with air sh...
A method for calculating the average spatial and energy characteristics of hadron-lepton cascades in...
In the sub-TeV regime, the most widely used hadronic interaction models disagree significantly in th...
The x-y controversy is studied by introducing models with as many features (except for x and y distr...
The description of high-energy hadronic interactions plays an important role in the (astrophysical) ...
Experiments measuring cosmic rays above an energy of ∼ 1014 eV deduce the energy and mass of the pri...
One of the most promising approaches to determine the energy spectrum and composition of cosmic rays...
Whereas air shower simulations are very valuable tools for interpreting cosmic ray data, there is a ...
When high-energy cosmic rays (gamma's, protons, or heavy nuclei) impinge onto the Earth's atmosphere...
We report on a study about some characteristics of muon production during the development of extende...
Extensive Air Showers are still the only source of information on primary cosmic rays and their inte...
In view of the interpretation of data collected by large, deep underground experiments in terms of p...
The particle showers produced in the atmosphere due to the interactions of primary cosmic particles ...
This thesis describes the results of computer simulations of cosmic ray extensive air showers with p...
An analysis has been made of the present situation with respect to the high energy hadron-nucleus an...
We present a summary of recent tests and measurements of hadronic interaction properties with air sh...
A method for calculating the average spatial and energy characteristics of hadron-lepton cascades in...
In the sub-TeV regime, the most widely used hadronic interaction models disagree significantly in th...
The x-y controversy is studied by introducing models with as many features (except for x and y distr...
The description of high-energy hadronic interactions plays an important role in the (astrophysical) ...
Experiments measuring cosmic rays above an energy of ∼ 1014 eV deduce the energy and mass of the pri...
One of the most promising approaches to determine the energy spectrum and composition of cosmic rays...
Whereas air shower simulations are very valuable tools for interpreting cosmic ray data, there is a ...
When high-energy cosmic rays (gamma's, protons, or heavy nuclei) impinge onto the Earth's atmosphere...
We report on a study about some characteristics of muon production during the development of extende...
Extensive Air Showers are still the only source of information on primary cosmic rays and their inte...
In view of the interpretation of data collected by large, deep underground experiments in terms of p...
The particle showers produced in the atmosphere due to the interactions of primary cosmic particles ...