We begin with a brief introduction of the cosmic ray energy spectrum and its main features. At energies higher than 105 GeV cosmic rays are detected by the showers they initiate in the atmosphere. We continues with a brief description of the energy spectrum and composition derived from air shower data
Aims.A model to describe cosmic ray spectra in the energy region from 1010 to 1017 eV is suggested ...
The shape of the primary cosmic-ray spectrum at very high energies and its connection with the spect...
The energy spectrum of cosmic rays between 10(16) eV and 10(18) eV, derived from measurements of the...
Extensive air showers are a very unique phenomenon. In the more than six decades since their discove...
Calculations of the longitudinal development of air showers initiated by protons and heavy primaries...
Ultrahigh energy cosmic rays carry information about their sources and the intervening medium apart ...
(Reçu le, accepte ́ le) Abstract. A cosmic ray observatory records individual particles using the a...
We present an introductory lecture on general features of cosmic rays, for non-experts, and some rec...
In this paper we review air shower data related to the mass composition of cosmic rays above 1015 eV...
© CSIRO 2002AbstractAn examination is made of the relationship between the observed energy spectrum ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
The energies of cosmic rays, fully ionized charged nuclei, extend over a wide range up to 1020 eV. A...
Abstract. This paper is intended to be pedagogic. The first part is devoted to a brief exposition of...
A model to describe cosmic ray spectra in the energy region from 100 GeV up to 100 PeV is suggested....
A combined analysis of the energy spectrum and the chemical composition of ultra-high energy cosmic ...
Aims.A model to describe cosmic ray spectra in the energy region from 1010 to 1017 eV is suggested ...
The shape of the primary cosmic-ray spectrum at very high energies and its connection with the spect...
The energy spectrum of cosmic rays between 10(16) eV and 10(18) eV, derived from measurements of the...
Extensive air showers are a very unique phenomenon. In the more than six decades since their discove...
Calculations of the longitudinal development of air showers initiated by protons and heavy primaries...
Ultrahigh energy cosmic rays carry information about their sources and the intervening medium apart ...
(Reçu le, accepte ́ le) Abstract. A cosmic ray observatory records individual particles using the a...
We present an introductory lecture on general features of cosmic rays, for non-experts, and some rec...
In this paper we review air shower data related to the mass composition of cosmic rays above 1015 eV...
© CSIRO 2002AbstractAn examination is made of the relationship between the observed energy spectrum ...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
The energies of cosmic rays, fully ionized charged nuclei, extend over a wide range up to 1020 eV. A...
Abstract. This paper is intended to be pedagogic. The first part is devoted to a brief exposition of...
A model to describe cosmic ray spectra in the energy region from 100 GeV up to 100 PeV is suggested....
A combined analysis of the energy spectrum and the chemical composition of ultra-high energy cosmic ...
Aims.A model to describe cosmic ray spectra in the energy region from 1010 to 1017 eV is suggested ...
The shape of the primary cosmic-ray spectrum at very high energies and its connection with the spect...
The energy spectrum of cosmic rays between 10(16) eV and 10(18) eV, derived from measurements of the...