Energy spectra for primary cosmic rays C-Fe above 20 GeV/n were measured on a balloon flight from Greenville S.C. in June 1982 with a hybrid electronic counter-emulsion chamber experiment. Fluxes above the atmosphere appear in general agreement with previously published values. The heavy events included in this data will be used along with the JACEE passive chamber data to provide a heavy composition direct measurement from 10 to the 12th power to approximately 10 to the 15th power eV total energy
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
To investigate the chemical composition of primary cosmic rays, several emulsion chambers were expos...
The composition and energy spectra of charge groups (C - 0), (Ne - S), and (Z approximately 17) abo...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The study of the cosmic ray abundances beyond 20 GeV/n provides additional information on the propag...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
The chemical composition cosmic rays as a function of energy in the range of a few GeV/nucleon to so...
We present new measurements of heavy cosmic-ray nuclei at high energies per- formed during the first...
We study the spectrum and average mass composition of cosmic rays with primary energies between 1017...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
Based on the air shower data, the chemical composition of the primary cosmic rays in the energy rang...
Experimental results from the balloon borne ionization spectrometer have enabled the extension of th...
Direct measurements on cosmic ray protons through iron above about 1 TeV/amu have been performed in ...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
To investigate the chemical composition of primary cosmic rays, several emulsion chambers were expos...
The composition and energy spectra of charge groups (C - 0), (Ne - S), and (Z approximately 17) abo...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The study of the cosmic ray abundances beyond 20 GeV/n provides additional information on the propag...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
The chemical composition cosmic rays as a function of energy in the range of a few GeV/nucleon to so...
We present new measurements of heavy cosmic-ray nuclei at high energies per- formed during the first...
We study the spectrum and average mass composition of cosmic rays with primary energies between 1017...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
Based on the air shower data, the chemical composition of the primary cosmic rays in the energy rang...
Experimental results from the balloon borne ionization spectrometer have enabled the extension of th...
Direct measurements on cosmic ray protons through iron above about 1 TeV/amu have been performed in ...
We show that the simplest assumptions for the dynamics of particle production allow us to understand...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
To investigate the chemical composition of primary cosmic rays, several emulsion chambers were expos...