Several possible methods to distinguish protons and pions in the cosmic radiation at energies of over 100 GeV are discussed. One of these methods based on multiple sampling of ionization losses in an array of gas proportional counters together with a measurement of energy in an ionization calorimeter or momentum in a magnet spectrograph is discussed in greater detail.Fluctuations in ionization losses ("Landau" fluctuations) make the method difficult but not impossible. Experimental results on Landau fluctuations with a variety of incident particles and energies are presented and it is shown that they are in better agreement with the theory of Blunck and Leisegang than with that of Landau.Artificial events in which the sampled ionization los...
A calorimeter-spark chamber system was used to collect data on several hundred proton-nucleus intera...
Differential energy spectra of cosmic ray protons and helium nuclei were measured by an ionization s...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
A balloon-borne detector system for extending the study of cosmic ray composition to the energy regi...
The most probable energy loss in a gaseous medium, as also in other media, was theoretically predict...
The results from a balloon-borne gas Cherenkov counter (threshold 16.5 GeV/nucleon) and an ionizatio...
An ionization spectrometer consisting of a sandwich of iron absorbers and plastic scintillation coun...
The primary cosmic ray proton and He spectra from 50 GeV to 2000 GeV have been measured by an ioniza...
Proton-proton interactions above 100 GeV have been studied in an experiment using cosmic-ray protons...
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and ...
We report new results for the cosmic-ray antiproton-to-proton ratio from 3 to 50 GeV at the top of t...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
The chemical composition cosmic rays as a function of energy in the range of a few GeV/nucleon to so...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
The results of a new balloon borne cosmic ray detector flown from Palestine, TX in Sept., 1982 are d...
A calorimeter-spark chamber system was used to collect data on several hundred proton-nucleus intera...
Differential energy spectra of cosmic ray protons and helium nuclei were measured by an ionization s...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
A balloon-borne detector system for extending the study of cosmic ray composition to the energy regi...
The most probable energy loss in a gaseous medium, as also in other media, was theoretically predict...
The results from a balloon-borne gas Cherenkov counter (threshold 16.5 GeV/nucleon) and an ionizatio...
An ionization spectrometer consisting of a sandwich of iron absorbers and plastic scintillation coun...
The primary cosmic ray proton and He spectra from 50 GeV to 2000 GeV have been measured by an ioniza...
Proton-proton interactions above 100 GeV have been studied in an experiment using cosmic-ray protons...
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and ...
We report new results for the cosmic-ray antiproton-to-proton ratio from 3 to 50 GeV at the top of t...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
The chemical composition cosmic rays as a function of energy in the range of a few GeV/nucleon to so...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
The results of a new balloon borne cosmic ray detector flown from Palestine, TX in Sept., 1982 are d...
A calorimeter-spark chamber system was used to collect data on several hundred proton-nucleus intera...
Differential energy spectra of cosmic ray protons and helium nuclei were measured by an ionization s...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...