Observations on the abundance of nitrogen in the primary cosmic radiation
Primary cosmic ray nitrogen nuclei intensity and spectrum measured by balloons and Pioneer 8 space probe, obtaining abundance difference from solar atmosphere
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Primary cosmic ray nitrogen nuclei intensity and spectrum measured by balloons and Pioneer 8 space probe, obtaining abundance difference from solar atmosphere
Primary cosmic radiation abundance measurements on iron and heavier nuclei, using Cerenkov counter on balloon flights
Temporal variation in flux of primary heavy nuclei in primary cosmic radiation at solar maximum conditions
Flux observation of heavy primary cosmic radiation in explorer vii satellite-borne instrumentation
Positron-electron ratio in primary cosmic radiation measured as function of energy - cosmic ray origin
Ratio of electron to positrons in primary cosmic radiation investigated by balloon-borne instrument over Ft. Churchill
Primary cosmic ray charge and energy spectra determination for helium through neon during solar minimum
Primary cosmic ray charge and energy spectra for helium through oxygen during 1965 minimum solar modulation effect
Trans-iron nuclei flux in primary cosmic radiation determined through high altitude balloon exposure of interleaved layers of nuclear photographic emulsion and plastic detectors
Charge and energy spectra of primary cosmic rays made with large area Cerenkov scintillation counter on baloon flights - heavier than iron nuclei
Primary cosmic ray origin and acceleration and antiproton energy spectrum, using Fokker-Planck diffusion equation
Charge composition of primary electron component from balloon-borne magnetic spectrometer measurements, discussing energy dependence of positron-electron ratio in primary cosmic radiation
Isotopic composition and energy spectrum of low energy helium nuclei in primary cosmic radiation
Energy spectra of carbon and oxygen nuclei in primary cosmic radiation, comparing results to earlier measurements and satellite observation
Fluorine nuclei in primary cosmic radiation identified by counter telescope measurements on Pioneer 8 spacecraft
A search for anti-alpha-particles in the primary cosmic radiation has been carried out, and a new upper limit for these particles in the range 0.2-4.3 GeV per nucleon has been obtained. At the 95 per cent confidence level the upper limit is found to be 0.14 per cent of the alpha-particle flux. The instrument used for this purpose is a magnetic spectrometer employing spark chambers for determining particle trajectories and time-of-flight measurement for the rejection of upward-moving particles. Implications of these results for various models of the sources of cosmic radiation are discussed.
Energy dependence of lithium, beryllium and boron abundance in primary cosmic radiation observed at Fort Churchill
Satellite investigation of time variations of heavy nuclei in the primary cosmic radiation