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Simple technique for determining the mean lifetime of the cosmic ray μ meson
American Journal of Physics, 1978A single scintillation counter is used for determining the lifetime of cosmic ray μ mesons. The experimental arrangement has a greater detection rate and a higher detection efficiency than the conventional multidetector delayed coincidence technique.
A. Owens, A. E. Macgregor
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The correlation of two atmospheric Cerenkov techniques for studying cosmic-ray shower development
Journal of Physics G: Nuclear Physics, 1981A comparison of the lateral distribution function and the pulse time profile of Cerenkov light from individual cosmic-ray showers shows good correlation between these parameters for showers with sizes around 106 particles at sea level. This is as would be expected if both parameters reflect the pattern of shower development in the atmosphere.
J D Kuhlmann +5 more
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New cosmic ray radiosonde techniques
Journal of the Franklin Institute, 1946S A, KORFF, B, HAMERMESH
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1978
An instrument, the Caltech High Energy Isotope Spectrometer Telescope (HEIST), has been developed to measure isotopic abundances of cosmic ray nuclei in the charge range 3 ≤ Z ≤ 28 and the energy range between 30 and 800 MeV/nuc by employing an energy loss -- residual energy technique.
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An instrument, the Caltech High Energy Isotope Spectrometer Telescope (HEIST), has been developed to measure isotopic abundances of cosmic ray nuclei in the charge range 3 ≤ Z ≤ 28 and the energy range between 30 and 800 MeV/nuc by employing an energy loss -- residual energy technique.
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Markov stochastic technique to determine galactic cosmic ray sources distribution
Journal of Astrophysics and Astronomy, 2010A new numerical model of particle propagation in the Galaxy has been developed, which allows the study of cosmic-ray production and propagation in 2D. The model has been used to solve cosmic ray diffusive transport equation with a complete network of nuclear interactions using the time backward Markov stochastic process by tracing the particles ...
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A Markov chain Monte Carlo technique for Galactic cosmic-ray physics
2009We implemented a Markov Chain Monte Carlo technique to estimate the probability-density functions of the cosmic-ray transport and source parameters in a diffusion model. From the measurement of the B/C ratio and radioactive cosmic-ray clocks, we calculate their probability density functions, with a special emphasis on the halo size L of the Galaxy and ...
Putze, A., Maurin, D., Derome, L.
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Galactic factories of cosmic-ray electrons and positrons
Physical Review D, 2021Carmelo Evoli +2 more
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