Composition and energy spectra of cosmic-ray primaries in the energy range 1013–1015 eV/particle observed by Japanese–Russian joint balloon experiment

By A. V. Apanasenko, V. A. Sukhadolskaya, V. A. Derbina, M. Fujii, V. Galkine, G. G. Getsov, M. Hareyama, M. Ichimura, S. Ito, E. Kamioka and 42 more. 2001

135 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/5bd1d6cf6fd92852c0491542bce02dfd6b6ecd64

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Citations in the corpus

• COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE FIRST CREAM FLIGHT (2011, background): “Above this energy the composition and energy spectra are not accurately known, although there have been some pioneering measurements (Müller et al. 1991; Asakimori et al. 1998; Apanasenko et al. 2001).”
• The All-Particle Spectrum of Primary Cosmic Rays in the Wide Energy Range from 1014 to 1017 eV Observed with the Tibet-III Air-Shower Array (2008, methodology): “PROTON satellite (Grigorov et al. 1971), AKENO (Nagano et al. 1984),JACEE (Asakimori et al. 1998),RUNJOB (Apanasenko et al. 2001). same detector configuration as the Tibet-III array with use of Epics code (ver.”