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  1. No Access

    Article

    The energy dependence of the leading nucleon distribution and the evolution of the nucleonic cosmic ray component in the atmosphere

    We show that in order to obtain a fairly accurate description of the nucleonic component of cosmic ray at sea level the energy dependence of the leading nucleon distribution has to be taken into account. By re...

    J. Bellandi FO, S. Q. Brunetto… in Zeitschrift für Physik C Particles and Fie… (1991)

  2. No Access

    Article

    Solution of the one-dimensional diffusion equation for the hadronic cosmic-ray component in the atmosphere

    We solve the one-dimensional diffusion equation for the hadronic cosmic-ray component in the atmosphere assuming for the interaction mean free path a ln2 E-dependence on the energy and comparing w...

    J. Bellandi Fo, S. Q. Brunetto, J. A. Chinellato, R. J. M. Covolan… in Il Nuovo Cimento C (1991)

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    Article

    Elasticity and the nucleon energy spectrum in the atmosphere

    The nucleon intensity in the atmosphere is calculated with a In2(E) energy dependence of the inelastic nucleon-air cross-section and an arbitrary elasticity distribution. A good agreement with the measured nucleo...

    J. Bellandi F., J. Dias de Deus, J. A. Chinellato… in Il Nuovo Cimento A (1965-1970) (1989)