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- W1497376067 abstract "The cosmic p flux have recently been measured by several balloon experiment but although the measurement was made at hight altitude, the atmospheric p contribution is significant and have to be subtracted. This requires a precise description of the particle interaction and propagation in the atmosphere for p, n and p. Here the secondary atmospheric p and p flux are studied by means of a Monte-Carlo simulation procedure. The calculated flux are compared with the available experimental measurements from sea level up to the top of atmosphere (TOA). The agreement with data are very good at all altitudes, and a new estimation of p flux at balloon altitude is shown. The calculation are extended at higher altitudes up to 10 Earth radii, to study the extension of the quasi-trapped particle belt beyond the atmosphere." @default.
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- W1497376067 date "2003-07-01" @default.
- W1497376067 modified "2023-09-26" @default.
- W1497376067 title "Atmospheric Protons and Antiprotons form Sea Level to Satellite Altitudes" @default.
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