2003/05/20 by Ching‐Yuan Huang, C. Y. Huang, L. Derome +2 · 1 citation
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #astro-ph
paper · pdf · doi:10.1103/physrevd.68.053008
published as Phys.Rev. D68 (2003) 053008 · 12 pages, 9 figures, 1 table, submitted to Phys. Rev. D
arxiv created 2003/05/20 · openalex publication_date 2003/09/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The atmospheric secondary antiproton flux is studied for detection altitudes extending from sea level up to about three earth radii, by means of a three-dimensional Monte Carlo simulation, successfully applied previously to other satellite and balloon data. The calculated antiproton flux at mountain altitude is found to be in fair agreement with the recent BESS measurements. The flux obtained at balloon altitude is also in agreement with calculations performed in previous studies and used for the analysis of balloon data. The flux at sea level is found to be significant. The antineutron flux is also evaluated. The antiproton flux is prospectively explored up to around 2\ifmmode×\else\texttimes\fi104km from the Earth. The results are discussed in the context of the forthcoming measurements by large acceptance experiments.