Solar Modulation Effect on the Cosmic-Ray Proton Spectra Measured by BESS

Physics

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Scientific paper

We have measured cosmic-ray proton and helium fluxes under the residual atmospheric depth of 5 g/cm2 by the BESS spectrometer launched from Lynn Lake, Manitoba, Canada from 1997 to 2000. By using realistic estimation of the atmospheric secondary protons, we obtained the precise primary fluxes at the top of the atmosphere (TOA) in a kinetic energy region of 0.2 20 GeV/nucleon. The solar modulation effects were observed in the obtained fluxes.

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