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• W2052854913 abstract "New measurements with good statistics will make it possible to observe the time variation of cosmic antiprotons at 1 AU through the approaching peak of solar activity. We report a new computation of the interstellar antiproton spectrum expected from collisions between cosmic protons and the interstellar gas. This spectrum is then used as input to a steady-state drift model of solar modulation, in order to provide predictions for the antiproton spectrum as well as the antiproton/proton ratio at 1 AU. Our model predicts a surprisingly large, rapid increase in the antiproton/proton ratio through the next solar maximum, followed by a large excursion in the ratio during the following decade." @default.
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• W2052854913 date "1999-07-26" @default.
• W2052854913 modified "2023-10-18" @default.
• W2052854913 title "Antiprotons at Solar Maximum" @default.
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• W2052854913 doi "https://doi.org/10.1103/physrevlett.83.674" @default.
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