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• W2145487037 abstract "We compute cosmic ray (CR) nuclei, proton, antiproton, electron and positron spectra below 1 TeV at Earth by means of a detailed transport description in the galaxy and in the solar system. CR spectra below 10 GeV are strongly modified by charge-sign dependent propagation effects. These depend on the polarity of the solar magnetic field and therefore vary with the solar cycle. The puzzling discrepancy between the low-energy positron fraction measured by PAMELA and AMS-01 is then easily explained by their different data-taking epochs. We reproduce the observed spectra of CR light nuclei within the same galactic and solar-system propagation model." @default.
• W2145487037 created "2016-06-24" @default.
• W2145487037 creator A5018561553 @default.
• W2145487037 date "2013-02-19" @default.
• W2145487037 modified "2023-10-10" @default.
• W2145487037 title "Low Energy Cosmic Ray Positron Fraction Explained by Charge-Sign Dependent Solar Modulation" @default.
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• W2145487037 doi "https://doi.org/10.1103/physrevlett.110.081101" @default.
• W2145487037 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/23473125" @default.
• W2145487037 hasPublicationYear "2013" @default.
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