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- W2027706724 abstract "The properties of solar energetic particles (SEPs) in solar flares are studied through remote imaging in the radio, hard X-ray, and γ-ray energy ranges. However, the heliospheric SEP populations are observed only in situ by satellite measurements, which drastically limits our understanding of their spatial and temporal variations. Can those SEP populations be remotely imaged, as are the solar SEPs? We consider two possibilities for detecting faint γ-ray emission from SEP interactions with solar wind (SW) ions. First, the 6.13 and 4.44 MeV γ-ray lines of 16O and 12C, respectively, produced by the interactions of the SEPs from a large low-energy (E 300 MeV protons captured in strong coronal loops, but we suggest that the observed emission was due to SEP-SW collisions following shock acceleration on open field lines." @default.
- W2027706724 created "2016-06-24" @default.
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- W2027706724 date "2008-03-01" @default.
- W2027706724 modified "2023-10-18" @default.
- W2027706724 title "Remote Sensing of Gamma‐Ray Emission from Solar Energetic Proton Interactions with the Solar Wind" @default.
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- W2027706724 doi "https://doi.org/10.1086/526416" @default.
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