MHD models predict that above 10 keV the solar magnetic field collimates plasma into high-latitude lobes, producing a factor of ~2 ENA enhancement at 80 keV that IMAP can detect.
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Prediction for IMAP: Revealing the Role of the Solar Magnetic Field in the Heliotail
MHD models predict that above 10 keV the solar magnetic field collimates plasma into high-latitude lobes, producing a factor of ~2 ENA enhancement at 80 keV that IMAP can detect.