Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tailJan 1, 2012ยทP. Desiati,A. Lazarianยท 0 min read Cite DOI URLTypeConference paperPublicationAIP Conference ProceedingsLast updated on Jan 1, 2012 ← Influence of hadronic interaction models and the cosmic ray spectrum on the high energy atmospheric muon and neutrino flux Jan 1, 2012Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program Jan 1, 2012 →