Isotopic composition of cosmic-ray sources

Simple item page
dc.creatorMoskalenko, Igor V.
dc.creatorStrong, Andrew W.
dc.creatorPorter, Troy A.
dc.date2007-08-15
dc.date.accessioned2026-07-07T12:46:00Z
dc.date.available2026-07-07T12:46:00Z
dc.descriptionWe use the GALPROP code and the Advanced Composition Explorer (ACE) data to derive the cosmic ray (CR) isotopic composition at the sources. The composition is derived for two propagation models, diffusive reacceleration and plain diffusion. We show that the compositions derived assuming these two propagation models are different. We also compare the isotopic composition at the sources with the latest solar composition.
dc.description4 pages, 2 figures. Contribution to the 30th ICRC, Merida, Mexico, 2007 (final version)
dc.identifierhttps://arxiv.org/abs/0708.1974
dc.identifierhttp://arxiv.org/abs/0708.1974
dc.identifierProc. 30th ICRC (Merida), 2, 129-132 (2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/221234
dc.subjectAstrophysics
dc.titleIsotopic composition of cosmic-ray sources
dc.typetext

Files

Collections

arXiv