High energy neutrino production by cosmic ray interactions in the Sun
1996 (English)In: PHYSICAL REVIEW D, ISSN 0556-2821, Vol. 54, no 7, 4385-4392 p.Article in journal (Refereed) Published
The flux of neutrinos originating from cosmic ray interactions with matter in the Sun has been calculated based on Monte Carlo models for high energy particle interactions. The resulting flux at the Earth (within the Sun's solid angle) is higher than the
Place, publisher, year, edition, pages
1996. Vol. 54, no 7, 4385-4392 p.
ATMOSPHERIC NEUTRINOS; OSCILLATIONS; MATTER; SPECTROSCOPY; SPECTRUM; PHYSICS; SEARCH; MODEL
IdentifiersURN: urn:nbn:se:uu:diva-26767OAI: oai:DiVA.org:uu-26767DiVA: diva2:54661
Addresses: Ingelman G, UNIV UPPSALA, DEPT RADIAT SCI, BOX 535, S-75121 UPPSALA, SWEDEN. DESY, D-22603 HAMBURG, GERMANY.2008-05-252008-05-252011-01-15