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Modelling solar atmospheric gravity oscillation modes

✍ Scribed by B. Pintér


Book ID
101697894
Publisher
John Wiley and Sons
Year
2008
Tongue
English
Weight
493 KB
Volume
329
Category
Article
ISSN
0004-6337

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The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the solar atmosphere. We study the impact of three-flavor oscillations on the solar atmosphere neutrino fluxes observable at Earth. We find that peculiar matter oscillation effects in the Sun do exist, b