Physics
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974izssr..38.1827v&link_type=abstract
(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Kharkov, Ukrainian SSR, Sept. 25-28, 1973.) Akademiia Nauk SSSR, Izv
Physics
2
Astronomical Models, Neutrinos, Nuclear Reactions, Solar Corpuscular Radiation, Solar Flux, Energy Conversion, Nuclear Transformations, Solar Physics, Tables (Data)
Scientific paper
A method of constructing solar models, which is free from certain inadequacies characteristic of modern methods of constructing stellar models is proposed. The principal characteristics of solar models calculated for six moments of time are tabulated. The neutrino fluxes from neutrino produced by three different reactions are calculated for a given solar model, and the calculated (tabulated) data are analyzed.
Kocharov Grant E.
Levkovskii Aleksey A.
Vasil'ev S. S.
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