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The Standard Solar Model
Published online by Cambridge University Press: 12 April 2016
Abstract
The main features of standard solar models, the logic of the calculations, and some of the important results concerning solar neutrinos experiments are given. The input parameters that cause the greatest uncertainties in the calculated neutrino fluxes are the nuclear rection rates, the chemical abundances, the radiative opacity, and the equation of state. This article is based, with permission of the publisher, on Chapters 1 and 4 of Neutrino Astrophysics by J. N. Bahcall, Cambridge University Press (1989).
- Type
- Part 1: Solar Modelling
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- Copyright © Kluwer 1990