Helioseismic Constraints on the Properties of the Solar Core and on the Solar Neutrino Fluxes
نویسنده
چکیده
The temperature and the abundance of hydrogen in the Sun's interior are estimated by the method of`secondary' inversion of solar oscillation frequencies. In this method, the equations of state and thermal balance are used in addition to the hydrostatic equations. The temperature of the solar core estimated from the current helioseismic data is slightly higher than in the standard solar model, that favors the MSW solution of the solar neutrino problem. We discuss the technique and the uncertainties of the helioseismic estimates.
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تاریخ انتشار 2007