We present a systematical analysis of uncertainties in the helioseismological determination of quantities characterizing the solar structure. We discuss the effect of errors on the measured frequencies, the residual solar model dependence and the uncertainties of the inversion method. We find Y-ph = 0.238 - 0.259, R-b/R. = 0.708 - 0.714 and rho(b) = (0.185 - 0.199) gr/cm(3) (the index b refers to the bottom of the convective envelope). In the interval 0.2 < R/R. < 0.65, the quantity U = P/rho is determined with and accuracy of +/-5 parts per thousand or better. The predictions of a few recent solar model calculations are compared with helioseismological results. (C) 1997 Elsevier Science B.V.
Helioseismology and standard solar models
DEGL'INNOCENTI, SCILLA;
1997-01-01
Abstract
We present a systematical analysis of uncertainties in the helioseismological determination of quantities characterizing the solar structure. We discuss the effect of errors on the measured frequencies, the residual solar model dependence and the uncertainties of the inversion method. We find Y-ph = 0.238 - 0.259, R-b/R. = 0.708 - 0.714 and rho(b) = (0.185 - 0.199) gr/cm(3) (the index b refers to the bottom of the convective envelope). In the interval 0.2 < R/R. < 0.65, the quantity U = P/rho is determined with and accuracy of +/-5 parts per thousand or better. The predictions of a few recent solar model calculations are compared with helioseismological results. (C) 1997 Elsevier Science B.V.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
