Open AccessEffects of errors in the solar radius on helioseismic inferences
Author(s) -
Basu Sarbani
Publication year - 1998
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1998.01690.x
Subject(s) - physics , solar radius , radius , helioseismology , convection zone , standard solar model , astrophysics , systematic error , equation of state , computational physics , opacity , oscillation (cell signaling) , solar physics , helium , optics , solar wind , coronal mass ejection , solar neutrino , statistics , thermodynamics , plasma , atomic physics , stars , computer security , mathematics , computer science , genetics , biology , neutrino oscillation , quantum mechanics , magnetic field , nuclear physics , neutrino
Frequencies of intermediate‐degree f modes of the Sun seem to indicate that the solar radius is smaller than what is normally used in constructing solar models. We investigate the possible consequences of an error in radius on results for solar structure obtained using helioseismic inversions. It is shown that solar sound speed will be overestimated if oscillation frequencies are inverted using reference models with a larger radius. Using solar models with a radius of 695.78 Mm and new data sets, the base of the solar convection zone is estimated to be at a radial distance of 0.7135 ± 0.0005 of the solar radius. The helium abundance in the convection zone as determined using models with an OPAL equation of state is 0.248 ± 0.001, where the errors reflect the estimated systematic errors in the calculation, the statistical errors being much smaller. Assuming that the OPAL opacities used in the construction of the solar models are correct, the surface Z / X is estimated to be 0.0245 ± 0.0006.