No CrossRef data available.
Article contents
A Seismic Model of the Solar Convective Envelope
Published online by Cambridge University Press: 08 February 2017
Abstract
We determine the structure of the solar convective envelope by solving the basic equations for mass conservation and hydrostatic equilibrium with the imposition of the sound-speed profile determined from helioseismology and the equation of state. The solution is required to match with the structure of the radiative core, which is also determined with the imposition of the sound speed profile. The helium abundance is obtained as a part of the solutions.
- Type
- II. Solar Convection and Variation of Irradiance
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 81 - 84
- Copyright
- Copyright © Kluwer 1998