Localized Helioseismic Constraints on Solar Structure

Preprint

13 June 1997

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9702075

Abstract

Localized differences between the real sun and standard solar models are shown to be small. The sound speeds of the real and the standard model suns typically differ by less than 0.3% in the solar core.

Keywords

HELIOSEISMIC CONSTRAINTS
LOCALIZED HELIOSEISMIC
LOCALIZED DIFFERENCES
STRUCTURE LOCALIZED
SOLAR STRUCTURE
STANDARD MODEL
SOUND SPEEDS
SUNS

All Related Versions

Version 1, 1997-02-07, ArXiv
Version 2, 1997-06-13, ArXiv
Published version: The Astrophysical Journal, 485 (2), L91.

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