2008/03/27 by S. Mathur, A. Eff‐Darwich, A. Eff-Darwich +3
Physics and Astronomy · #Astro and Planetary Science #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20078839
Accepted for publication in A&A, 8 pages, 11 figures
arxiv created 2008/03/27 · openalex publication_date 2008/04/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
Context. The dynamics of the solar core cannot be properly constrained through the analysis of acoustic oscillation modes. Gravity modes (g modes) are necessary to understand the structure and dynamics of the deepest layers of the Sun. Through recent progress on the observation of these modes – both individually and collectively – new information is available to contribute to inferring the rotation profile inside the nuclear burning core.