2008/10/31 by K. Belkacem, R. Samadi, M. J. Goupil +4 · 1 citation
Physics and Astronomy · #Amplitude #Astro and Planetary Science #Context (archaeology) #Convection #Core (optical fiber) #Excitation #Geology #Geophysics #Inner core #Mechanics #Optics #Physics #Quantum mechanics #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:200810827
18 pages, 19 figures, accepted for publication in Astronomy & Astrophysics
arxiv created 2008/11/28 · openalex publication_date 2008/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
Context. Detection of solar gravity modes remains a major challenge to our understanding of the inner parts of the Sun. Their frequencies would enable the derivation of constraints on the core physical properties, while their amplitudes can put severe constraints on the properties of the inner convective region.