General Earth and Planetary Sciences; General Environmental Science; General Engineering; General Materials Science
Abstract :
[en] The rotation and mixing of the core of the Sun, which control solar evolution and the present-day Sun, remain poorly constrained in spite of their crucial importance. The detection of a few gravity (g)-modes should enable the helioseismic probing of the solar core much like that already achieved for the outer radiative zone and convection zone with pressure (p)-modes.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Leibacher, John ; National Solar Observatory, LPL/University of Arizona, IAS/Université Paris-Saclay
Buldgen, Gaël ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie ; Département d’Astronomie, Université de Genève
García, Rafael A. ; Université Paris–Saclay. Université Paris–Cité, CEA, CNRS, AIM: ORCID 0000-0002-8854-3776
Gizon, Laurent ; Max Planck Institute for Solar System Research: ORCID 0000-0001-7696-8665
Scherrer, Philip ; Stanford University
Language :
English
Title :
Probing the Structure and Dynamics of the Solar Core with Gravity Modes
