Jump to: Page Content, Section Navigation, Site Navigation, Site Search, Account Information, or Site Tools.
|
|
ReportsTracking Solar Gravity Modes: The Dynamics of the Solar Core
Solar gravity modes have been actively sought because they directly probe the solar core (below 0.2 solar radius), but they have not been conclusively detected in the Sun because of their small surface amplitudes. Using data from the Global Oscillation at Low Frequency instrument, we detected a periodic structure in agreement with the period separation predicted by the theory for gravity dipole modes. When studied in relation to simulations including the best physics of the Sun determined through the acoustic modes, such a structure favors a faster rotation rate in the core than in the rest of the radiative zone.
1 DSM/DAPNIA/Service d'Astrophysique, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France.
2 AIMUnité Mixte de Recherche CEACNRSUniversité Paris VIIUMR 7158, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France. 3 Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife, Spain. 4 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, Postfach 1317, 85741 Garching, Germany. 5 Departamento de Edafología y Geología, Universidad de La Laguna, Tenerife, Spain. 6 Département Cassiopée, UMR CNRS 6202, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France. * To whom correspondence should be addressed. E-mail: rafael.garcia{at}cea.fr
The editors suggest the following Related Resources on Science sites:In Science Magazine
|
Science. ISSN 0036-8075 (print), 1095-9203 (online)