Calculation of Solar P-mode Oscillation Frequency Splittings Based on a Two-dimensional Solar Model

Simple item page
dc.creatorLi, Linghuai
dc.creatorBasu, Sarbani
dc.creatorSofia, Sabatino
dc.creatorDemarque, Pierre
dc.date2008-10-27
dc.date.accessioned2026-07-07T10:13:36Z
dc.date.available2026-07-07T10:13:36Z
dc.descriptionWe compute the p-mode oscillation frequencies and frequency splittings that arise in a two-dimensional model of the Sun that contains toroidal magnetic fields in its interior.
dc.description4 pages, 3 figures, in proceedings of GONG2008/SOHO XXI: Solar-stellar dynamos as revealed by helio- and asteroseismology, August 11-15, 2008 - Boulder, Colorado
dc.identifierhttps://arxiv.org/abs/0810.4943
dc.identifierhttp://arxiv.org/abs/0810.4943
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/172589
dc.subjectAstrophysics
dc.titleCalculation of Solar P-mode Oscillation Frequency Splittings Based on a Two-dimensional Solar Model
dc.typetext

Files

Collections

arXiv