Radiative zone solar magnetic fields and g-modes
NAGIOS: RODERIC FUNCIONANDO

Radiative zone solar magnetic fields and g-modes

DSpace Repository

Radiative zone solar magnetic fields and g-modes

Show full item record

View       (261.7Kb)

    
Rashba, Timur I.; Semikoz, Victor B.; Furtado Valle, José Wagner Perfil
This document is a artículoDate2006

Este documento está disponible también en : http://hdl.handle.net/10550/47487
We consider a generalized model of seismic-wave propagation that takes into account the effect of a central magnetic field in the Sun. We determine the g-mode spectrum in the perturbative magnetic field limit using a one-dimensional Magneto-Hydrodynamics (MHD) picture. We show that central magnetic fields of about 600-800 kG can displace the pure g-mode frequencies by about 1%, as hinted by the helioseismic interpretation of GOLF observations.

    Rashba, Timur I. Semikoz, Victor B. Furtado Valle, José Wagner 2006 Radiative zone solar magnetic fields and g-modes Monthly Notices of the Royal Astronomical Society 370 2 845 850
http://dx.doi.org/10.1111/j.1365-2966.2006.10516.x

This item appears in the following Collection(s)

Show full item record

Search DSpace

Advanced Search

Browse

Statistics