- DSpace Home
- Investigació
- e-prints
- 22 - Física
- View Item
Radiative zone solar magnetic fields and g-modes
|
View
|
| 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)
-
22 - Física [3702]