Abstract
We discuss that sufficiently large magnetic fields in the solar radiative zone can significantly alter the spectra and the shapes of helioseismic g-modes. The influence of the magnetic field on the g-mode spectra could be used to probe radiative zone magnetic fields if solar g-modes would be definitively observed.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
