Detecting deep axisymmetric toroidal magnetic fields in stars: The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field - Dhouib, H.; Mathis, S.; Bugnet, L.; Van Reeth, T.; Aerts, C. (Astronomy and astrophysics (Berlin), 2022)
Keywords: Astrophysics; Physics; waves; methods: analytical; stars: oscillations; stars: magnetic field; magnetohydrodynamics (MHD); stars: rotation