Input data

Direct solver

  • Adiabatic pulsation equations
  • Coriolis force projected on a single spherical harmonic
  • Radial order identification using the Eckart-Scuflaire-Osaki-Takata scheme

Perturbative

  • Chandrasekhar-Milne expansion from a one-dimensional stellar model, up to P2P_2 Legendre polynomial
  • Coupling between different degrees of modes through the
  • Toroidal backcoupling through the Coriolis force

Not supported

  • Automatic regridding (requires improvements to the interpolation methods)
  • Non-adiabatic calculations
  • Full 2D stellar models
  • Traditional approximation of rotation