The GYRE Forums

Hi, Aleksey? Calculating the overlap integral Q_nl directly from the displacement eigenfunctions will inevitably suffer from the numerical inaccuracies, especially for high order g-modes. One way to circumvent the problem is to directly use the Eulerian perturbation of gravitation potential (see eq....

Hi, Abdel In the long run, GYRE will be able to model the tidal effect on stellar oscillations. For now, if you want to study free oscillations, you can just use stellar structure models from single or binary star evolution of MESA and feed them into GYRE assuming the effect of tides is negligible. ...

Hi, Rich
Is it possible to add the coefficients of Hough function as a combination of spherical harmonics
to the mode or summary file? It is interesting to use them to calculate mode visibility for g modes.
Thanks!

best regards,
Zhao