Assessing the validity of the anelastic and Boussinesq approximations to model solar inertial modes

TL;DR

This study evaluates the validity of common approximations in modeling solar inertial modes, finding that the anelastic approximation accurately captures these modes while the Boussinesq approximation does not.

Contribution

It demonstrates that the anelastic approximation is suitable for modeling solar inertial modes, whereas the Boussinesq approximation introduces significant inaccuracies, especially in non-toroidal modes.

Findings

Anelastic and compressible models produce nearly identical eigenmodes.

Boussinesq approximation results in significantly different eigenmodes.

Anelastic approximation reduces computational cost without loss of accuracy.

Abstract

Global-scale inertial modes of oscillations have been recently observed on the Sun. They might play an important dynamic and diagnostic role for the Sun. This work aims to assess the validity of simplifying assumptions in the equation of continuity, which have often been used in the linear models of solar inertial modes. We compute the linear eigenmodes of the Sun's convection zone in the inertial frequency range using the Dedalus code. This single framework enables us to compare the sensitivity of the modes to different model setups, such as the compressible setup and the Boussinesq and anelastic approximations. We consider both the cases of uniform rotation and solar differential rotation (as given by helioseismology). We find that the compressible and anelastic models have almost identical eigenmodes under uniform rotation and solar differential rotation. On the other hand, the absence of density stratification in the Boussinesq model results in significantly different eigenmodes under these setups. The differences are most prominent for the non-toroidal modes with significant radial motions mainly due to the absence of the compressional $\beta$ effect. The anelastic approximation simplifies the calculations and reduces the numerical cost without affecting the solar inertial modes. The Boussinesq or incompressible approximations cannot be used to model the solar inertial modes accurately. Given the strong influence of differential rotation on the eigenmodes, an acceptable setup is to use the anelastic approximation together with the solar differential rotation.