The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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Rossby waves in a stratified solar model exhibit two distinct wave cavities with radiative modes showing nearly constant radial vorticity throughout the convection zone.
citing papers explorer
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Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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Effects of density stratification on Rossby waves in deep atmospheres
Rossby waves in a stratified solar model exhibit two distinct wave cavities with radiative modes showing nearly constant radial vorticity throughout the convection zone.