Meridional cuts (x, θ) showing the leading order terms, for solar rotation, of the latitudinal σ₁ξ_θ and azimuthal σ₁ξ_ϕ flow velocity, the relative normal displacement ξ_x/H_p, the relative pressure p′/p, and density ρ′/ρ perturbations (from left to right respectively, as labelled in the colour bar) for the (ℓ,m, k) = (3, 3, 1) mode and for n = 1.49 (top) and n = 1.51 (bottom). H_p is the pressure height scale. The radial dependence of all the quantities has been normalised consistently so that at phase 0, a dimensionless velocity of 1 on this scale corresponds to a velocity of 1 m s⁻¹ on the Sun.