Rate of energy dissipation Ė_ij as a function of ϕ′ in a few selected parallels, for the n = 1.5 polytropic case ΔR₁/R₁ = 0.03, ν = 0.003  day^-1, ρ = 8.66 × 10^-7 g cm^-3, orbital period P = 10 days (a = 40.62   R_⊙), and β₀ = 1.2. The top curve shows results for the stellar equator, and following curves from top to bottom correspond to parallels with θ′ ≈ 81°, 73°, 64°, 55°, 46°, 38°, 29°, and 20°. Calculations with β₀ = 2.0 yield identical curves, but the Ė_ij values are higher for by  ~ 1.5 mag.