“…Since we are interested in a regime in which the interior velocity is much higher than the characteristic Sverdrup velocity, while there are still signs of westward intensification, the parameter δ is taken as 0.1 ( 1). The parameter , which is the nondimensional width of the inertial boundary layer, is related to δ through the relationship 2 δ = U S /β L 2 (Crisciani, 1998), where U S is the Sverdrup velocity, β is the planetary vorticity gradient and L is the horizontal length scale. Using typical values for these parameters, U S ≈ 10 −3 ms −1 , β ≈ 10 −1 m −1 s −1 and L ≈ 10 6 m, we take = 0.05 (< δ).…”