Example of distribution of gas density (first and third rows) and velocity (second and bottom rows) in the model with instantaneous (left panels) and rotation-averaged (right panels) energy input for a homogeneous nucleus. The flow streamlines are shown in black in the panels with the distribution of gas velocity. Computations were made for r_h = 3.266 (October 1, 2014). The Sun is in the Y = 0 plane at 41° from the +X axis in an anticlockwise direction.