An Energy-Theory for the Propagation of Gravity Currents

摘要: The problem of the propagation a gravity (density) current, with initial configuration: density p2 in region \(0 < X + \infty \),\( - y \), 0 z H and \({p_1} = {p_2} \delta p\) \( 0\), rigidly bounded at z=0, (Fig. 1(a)) is approached using Green Dalu mesoscale energetics theory (4).