Unsteady top-hat line-plume balances

Use half-width $b$, upward speed $w$, constant inertial reference density $R$, and positive buoyant reduced gravity $g^{\prime }$. Half-section fluxes are $Q=Rbw$, $M=Rb{w}^2$ and $F=R{g}^{\prime }bw$. With two-sided entrainment $u_e=\alpha w$, the Boussinesq balances areFull-width fluxes are twice these definitions. The shape coefficients differ from triangular transverse profiles, so their unsteady balances cannot be used unchanged here.

In a homogeneous ambient fluid, the displayed nonsteady power-law ansatz solves the unsteady top-hat line-plume balances for $\tau =t+t_{\ast }>0$. It gives $Q=R\alpha z^2/(3\tau )$, $M=2R\alpha z^3/(9{\tau }^2)$ and $F=2R\alpha z^3/(9{\tau }^3)$. The solution is singular at zero age and carries zero source flux at its unshifted ideal origin. It describes a separable branch away from a source; a finite-width boundary, virtual-origin shift or matching region is needed to supply nonzero physical source flux. It is distinct from the steady constant-flux line plume, whose top-hat half-width grows as $\alpha z$.