DJL equations: Difference between revisions
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The Dubreil-Jacotin-Long (DJL) equation is derived from the steady Euler equations. The result is a single equation for the isopycnal displacement <math>\eta</math>. Here are a few cases: | The Dubreil-Jacotin-Long (DJL) equation is derived from the steady, incompressible Euler equations. The result is a single, non-linear equation for the isopycnal displacement <math>\eta</math>. Here are a few cases: | ||
== Boussinesq with constant background current <math>U_0</math> == | == Boussinesq with constant background current <math>U_0</math> == | ||
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<math>\nabla^2 \eta + \frac{N^2(z-\eta)}{U_0^2}\eta = 0</math> | <math>\nabla^2 \eta + \frac{N^2(z-\eta)}{U_0^2}\eta = 0</math> | ||
where <math> N^2(z) = - | where <math> N^2(z) = -g\frac{\bar{\rho}'(z)}{\rho_0}</math>. <math>\bar{\rho}(z)</math> is the far upstream density profile, <math>\rho_0</math> is a constant reference density ,and <math>g</math> is the acceleration due to gravity. | ||
== Boussinesq with non-constant background current <math>U(z)</math> == | == Boussinesq with non-constant background current <math>U(z)</math> == | ||
<math>\nabla^2 \eta + \frac{N^2(z-\eta)}{U(z-\eta) | <math>\nabla^2 \eta + \frac{N^2(z-\eta)}{U^2(z-\eta)}\eta + \frac{U'(z-\eta)}{U(z-\eta)}\left[1- \left(\eta_x^2 +(1-\eta_z)^2\right)\right] = 0</math> | ||
Again, <math> N^2(z) = -g\frac{\bar{\rho}'(z)}{\rho_0}</math>. | |||
== Non-Boussinesq constant background current <math>U_0</math> == | == Non-Boussinesq constant background current <math>U_0</math> == | ||
<math>\nabla^2\eta + \frac{N^2(z-\eta)}{U_0^2}\eta +\frac{N^2(z-\eta)}{2g}\left[\eta_x^2 +\eta_z(\eta_z-2)\right] =0</math> | <math>\nabla^2\eta + \frac{N^2(z-\eta)}{U_0^2}\eta +\frac{N^2(z-\eta)}{2g}\left[\eta_x^2 +\eta_z(\eta_z-2)\right] =0</math> | ||
where <math> N^2(z) = -g\frac{\bar{\rho}'(z)}{\bar{\rho}(z)}</math> | where <math> N^2(z) = -g\frac{\bar{\rho}'(z)}{\bar{\rho}(z)}</math>. |
Latest revision as of 09:55, 27 October 2011
The Dubreil-Jacotin-Long (DJL) equation is derived from the steady, incompressible Euler equations. The result is a single, non-linear equation for the isopycnal displacement . Here are a few cases:
Boussinesq with constant background current
where . is the far upstream density profile, is a constant reference density ,and is the acceleration due to gravity.
Boussinesq with non-constant background current
Again, .
Non-Boussinesq constant background current
where .