How to convert Euler Equations to Lagrangian Form?

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SUMMARY

This discussion focuses on converting the one-dimensional Euler equations of fluid dynamics into Lagrangian form using the mass coordinate h. The original Euler equations are transformed into Lagrangian equations, demonstrating the relationship between Eulerian and Lagrangian time derivatives. Key equations include the conservation of mass and momentum, with specific transformations involving the density ρ and velocity v, leading to the final Lagrangian forms: ∂v/∂t - ∂u/∂h = 0 and ∂u/∂t + ∂p/∂h = 0. The discussion emphasizes the importance of understanding these transformations for fluid mechanics applications.

PREREQUISITES
  • Understanding of one-dimensional Euler equations in fluid dynamics
  • Familiarity with Lagrangian and Eulerian frameworks
  • Knowledge of partial derivatives and chain rule in calculus
  • Basic concepts of fluid mechanics and conservation laws
NEXT STEPS
  • Study the derivation of Lagrangian equations from Euler equations in fluid dynamics
  • Learn about the relationship between Eulerian and Lagrangian time derivatives
  • Explore applications of Lagrangian methods in computational fluid dynamics (CFD)
  • Investigate the implications of mass coordinates in fluid flow analysis
USEFUL FOR

Fluid mechanics students, researchers in computational fluid dynamics, and engineers working on fluid flow simulations will benefit from this discussion.

Mr. Cosmos
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I am not entirely sure how to convert the conservation of mass and momentum equations into the Lagrangian form using the mass coordinate h. The one dimensional Euler equations given by,
[tex]\frac{\partial \rho}{\partial t} + u\frac{\partial \rho}{\partial x} + \rho\frac{\partial u}{\partial x} = 0[/tex]
[tex]\frac{\partial u}{\partial t} + u\frac{\partial u}{\partial x} + \frac{1}{\rho}\frac{\partial p}{\partial x} = 0[/tex]
need to be converted to,
[tex]\frac{\partial v}{\partial t} - \frac{\partial u}{\partial h} = 0[/tex]
[tex]\frac{\partial u}{\partial t} + \frac{\partial p}{\partial h} = 0[/tex]
where the Lagrangian mass coordinate has the relation,
[tex]\frac{\partial h}{\partial x} = \rho[/tex]
and
[tex]v = \frac{1}{\rho}[/tex]
Thanks.
 
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So I played around with the equations and with the aid of my fluid mechanics book I figured it out. One must realize that the Lagrangian time derivative is related to the Eulerian time derivative by,
[tex]\left(\frac{\partial f}{\partial t}\right)_L = \left(\frac{\partial f}{\partial t}\right)_E + \vec{V} \cdot \left(\nabla f\right)[/tex] where f is a flow property like density, pressure, velocity, etc.
Therefore, in one dimension the Euler equations immediately reduce to the Lagrangian equivalent of,
[tex]\frac{\partial \rho}{\partial t} + \frac{1}{v} \frac{\partial u}{\partial x} = 0 \\<br /> \frac{\partial u}{\partial t} + v \frac{\partial p}{\partial x} = 0[/tex] Now realizing that,
[tex]\frac{\partial \rho}{\partial t} = -\frac{1}{v^2} \frac{\partial v}{\partial t}[/tex] and from the partial derivative chain rule,
[tex]\frac{\partial u}{\partial x} = \frac{\partial h}{\partial x} \frac{\partial u}{\partial h} = \frac{1}{v} \frac{\partial u}{\partial h} \\<br /> \frac{\partial p}{\partial x} = \frac{\partial h}{\partial x} \frac{\partial p}{\partial h} = \frac{1}{v} \frac{\partial u}{\partial h}[/tex] Substituting into the the Lagrangian form yields,
[tex]-\frac{1}{v^2} \frac{\partial v}{\partial t} + \frac{1}{v^2} \frac{\partial u}{\partial h} = 0 \\<br /> \frac{\partial u}{\partial t} + v \frac{1}{v} \frac{\partial p}{\partial h} = 0[/tex] or equivalently,
[tex]\frac{\partial v}{\partial t} - \frac{\partial u}{\partial h} = 0 \\<br /> \frac{\partial u}{\partial t} + \frac{\partial p}{\partial h} = 0[/tex] where h is the mass coordinate.
 

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