For steady inviscid flow, pressure, kinetic energy density, and conservative potential are constant along a streamline.
In a steady adiabatic inviscid fluid with a conservative body force, the Bernoulli invariant is the displayed specific energy, constant along each streamline. Dotting the Euler equations with velocity and using the specific enthalpy identity gives . In ideal magnetohydrodynamics, magnetic work need not vanish; the planar ideal-MHD Bernoulli invariant includes the corresponding electromagnetic correction.
A slowly varying, steady, inviscid channel flow has constant discharge per unit width and the displayed Bernoulli equation. The bed-height function of depth has its maximum at , where the Froude number is one. At a nondegenerate critical crest, a differentiable profile changes between the subcritical flow and supercritical flow branches. With subcritical upstream squared Froude number and upstream depth , the shock-free supercritical downstream depth is .
With the streamfunction convention , constant scalar vorticity gives . For steady inviscid constant-density flow without body force, this integrates to
throughout a connected fluid region. Reversing the streamfunction convention changes the sign of its term; the declared convention matters.
For steady flow of constant-density fluid in a uniformly rotating frame with conservative body forces, the displayed quantity is constant along each relative streamline. The centrifugal potential contributes the negative quadratic term, and the Coriolis force contributes no work because it is perpendicular to the relative velocity. The result follows by dotting the rotating Euler equations for an inviscid fluid with that velocity.
The Bernoulli function combines pressure, kinetic energy density, and conservative potential.
For steady potential flow over small hills, linearized Bernoulli pressure combines a hydrostatic term with a dynamic term .
If a tank and siphon tube have areas and , the tube outlet is below an inlet initially submerged by , and both free boundaries are at atmospheric pressure, continuity and Bernoulli's equation give
for the free surface to reach the inlet.

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  1. Euler equations for an inviscid fluid
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