Free surface

Flatness refers to the shape of a liquid's free surface. On Earth, the flatness of a liquid is a function of the curvature of the planet, and from trigonometry, can be found to deviate from true flatness by approximately 19.6 nanometers over an area of 1 square meter, a deviation which is dominated by the effects of surface tension. This calculation uses Earth's mean radius at sea level, however a liquid will be slightly flatter at the poles. Over large distances or planetary scale, the surface of an undisturbed liquid tends to conform to equigeopotential surfaces; for example, mean sea level follows approximately the geoid. ==Waves==

If the free surface of a liquid is disturbed, waves are produced on the surface. These waves are not elastic waves due to any elastic force; they are gravity waves caused by the force of gravity tending to bring the surface of the disturbed liquid back to its horizontal level. Momentum causes the wave to overshoot, thus oscillating and spreading the disturbance to the neighboring portions of the surface. Capillary ripples are damped both by sub-surface viscosity and by surface rheology. == Rotation ==

If a liquid is contained in a cylindrical vessel and is rotating around a vertical axis coinciding with the axis of the cylinder, the free surface will assume a parabolic surface of revolution known as a paraboloid. The free surface at each point is at a right angle to the force acting at it, which is the resultant of the force of gravity and the centrifugal force from the motion of each point in a circle. Since the main mirror in a telescope must be parabolic, this principle is used to create liquid-mirror telescopes. Consider a cylindrical container filled with liquid rotating in the z direction in cylindrical coordinates, the equations of motion are: : \frac{\partial P}{\partial r} = \rho r \omega^2, \quad \frac{\partial P}{\partial \theta} = 0, \quad \frac{\partial P}{\partial z} = -\rho g, where P is the pressure, \rho is the density of the fluid, r is the radius of the cylinder, \omega is the angular frequency, and g is the gravitational acceleration. Taking a surface of constant pressure (dP = 0) the total differential becomes : dP = \rho r \omega^2 dr - \rho g dz \to \frac{dz_\text{isobar}}{dr} = \frac{r \omega^2}{g}. Integrating, the equation for the free surface becomes : z_s = \frac{\omega^2}{2g} r^2 + h_c, where h_c is the distance of the free surface from the bottom of the container along the axis of rotation. If one integrates the volume of the paraboloid formed by the free surface and then solves for the original height, one can find the height of the fluid along the centerline of the cylindrical container: : h_c = h_0 - \frac{\omega^2 R^2}{4g}. The equation of the free surface at any distance r from the center becomes : z_s = h_0 - \frac{\omega^2}{4g} (R^2 - 2 r^2). If a free liquid is rotating about an axis, the free surface will take the shape of an oblate spheroid: the approximate shape of the Earth due to its equatorial bulge. ==Related terms==

• In hydrodynamics, the free surface is defined mathematically by the free-surface condition, that is, the material derivative on the pressure is zero: \frac{Dp}{Dt} = 0. • In fluid dynamics, a free-surface vortex, also known as a potential vortex or whirlpool, forms in an irrotational flow, for example when a bathtub is drained. • In naval architecture and marine safety, the free surface effect occurs when liquids or granular materials under a free surface in partially filled tanks or holds shift when the vessel heels. • In hydraulic engineering a free-surface jet is one where the entrainment of the fluid outside the jet is minimal, as opposed to submerged jet where the entrainment effect is significant. A liquid jet in air approximates a free surface jet. • In fluid mechanics a free surface flow, also called open-channel flow, is the gravity driven flow of a fluid under a free surface, typically water flowing under air in the atmosphere. ==See also==