barotropic | A barotropic fluid is one whose pressure and density are related by an equation of state that does not contain the temperature as a dependent variable. Mathematically, the equation of state can be expressed as p = p(r) or r = r(p). |
compressible | A fluid flow is compressible if its density r changes appreciably (typically by a few percent) within the domain of interest. Typically, this will occur when the fluid velocity exceeds Mach 0.3. Hence, low velocity flows (both gas and liquids) behave incompressibly. |
density, r | The mass of fluid per unit volume. For a compressible fluid flow, the density can vary from place to place. |
incompressible | An incompressible fluid is one whose density is constant everywhere. All fluids behave incompressibly (to within 5%) when their maximum velocities are below Mach 0.3. |
inviscid | Not viscous. |
irrotational | An irrotational fluid flow is one whose streamlines never loop back on themselves. Typically, only inviscid fluids can be irrotational. Of course, a uniform viscid fluid flow without boundaries is also irrotational, but this is a special (and boring!) case. |
laminar (non-turbulent) |
An organized flow field that can be described with streamlines. In order for laminar flow to be permissible, the viscous stresses must dominate over the fluid inertia stresses. |
Mach | Mach number is the relative velocity of a fluid compared to its sonic velocity. Mach numbers less than 1 correspond to sub-sonic velocities, and Mach numbers > 1 correspond to super-sonic velocities. |
Newtonian | A Newtonian fluid is a viscous fluid whose shear stresses are a linear function of the fluid strain rate. Mathematically, this can be expressed as: tij = Kijqp*Dpq, where tij is the shear stress component, and Dpq are fluid strain rate components. |
perfect | A perfect fluid is defined as a fluid with zero viscosity (i.e. inviscid). |
rotational | A rotational fluid flow can contain streamlines that loop back on themselves. Hence, fluid particles following such streamlines will travel along closed paths. Bounded (and hence nonuniform) viscous fluids exhibit rotational flow, typically within their boundary layers. Since all real fluids are viscous to some amount, all real fluids exhibit a level of rotational flow somewhere in their domain. Regions of rotational flow correspond to the regions of viscous losses in a fluid. Inviscid fluid flows can also be rotational, but these are special nonphysical cases. For an inviscid fluid flow to be rotational, it must be set up that way by initial conditions. The amount of rotation (called the velocity circulation) in an inviscid fluid flow is conserved, provided that the fluid is also barotropic and subject only to conservative body forces. This conservation is known as Kelvin's Theorem of constant circulation. |
Stokesian | A Stokesian (or non-Newtonian) fluid is a viscous fluid whose shear stresses are a non-linear function of the fluid strain rate. |
streamline | A path in a steady flow field along which a given fluid particle travels. |
turbulent | A flow field that cannot be described with streamlines in the absolute sense. However, time-averaged streamlines can be defined to describe the average behavior of the flow. In turbulent flow, the inertia stresses dominate over the viscous stresses, leading to small-scale chaotic behavior in the fluid motion. |
viscosity, m | A fluid property that relates the magnitude of fluid shear stresses to the fluid strain rate, or more simply, to the spatial rate of change in the fluid velocity field. Mathematically, this is expressed as: t = m*(dV/dy), where t is the shear stress in the same direction as the fluid velocity V, and y is a direction perpendicular to the fluid velocity direction. |