MEE 309 Engineering Fluid Mechanics Lecture Notes PDF
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These lecture notes cover Engineering Fluid Mechanics (MEE 309). They provide an introduction to fluid kinematics, including concepts like velocity and acceleration fields. The notes also discuss different approaches to analyzing fluid flow, like Eulerian and Lagrangian methods.
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## MEE 309: ENGINEERING FLUID MECHANICS ### Introduction Fluid mechanics is the discipline within applied mechanics that studies the behavior of liquids and gases at rest or in motion. > **Example:** A vast array of problems vary from the study of blood flow in capillaries to the flow of crude o...
## MEE 309: ENGINEERING FLUID MECHANICS ### Introduction Fluid mechanics is the discipline within applied mechanics that studies the behavior of liquids and gases at rest or in motion. > **Example:** A vast array of problems vary from the study of blood flow in capillaries to the flow of crude oil through a pipe. **Fluid mechanics helps explain:** * How a rocket generates thrust without air in outer space. * Why supersonic airplanes are inaudible until they pass you. * How a river flows downstream with significant velocity despite a shallow slope. * How data gathered from model airplanes informs the design of real things. * How aerodynamic car and truck design can improve gas mileage. **This makes fluid mechanics a very important and practical subject.** ### Fluid Kinematics Fluid kinematics is a branch of fluid mechanics that studies position, velocity, and acceleration of a fluid, describing and visualizing its motion without examining the forces that cause it. **In general, fluids flow, creating net motion of molecules from one point in space to another as a function of time.** * A typical portion of fluid contains so many molecules that tracking individual motion is unrealistic. * **Instead**, we consider **fluid particles** that interact with each other and surroundings. * This fluid particle motion can be described using terms of **velocity and acceleration**. ### Particle Location * **At a given instant**, a fluid property (density, pressure, velocity, acceleration) can be described as a function of its location. * This is called a **field representation** of the flow. * Different times result in different representations, so describing a flow requires a function of both spatial coordinates and time ($x$, $y$, $z$, $t$). ### Flow Descriptions There are two general approaches to analyzing fluid mechanics problems. #### Eulerian method * Uses the field concept. * Fluid motion is described by functions of space ($x$, $y$, $z$) and time ($t$) using properties like pressure, density, velocity. * Provides information about the flow at fixed points in space as fluid passes by. #### Lagrangian method * Involves following individual fluid particles as they move and determining changes in their properties over time. * Fluid particles are "tagged" and analyzed. > **Example:** Smoke discharging from a chimney. An Eulerian method fixes a measuring device at the top of the chimney to record temperature as a function of time, observing different particles passing by. A Lagrangian method attaches a device to a specific fluid particle to track its temperature as it moves. **Eulerian method is typically easier to use for experimental and analytical fluid mechanics investigations.** > **However,** there are applications where the Lagrangian approach is more convenient (for example, numerical fluid mechanics calculations involving interactions among particles). ### Velocity Field **One of the most important fluid variables is the velocity field:** $V = u(x, y, z, t)i + v(x, y, z, t)j + w(x, y, z, t)k$ * **u, v, and w are the x, y, and z components of the velocity vector.** * **Velocity is the time rate of change of the position vector for the fluid particle.** * **Velocity vector V has both direction and magnitude.** * **V = speed of the fluid** * **A velocity field can be visualized by sketching the velocity vector at different locations.** * **A stagnation point occurs where V = 0.** ### Acceleration Field Fluid motion can be described by either Lagrangian (following individual particles) or Eulerian (observing particles passing a fixed point) methods. * **Eulerian method requires expressing the acceleration field as a function of space and time.** * **The acceleration field is a resultant vector whose scalar components are:** * $a_x = \frac{\partial u}{\partial t} + u\frac{\partial u}{\partial x} + v\frac{\partial u}{\partial y} + w\frac{\partial u}{\partial z}$ * $a_y = \frac{\partial v}{\partial t} + u\frac{\partial v}{\partial x} + v\frac{\partial v}{\partial y} + w\frac{\partial v}{\partial z}$ * $a_z = \frac{\partial w}{\partial t} + u\frac{\partial w}{\partial x} + v\frac{\partial w}{\partial y} + w\frac{\partial w}{\partial z}$ * **Material derivative (substantial derivative) can be used to express the acceleration in shorthand form:** * $a = \frac{DV}{Dt} = \frac{\partial V}{\partial t} + (V \cdot \nabla)V$. ### Local and Convective Acceleration * **Local acceleration** refers to time-based changes in velocity at a fixed location. * $a_{local} = \frac{\partial V}{\partial t}$ * **Convective acceleration** results from changes in velocity due to movement of the fluid particle. * $a_{convective} = (V \cdot \nabla)V$ * **Total acceleration is the sum of local and convective acceleration.** * $a = a_{local} + a_{convective}$. ### Tangential and Normal Acceleration * **Tangential acceleration (a_s)** refers to the acceleration of a particle moving along a curved path. * **Normal acceleration (a_n)** is the acceleration towards the center of the curved path. * $a_n = \frac{V^2}{r}$ **This gives us an acceleration vector: $a = a_s + a_n$** ### One, Two, and Three-Dimensional Flows Fluid flow is generally three-dimensional and time-dependent. > **However,** certain assumptions can simplify analysis while maintaining accuracy. #### One-Dimensional Flow * Two velocity components are negligible. * Mathematically: $V = ui, v = 0, w = 0$ * **Example:** Flow in a pipe where average parameters are used. #### Two-Dimensional Flow * One velocity component is relatively small and negligible. * $V = ui + vj$ * **Example:** Flow between parallel plates, flow in the main stream of a wide river. #### Three-Dimensional Flow * Velocity is a function of time and three mutually perpendicular directions. * $V = V(x, y, z, t) = ui + vj + wk$ * **Example:** Flow in converging or diverging pipes. ### Steady and Unsteady Flow #### Steady Flow * Fluid characteristics (velocity, pressure, density) don't change with time at a given point in space -- they have a constant flow rate. * **Mathematically:** $\frac{\partial u}{\partial t} = 0, \frac{\partial v}{\partial t} = 0, \frac{\partial w}{\partial t} = 0$. * **Example:** Flow through a conduit with constant size and shape, and a velocity equation in the form $u = ax^2 + bx + c$ #### Unsteady Flow * Fluid characteristics change over time at a given point in space. * **Mathematically:** $\frac{\partial u}{\partial t} \neq 0, \frac{\partial v}{\partial t} \neq 0, \frac{\partial w}{\partial t} \neq 0$ **In reality, most flows are unsteady.** This is because it is generally harder to analyze and experiment with unsteady flows. So, steady-state assumptions are useful when they don't compromise the accuracy of the results. ### Compressible and Incompressible Flows * **Compressible flow:** Density of the fluid varies from point to point. * **Mathematically:** $\rho \neq constant$ * **Example:** Flow of gases through orifices, nozzles, gas turbines. * **Incompressible flow:** Density of the fluid remains constant throughout. * **Mathematically:** $\rho = constant$ * **Example:** Subsonic aerodynamics. ### Continuity Equation * The continuity equation is based on the principle of conservation of mass which states that, for a fluid flowing through a pipe, the mass passing through different sections across a length remains unchanged, unless additional fluid is added or removed. * **mathematically:** $\rho_1A_1V_1 = \rho_2A_2V_2$, where: * $A$ is the area of the pipe. * $V$ is the velocity of the fluid. * $\rho$ is the density of the fluid. * **For an incompressible fluid $\rho_1 = \rho_2$, simplifying the equation:** $A_1V_1 = A_2V_2$. ### Continuity Equation in Cartesian Coordinates * **Consider a fluid element in the shape of a parallelepiped:** with sides $dx$, $dy$, $dz$. * **Let:** * $\rho$ = Mass density of the fluid at an instant. * u, v, w = velocity components of the fluid across the parallelepiped's faces. * **Steps to derive the continuity equation in Cartesian coordinates:** 1. **Fluid influx:** * $\rho udydz$ 2. **Fluid efflux:** * $\rho udydz + \frac{\partial (\rho u)}{\partial x}dxdydz$ 3. **Gain in mass per unit time in X-direction:** * $- \frac{\partial (\rho u)}{\partial x}dxdydz$ 4. **Gain in mass per unit time in Y and Z directions:** * $-\frac{\partial (\rho v)}{\partial y} dxdydz$ * $-\frac{\partial (\rho w)}{\partial z} dxdydz$ 5. **Total gain in mass per unit time (along coordinate axes):** * $-\left(\frac{\partial (\rho u)}{\partial x}+\frac{\partial (\rho v)}{\partial y}+\frac{\partial (\rho w)}{\partial z}\right)dxdydz$ 6. **Rate of change in mass of the parallelepiped**: * $\frac{\partial (\rho dxdydz)}{\partial t}$ 7. **Equate steps 5 and 6**: * $-\left(\frac{\partial (\rho u)}{\partial x}+\frac{\partial (\rho v)}{\partial y}+\frac{\partial (\rho w)}{\partial z}\right)dxdydz = \frac{\partial (\rho dxdydz)}{\partial t}$ 8. **Simplify the equation:** * $\frac{\partial \rho}{\partial t} + \frac{\partial (\rho u)}{\partial x}+\frac{\partial (\rho v)}{\partial y}+\frac{\partial (\rho w)}{\partial z} = 0$ 9. **For steady flow:** $\frac{\partial \rho}{\partial t} = 0$ * $\frac{\partial u}{\partial x}+\frac{\partial v}{\partial y}+\frac{\partial w}{\partial z} = 0$ 10. **For two-dimensional flow ($w = 0$):** * $\frac{\partial u}{\partial x}+\frac{\partial v}{\partial y} = 0$ * **Integrating the above equation for a constant flow rate:** $Q = au = constant$ ### Types of Flow Lines Flow analysis can be simplified by visualizing and analyzing flow fields using: * **Streamlines:** A line everywhere tangent to the velocity field. * For steady flows, streamlines are fixed. * For unsteady flows, streamlines can change shape over time. * **Equation of streamline:** * $\frac{dx}{u} = \frac{dy}{v} = \frac{dz}{w}$ * **Properties of streamlines:** * Streamlines cannot intersect each other or themselves. * Fluid cannot move across streamlines. * Streamline spacing is inverse to flow velocity: flow converges as spacing decreases. * Streamline represents the direction of flow particles at a given instant. * In steady flow, streamlines and pathlines are identical. > **However**, in unsteady flow, streamline patterns may change over time. * **Stream tube:** A fluid mass bounded by a group of streamlines. * **Example:** Pipes and nozzles. * **Stream function (:psi):** A function of space and time that gives velocities perpendicular to the direction of differentiation. * For two-dimensional flow: $\psi = f(x, y, t)$. * **Equation for steady flow:** $\frac{\partial^2\psi}{\partial x\partial y} = 0$ * **Streakline:** Continuous path taken by fluid particles passing a given point over time. * **Example:** Smoke emitted from a chimney. * **Vortex:** Streamlines form concentric circles. * **Two types:** * **Free vortex:** Rotating fluid without external forces. * **Forced vortex:** Rotating fluid due to external forces. * **Circulation (Γ):** Line integral of the velocity component tangent to a closed curve in a flow field. > **Example:** The area around a closed curve of a vortex. * **Vorticity (ζ):** A vector that is twice the rotation vector. * **For two-dimensional flow in the xy plane:** $\zeta = 2\omega_{z}= \frac{\partial v}{\partial x} - \frac{\partial u}{\partial y}$. * **Rotational flow:** Flow possessing vorticity. * **Irrotational flow:** Rotation is equal to zero. * **Velocity potential (Φ):** A scalar function whose negative derivative in any direction gives the velocity in that direction. * **For steady flow:** $\Phi = f(x, y,z)$ * **Formula:** $u = -\frac{\partial \Phi}{\partial x}$, $v = -\frac{\partial \Phi}{\partial y}$, $w = -\frac{\partial \Phi}{\partial z}$. * **Laplace's equation (for incompressible, irrotational flow):** $\frac{\partial^2 \Phi}{\partial x^2} + \frac{\partial^2 \Phi}{\partial y^2} + + \frac{\partial^2 \Phi}{\partial z^2} = 0$ > **This type of flow is called potential flow.** * **Potential flow can be defined by boundary conditions**. * The boundary conditions are used to determine the velocity potential function and the velocity at points in the flow. **The velocity potential is a consequence of the irrotational nature of the flow, whereas the stream function is a consequence of conservation of mass.** **Stream function is defined for two-dimensional flow, while the velocity potential can be defined for three-dimensional flows.**