add mmme1048 back in lol
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uni/mmme/1048_thermodynamics_and_fluid_mechanics/fluid_dynamics.md
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---
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author: Alvie Rahman
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date: \today
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title: MMME1048 // Fluid Dynamics
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tags: [ uni, nottingham, mechanical, engineering, fluid_mechanics, mmme1048, fluid_dynamics ]
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---
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\newcommand\Rey{\mbox{\textit{Re}}}
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\newcommand\textRey{$\Rey$}
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# Introductory Concepts
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These are ideas you need to know about to know what's going on, I guess?
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## Control Volumes
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A control volume is a volume with an imaginary boundry to make it easier to analyze the flow of a
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fluid.
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The boundry is drawn where the properties and conditions of the fluid is known, or where an
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approximation can be made.
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Properties which may be know include:
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- Velocity
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- Pressure
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- Temperature
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- Viscosity
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The region in the control volume is analyed in terms of enery and mass flows entering and leaving
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the control volumes.
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You don't have to understand what's going on inside the control volume.
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<details>
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<summary>
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### Example 1
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The thrust of a jet engine on an aircraft at rest can be analysed in terms of the changes in
|
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momentum or the air passing through the engine.
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</summary>
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![](./images/vimscrot-2021-11-03T21:51:51,497459693+00:00.png)
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The control volume is drawn far enough in front of the engine that the air velocity entering can
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be assumed to be at atmospheric pressurce and its velocity negligible.
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At the exit of the engine the boundary is drawn close where the velocity is known and the air
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pressure atmospheric.
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The control volume cuts the material attaching the engine to the aircraft and there will be a force
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transmitted across the control volume there to oppose the forces on the engine created by thrust
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and gravity.
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The details of the flows inside the control volume do not need to be known as the thrust can be
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determined in terms of forces and flows crossing the boundaries drawn.
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However, to understand the flows inside the engine in more detail, a more detailed analysis would
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be required.
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</details>
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## Ideal Fluid
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The actual flow pattern in a fluid is usually complex and difficult to model but it can be
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simplified by assuming the fluid is ideal.
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The ideal fluid has the following properties:
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- Zero viscosity
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- Incompressible
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- Zero surface tension
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- Does not change phases
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Gases and vapours are compressible so can only be analysed as ideal fluids when flow velocities are
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low but they can often be treated as ideal (or perfect) gases, in which case the ideal gas equations
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apply.
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## Steady Flow
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Steady flow is a flow which has *no changes in properties with respect to time*.
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Properties may vary from place to place but in the same place the properties must not change in
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the control volume to be steady flow.
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Unsteady flow does change with respect to time.
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## Uniform Flow
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Uniform flow is when all properties are the same at all points at any given instant but can change
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with respect to time, like the opposite of steady flow.
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## One Dimensional Flow
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In one dimensional (1D) flow it is assumed that all properties are uniform over any plane
|
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perpedenciular to the direction of flow (e.g. all points along the cross section of a pipe have
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identical properties).
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This means properties can only flow in one direction---usually the direction of flow.
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1D flow is never achieved exactly in practice as when a fluid flows along a pipe, the velocity at
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the wall is 0, and maximum in the centre of the pipe.
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Despite this, assuming flow is 1D simplifies the analysis and often is accurate enough.
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## Flow Patterns
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There are multiple ways to visualize flow patterns.
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### Streamlines
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A streamline is a line along which all the particle have, at a given instant, velocity vectors
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which are tangential to the line.
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Therefore there is no component of velocity of a streamline.
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A particle can never cross a streamline and *streamlines never cross*.
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They can be constructed mathematically and are often shown as output from CFD analysis.
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For a steady flow there are no changes with respect to time so the streamline pattern does not.
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The pattern does change when in unsteady flow.
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Streamlines in uniform flow must be straight and parallel.
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They must be parallel as if they are not, then different points will have different directions and
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therefore different velocities.
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Same reasoning with if they are not parallel.
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### Pathlines
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A pathline shows the route taken by a single particle during a given time interval.
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It is equivalent to a high exposure photograph which traces the moevement of the particle marked.
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You could track pathlines with a drop of injected dye or inserting a buoyant solid particle which
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has the same density as the solid.
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Pathlines may cross.
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### Streaklines
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A streakline joins, at any given time, all particles that have passed through a given point.
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Examples of this are line dye or a smoke stream which is produced from a continuous supply.
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## Viscous (Real) Fluids
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### Viscosity
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A fluid offers resisistance to motion due to its viscosity or internal friction.
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The greater the resistance to flow, the greater the viscosity.
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Higher viscosity also reduces the rate of shear deformation between layers for a given shear stress.
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Viscosity comes from two effects:
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- In liquids, the inter-molecular forces act as drag between layers of fluid moving at different
|
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velocities
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- In gases, the mixing of faster and slower moving fluid causes friction due to momentum transfer.
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The slower layers tend to slow down the faster ones
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### Newton's Law of Viscosity
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Viscosity can be defined in terms of rate of shear or velocity gradient.
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![](./images/vimscrot-2021-11-17T14:14:05,079195275+00:00.png)
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Consider the flow in the pipe above.
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Fluid in contact with the surface has a velocity of 0 because the surface irregularities trap the
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fluid particles.
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A short distance away from the surface the velocity is low but in the middle of the pipe the
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velocity is $v_F$.
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Let the velocity at a distance $y$ be $v$ and at a distance $y + \delta y$ be $v + \delta v$.
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The ratio $\frac{\delta v}{\delta y}$ is the average velocity gradient over the distance
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$\delta y$.
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But as $\delta y$ tends to zero, $\frac{\delta v}{\delta y} \rightarrow$ the value of the
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differential $\frac{\mathrm{d}v}{\mathrm{d}y}$ at a point such as point A.
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For most fluids in engineering it is found that the shear stress, $\tau$, is directly proportional
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to the velocity gradient when straight and parallel flow is involved:
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$$\tau = \mu\frac{\mathrm{d}v}{\mathrm{d}y}$$
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Where $\mu$ is the constant of proportinality and known as the dynamic viscosity, or simply the
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viscosity of the fluid.
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This is Newton's Law of Viscosity and fluids that ovey it are known as Newtonian fluids.
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### Viscosity and Lubrication
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Where a fluid is a thin film (such as in lubricating flows), the velocity gradient can be
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approximated to be linear and an estimate of shear stress obtained:
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$$\tau = \mu \frac{\delta v}{\delta y} \approx \mu \frac{v}{y}$$
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From the shear stress we can calculate the force exerted by a film by the relationship:
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$$\tau = \frac F A$$
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# Fluid Flow
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## Types of flow
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There are essentially two types of flow:
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- Smooth (laminar) flow
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At low flow rates, particles of fluid are moving in straight lines and can be considered to be
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moving in layers or laminae.
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- Rough (turbulent) flow
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At higher flow rates, the paths of the individual fluid particles are not straight but disorderly
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resulting in mixing taking place
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Between fully laminar and fully turbulent flows is a transition region.
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## The Reynolds Number
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### Development of the Reynolds Number
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In laminar flow the most influentialfactor is the magnitude of the viscous forces:
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$$viscous\, forces \propto \mu\frac v l l^2 = \mu vl$$
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where $v$ is a characteristic velocit and $l$ is a characteristic length.
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In turbulent flow viscous effects are not significant but inertia effects (mixing, momentum
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exchange, acceleration of fluid mass) are.
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Interial forces can be represented by $F = ma$
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\begin{align*}
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m &\propto \rho l^3 \\
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a &= \frac{dv}{dt} \\
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&\therefore a \propto \frac v t \text{ and } t = \frac l v \\
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&\therefore a \propto \frac {v^2} l \\
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&\therefore \text{Interial forces} \propto \rho l^2\frac{v^2} l = \rho l^2v^2
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\end{align*}
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The ratio of internalforces to viscous forces is called the Reynolds number and is abbreviated to
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Re:
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$$\Rey = \frac{\text{interial forces}}{\text{viscous forces}} = \frac {\rho l^2v^2}{\mu vl} = \frac {\rho vl} \mu$$
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where $\rho$ and $\mu$ are fluid properties and $v$ and $l$ are characteristic velocity and length.
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- During laminar flow, $\Rey$ is small as viscous forces dominate.
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- During turbulent flow, $\Rey$ is large as intertial forces dominate.
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\textRey is a non dimensional group.
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It has no units because the units cancel out.
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Non dimensional groups are very important in fluid mechancics and need to be considered when scaling
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experiments.
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If \textRey is the same in two different pipes, the flow will be the same regardless of actual
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diameters, densities, or other properties.
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#### \textRey for a Circular Section Pipe
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The characteristic length for pipe flow is the diameter $d$ and the characteristic velocity is
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mean flow in the pipe, $v$, so \textRey of a circular pipe section is given by:
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$$\Rey = \frac{\rho vd} \mu$$
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For flow in a smooth circular pipe under normal engineering conditions the following can be assumed:
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- $\Rey < 2000$ --- laminar flow
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- $2000 < \Rey < 4000$ --- transition
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- $\Rey > 4000$ --- fully turbulent flow
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These figures can be significantly affected by surface roughness so flow may be turbulent below
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$\Rey = 4000$.
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# Euler's Equation
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In a static fluid, pressure only depends on density and elevation.
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In a moving fluid the pressure is also related to acceleration, viscosity, and shaft work done on or
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by the fluid.
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$$\frac 1 \rho \frac{\delta p}{\delta s} + g\frac{\delta z}{\delta s} + v\frac{\delta v}{\delta s} = 0$$
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## Assumptions / Conditions
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The Euler euqation applies where the following can be assumed:
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- Steady flow
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- The fluid is inviscid
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- No shaft work
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- Flow along a streamline
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# Bernoulli's Equation
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Euler's equation comes in differential form, which is difficult to apply.
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We can integrate it to make it easier
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\begin{align*}
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\frac 1 \rho \frac{\delta p}{\delta s} + g\frac{\delta z}{\delta s} + v\frac{\delta v}{\delta s} &= 0
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& \text{(Euler's equation)} \\
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\int\left\{\frac{\mathrm{d}p} \rho + g\mathrm{d}z + v\mathrm{d}v \right\} &= \int 0 \,\mathrm{d}s \\
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\therefore \int \frac 1 \rho \,\mathrm{d}p + g\int \mathrm{d}z + \int v \,\mathrm{d}v &= \int 0 \,\mathrm{d}s \\
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\therefore \int \frac 1 \rho \,\mathrm{d}p + gz + \frac{v^2}{2} &= \text{constant}_1
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\end{align*}
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The first term of the equation can only be integrated if $\rho$ is constant as then:
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$$\int \frac 1 \rho \,\mathrm{d}p = \frac 1 \rho \int \mathrm{d}p = \frac p \rho$$
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So, if density is constant:
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$$\frac p \rho + gz + \frac{v^2}{2} = \text{constant}_2$$
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## Assumptions / Conditions
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All the assumptions from Euler's equation apply:
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- Steady flow
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- The fluid is inviscid
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- No shaft work
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- Flow along a streamline
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But also one more:
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- Incompressible flow
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## Forms of Bernoulli's Equation
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### Energy Form
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This form of Bernoulli's Equation is known as the energy form as each component has the units
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energy/unit mass:
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$$\frac p \rho + gz + \frac{v^2}{2} = \text{constant}_2$$
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It is split into 3 parts:
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- Pressure energy ($\frac p \rho$) --- energy needed to move the flow against the pressure
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(flow work)
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- Potential energy ($gz$) --- elevation
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- Kinetic energy ($\frac{v^2}{2}$) --- kinetic energy
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### Elevation / Head Form
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Divide the energy form by $g$:
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$$\frac\rho{\rho g} + z + \frac{v^2}{2g} = H_T$$
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where $H_T$ is constant and:
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- $\frac{p}{\rho g}$ --- static/pressure haed
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- $z$ --- elevation head
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- $\frac{v_2}{2g}$ --- dynamic/velocity head
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- $H_T$ --- total head
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- Each term now has units of elevations
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- In fluids the elevation is sometimes called head
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- This form of the equation is also useful in some applications
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### Pressure Form
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Multiply the energy form by $\rho$ to give the pressure form:
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$$p + \rho gz + \frac 1 2 \rho v^2 = \text{constant}$$
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where:
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- $p$ --- static pressure (often written as $p_s$)
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- $\rho gz$ --- elevation pressure
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- $\frac 1 2 \rho v^2$ --- dynamic pressure
|
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|
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- Density is constant
|
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- Each term now has the units of pressure
|
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- This form is useful is we are interested in pressures
|
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### Comparing two forms of the Bernoulli Equation (Piezometric)
|
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$$\text{piezometric} = \text{static} + \text{elevation}$$
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Pressure form:
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\begin{align*}
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p_s + \rho gz + \frac 1 2 \rho v^2 &= \text{total pressure} \\
|
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p_s + \rho gz &= \text{piezometric pressure}
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\end{align*}
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Head form:
|
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\begin{align*}
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\frac{p_s}{\rho g} + z + \frac{v^2}{2g} &= \text{total head} \\
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\frac{p_s}{\rho g} + z &= \text{piezometric head}
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\end{align*}
|
506
uni/mmme/1048_thermodynamics_and_fluid_mechanics/fluid_mechanics.md
Executable file
@ -0,0 +1,506 @@
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---
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||||
author: Alvie Rahman
|
||||
date: \today
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||||
title: MMME1048 // Fluid Mechanics Intro and Statics
|
||||
tags: [ uni, nottingham, mechanical, engineering, fluid_mechanics, mmme1048, fluid_statics ]
|
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---
|
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# Properties of Fluids
|
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|
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## What is a Fluid?
|
||||
|
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- A fluid may be liquid, vapor, or gas
|
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- No permanent shape
|
||||
- Consists of atoms in random motion and continual collision
|
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- Easy to deform
|
||||
- Liquids have fixed volume, gasses fill up container
|
||||
- **A fluid is a substance for wich a shear stress tends to produce unlimited, continuous
|
||||
deformation**
|
||||
|
||||
## Shear Forces
|
||||
|
||||
- For a solid, application of shear stress causes a deformation which, if not too great (elastic),
|
||||
is not permanent and solid regains original positon
|
||||
- For a fluid, continuious deformation takes place as the molecules slide over each other until the
|
||||
force is removed
|
||||
- **A fluid is a substance for wich a shear stress tends to produce unlimited, continuous
|
||||
deformation**
|
||||
|
||||
## Density
|
||||
|
||||
- Density: $$ \rho = \frac m V $$
|
||||
- Specific Density: $$ v = \frac 1 \rho $$
|
||||
|
||||
### Obtaining Density
|
||||
|
||||
- Find mass of a given volume or volume of a given mass
|
||||
- This gives average density and assumes density is the same throughout
|
||||
|
||||
- This is not always the case (like in chocolate chip ice cream)
|
||||
- Bulk density is often used to refer to average density
|
||||
|
||||
### Engineering Density
|
||||
|
||||
- Matter is not continuous on molecular scale
|
||||
- For fluids in constant motion, we take a time average
|
||||
- For most practical purposes, matter is considered to be homogenous and time averaged
|
||||
|
||||
## Pressure
|
||||
|
||||
- Pressure is a scalar quantity
|
||||
- Gases cannot sustain tensile stress, liquids a negligible amount
|
||||
|
||||
- There is a certain amount of energy associated with the random continuous motion of the molecules
|
||||
- Higher pressure fluids tend to have more energy in their molecules
|
||||
|
||||
### How Does Molecular Motion Create Force?
|
||||
|
||||
- When molecules interact with each other, there is no net force
|
||||
- When they interact with walls, there is a resultant force perpendicular to the surface
|
||||
- Pressure caused my molecule: $$ p = \frac {\delta{}F}{\delta{}A} $$
|
||||
- If we want total force, we have to add them all up
|
||||
- $$ F = \int \mathrm{d}F = \int p\, \mathrm{d}A $$
|
||||
|
||||
- If pressure is constant, then this integrates to $$ F = pA $$
|
||||
- These equations can be used if pressure is constant of average value is appropriate
|
||||
- For many cases in fluids pressure is not constant
|
||||
|
||||
### Pressure Variation in a Static Fluid
|
||||
|
||||
- A fluid at rest has constant pressure horizontally
|
||||
- That's why liquid surfaces are flat
|
||||
- But fluids at rest do have a vertical gradient, where lower parts have higher presure
|
||||
|
||||
### How Does Pressure Vary with Depth?
|
||||
|
||||
![From UoN MMME1048 Fluid Mechanics Notes](./images/vimscrot-2021-10-06T10:51:51,499044519+01:00.png)
|
||||
|
||||
Let fluid pressure be p at height $z$, and $p + \delta p$ at $z + \delta z$.
|
||||
|
||||
Force $F_z$ acts upwards to support the fluid, countering pressure $p$.
|
||||
|
||||
Force $F_z + \delta F_z$acts downwards to counter pressure $p + \delta p$ and comes from the weight
|
||||
of the liquid above.
|
||||
|
||||
Now:
|
||||
|
||||
\begin{align*}
|
||||
F_z &= p\delta x\delta y \\
|
||||
F_z + \delta F_z &= (p + \delta p) \delta x \delta y \\
|
||||
\therefore \delta F_z &= \delta p(\delta x\delta y)
|
||||
\end{align*}
|
||||
|
||||
Resolving forces in z direction:
|
||||
|
||||
\begin{align*}
|
||||
F_z - (F_z + \delta F_z) - g\delta m &= 0 \\
|
||||
\text{but } \delta m &= \rho\delta x\delta y\delta z \\
|
||||
\therefore -\delta p(\delta x\delta y) &= g\rho(\delta x\delta y\delta z) \\
|
||||
\text{or } \frac{\delta p}{\delta z} &= -\rho g \\
|
||||
\text{as } \delta z \rightarrow 0,\, \frac{\delta p}{\delta z} &\rightarrow \frac{dp}{dz}\\
|
||||
\therefore \frac{dp}{dz} &= -\rho g\\
|
||||
\Delta p &= \rho g\Delta z
|
||||
\end{align*}
|
||||
|
||||
The equation applies for any fluid.
|
||||
The -ve sign indicates that as $z$, height, increases, $p$, pressure, decreases.
|
||||
|
||||
### Absolute and Gauge Pressure
|
||||
|
||||
- Absolute Pressure is measured relative to zero (a vacuum)
|
||||
- Guage pressure = absolute pressure - atmospheric pressure
|
||||
|
||||
- Often used in industry
|
||||
|
||||
- If abs. pressure = 3 bar and atmospheric pressure is 1 bar, then gauge pressure = 2 bar
|
||||
- Atmospheric pressure changes with altitude
|
||||
|
||||
## Compressibility
|
||||
|
||||
- All fluids are compressible, especially gasses
|
||||
- Most liquids can be considered **incompressible** most of the time (and will be in MMME1048, but
|
||||
may not be in future modules)
|
||||
|
||||
## Surface Tension
|
||||
|
||||
- In a liquid, molecules are held together by molecular attraction
|
||||
- At a boundry between two fluids this creates "surface tension"
|
||||
- Surface tension usually has the symbol $$\gamma$$
|
||||
|
||||
## Ideal Gas
|
||||
|
||||
- No real gas is perfect, although many are similar
|
||||
- We define a specific gas constant to allow us to analyse the behaviour of a specific gas:
|
||||
|
||||
$$ R = \frac {\tilde R}{\tilde m} $$
|
||||
|
||||
(Universal Gas Constant / molar mass of gas)
|
||||
|
||||
- Perfect gas law
|
||||
|
||||
$$pV=mRT$$
|
||||
|
||||
or
|
||||
|
||||
$$ p = \rho RT$$
|
||||
|
||||
- Pressure always in Pa
|
||||
- Temperature always in K
|
||||
|
||||
## Units and Dimentional Analysis
|
||||
|
||||
- It is usually better to use SI units
|
||||
- If in doubt, DA can be useful to check that your answer makes sense
|
||||
|
||||
# Fluid Statics
|
||||
|
||||
## Manometers
|
||||
|
||||
![](./images/vimscrot-2021-10-13T09:09:32,037006075+01:00.png)
|
||||
|
||||
$$p_{1,gauge} = \rho g(z_2-z_1)$$
|
||||
|
||||
- Manometers work on the principle that pressure along any horizontal plane through a continuous
|
||||
fluid is constant
|
||||
- Manometers can be used to measure the pressure of a gas, vapour, or liquid
|
||||
- Manometers can measure higher pressures than a piezometer
|
||||
- Manometer fluid and working should be immiscible (don't mix)
|
||||
|
||||
![](./images/vimscrot-2021-10-13T09:14:59,628661490+01:00.png)
|
||||
|
||||
\begin{align*}
|
||||
p_A &= p_{A'} \\
|
||||
p_{bottom} &= p_{top} + \rho gh \\
|
||||
\rho_1 &= density\,of\,fluid\,1 \\
|
||||
\rho_2 &= density\,of\,fluid\,2
|
||||
\end{align*}
|
||||
|
||||
Left hand side:
|
||||
|
||||
$$p_A = p_1 + \rho_1g\Delta z_1$$
|
||||
|
||||
Right hand side:
|
||||
|
||||
$$p_{A'} = p_{at} + \rho_2g\Delta z_2$$
|
||||
|
||||
Equate and rearrange:
|
||||
|
||||
\begin{align*}
|
||||
p_1 + \rho_1g\Delta z_1 &= p_{at} + \rho_2g\Delta z_2 \\
|
||||
p_1-p_{at} &= g(\rho_2\Delta z_2 - \rho_1\Delta z_1) \\
|
||||
p_{1,gauge} &= g(\rho_2\Delta z_2 - \rho_1\Delta z_1)
|
||||
\end{align*}
|
||||
|
||||
If $\rho_a << \rho_2$:
|
||||
|
||||
$$\rho_{1,gauge} \approx \rho_2g\Delta z_2$$
|
||||
|
||||
### Differential U-Tube Manometer
|
||||
|
||||
![](./images/vimscrot-2021-10-13T09:37:02,070474894+01:00.png)
|
||||
|
||||
- Used to find the difference between two unknown pressures
|
||||
- Can be used for any fluid that doesn't react with manometer fluid
|
||||
- Same principle used in analysis
|
||||
|
||||
\begin{align*}
|
||||
p_A &= p_{A'} \\
|
||||
p_{bottom} &= p_{top} + \rho gh \\
|
||||
\rho_1 &= density\,of\,fluid\,1 \\
|
||||
\rho_2 &= density\,of\,fluid\,2
|
||||
\end{align*}
|
||||
|
||||
Left hand side:
|
||||
|
||||
$$p_A = p_1 + \rho_wg(z_C-z_A)$$
|
||||
|
||||
Right hand side:
|
||||
|
||||
$$p_B = p_2 + \rho_wg(z_C-z_B)$$
|
||||
|
||||
Right hand manometer fluid:
|
||||
|
||||
$$p_{A'} = p_B + \rho_mg(z_B - z_a)$$
|
||||
|
||||
\begin{align*}
|
||||
p_{A'} &= p_2 + \rho_mg(z_C - z_B) + \rho_mg(z_B - zA)\\
|
||||
&= p_2 + \rho_mg(z_C - z_B) + \rho_mg\Delta z \\
|
||||
\\
|
||||
p_A &= p_{A'} \\
|
||||
p_1 + \rho_wg(z_C-z_A) &= p_2 + \rho_mg(z_C - z_B) + \rho_mg\Delta z \\
|
||||
p_1 - p_2 &= \rho_wg(z_C-z_B-z_C+z_A) + \rho_mg\Delta z \\
|
||||
&= \rho_wg(z_A-z_B) + \rho_mg\Delta z \\
|
||||
&= -\rho_wg\Delta z + \rho_mg\Delta z
|
||||
\end{align*}
|
||||
|
||||
### Angled Differential Manometer
|
||||
|
||||
![](./images/vimscrot-2021-10-13T09:56:15,656796805+01:00.png)
|
||||
|
||||
- If the pipe is sloped then
|
||||
|
||||
$$p_1-p_2 = (\rho_m-\rho_w)g\Delta z + \rho_wg(z_{C2} - z_{C1})$$
|
||||
|
||||
- $p_1 > p_2$ as $p_1$ is lower
|
||||
- If there is no flow along the tube, then
|
||||
|
||||
$$p_1 = p_2 + \rho_wg(z_{C2} - z_{C1})$$
|
||||
|
||||
<details>
|
||||
<summary>
|
||||
|
||||
### Exercise Sheet 1
|
||||
|
||||
</summary>
|
||||
|
||||
1. If 4 m$^3$ of oil weighs 35 kN calculate its density and relative density.
|
||||
Relative density is a term used to define the density of a fluid relative
|
||||
|
||||
> $$ \frac{35000}{9.81\times4} = 890 \text{ kgm}^{-3} $$
|
||||
>
|
||||
> $$1000 - 891.9... = 108 \text{ kgm}^{-3}$$
|
||||
|
||||
2. Find the pressure relative to atmospheric experienced by a diver
|
||||
working on the sea bed at a depth of 35 m.
|
||||
Take the density of sea water to be 1030 kgm$^{-3}$.
|
||||
|
||||
> $$
|
||||
> \rho gh = 1030\times 9.81 \times 35 = 3.5\times10^5
|
||||
> $$
|
||||
|
||||
3. An open glass is sitting on a table, it has a diameter of 10 cm.
|
||||
If water up to a height of 20 cm is now added calculate the force exerted onto the table by
|
||||
the addition of the water.
|
||||
|
||||
> $$V_{cylinder} = \pi r^2h$$
|
||||
> $$m_{cylinder} = \rho\pi r^2h$$
|
||||
> $$W_{cylinder} = \rho g\pi r^2h = 1000\times9.8\pi\times0.05^2\times0.2 = 15.4 \text{ N} $$
|
||||
|
||||
4. A closed rectangular tank with internal dimensions 6m x 3m x 1.5m
|
||||
high has a vertical riser pipe of cross-sectional area 0.001 m2 in
|
||||
the upper surface (figure 1.4). The tank and riser are filled with
|
||||
water such that the water level in the riser pipe is 3.5 m above the
|
||||
|
||||
Calulate:
|
||||
|
||||
i. The gauge pressure at the base of the tank.
|
||||
|
||||
> $$\rho gh = 1000\times9.81\times(1.5+3.5) = 49 \text{ kPa}$$
|
||||
|
||||
ii. The gauge pressure at the top of the tank.
|
||||
|
||||
> $$\rho gh = 1000\times9.81\times3.5 = 34 \text{ kPa}$$
|
||||
|
||||
iii. The force exercted on the base of the tank due to gauge water pressure.
|
||||
|
||||
> $$F = p\times A = 49\times10^3\times6\times3 = 8.8\times10^5 \text{ N}$$
|
||||
|
||||
iv. The weight of the water in the tank and riser.
|
||||
|
||||
> $$V = 6\times3\times1.5 + 0.001\times3.5 = 27.0035$$
|
||||
> $$W = \rho gV = 1000\times9.8\times27.0035 = 2.6\times10^5\text{ N}$$
|
||||
|
||||
v. Explain the difference between (iii) and (iv).
|
||||
|
||||
*(It may be helpful to think about the forces on the top of the tank)*
|
||||
|
||||
> The pressure at the top of the tank is higher than atmospheric pressure because of the
|
||||
> riser.
|
||||
> This means there is an upwards force on the top of tank.
|
||||
> The difference between the force acting up and down due to pressure is equal to the
|
||||
> weight of the water.
|
||||
|
||||
6. A double U-tube manometer is connected to a pipe as shown below.
|
||||
|
||||
Taking the dimensions and fluids as indicated; calculate
|
||||
the absolute pressure at point A (centre of the pipe).
|
||||
|
||||
Take atmospheric pressure as 1.01 bar and the density of mercury as 13600 kgm$^{-3}$.
|
||||
|
||||
![](./images/vimscrot-2021-10-13T10:42:52,999793176+01:00.png)
|
||||
|
||||
> \begin{align*}
|
||||
P_B &= P_A + 0.4\rho_wg &\text{(1)}\\
|
||||
P_C = P_{C'} &= P_B - 0.2\rho_mg &\text{(2)}\\
|
||||
P_D = P_{at} &= P_A + 0.4\rho_wg &\text{(3)}\\
|
||||
\\
|
||||
\text{(2) into (3)} &\rightarrow P_B -0.2\rho_mg-0.1\rho_wg = P_{at} &\text{(4)}\\
|
||||
\text{(1) into (4)} &\rightarrow P_A + 0.4\rho_wg - 0.2\rho_mg - 0.1\rho_wg = P_{at} \\
|
||||
\\
|
||||
P_A &= P_{at} + 0.1\rho_wg + 0.2\rho_mg - 0.4\rho_wg \\
|
||||
&= P_{at} + g(0.2\rho_m - 0.3\rho_w) \\
|
||||
&= 1.01\times10^5 + 9.81(0.2\times13600 - 0.3\times1000)\\
|
||||
&= 124.7\text{ kPa}
|
||||
> \end{align*}
|
||||
|
||||
</details>
|
||||
|
||||
## Submerged Surfaces
|
||||
|
||||
### Prepatory Maths
|
||||
|
||||
#### Integration as Summation
|
||||
|
||||
#### Centroids
|
||||
|
||||
- For a 3D body, the centre of gravity is the point at which all the mass can be considered to act
|
||||
- For a 2D lamina (thin, flat plate) the centroid is the centre of area, the point about which the
|
||||
lamina would balance
|
||||
|
||||
To find the location of the centroid, take moments (of area) about a suitable reference axis:
|
||||
|
||||
$$moment\,of\,area = moment\,of\,mass$$
|
||||
|
||||
(making the assumption that the surface has a unit mass per unit area)
|
||||
|
||||
$$moment\,of\,mass = mass\times distance\,from\,point\,acting\,around$$
|
||||
|
||||
Take the following lamina:
|
||||
|
||||
![](./images/vimscrot-2021-10-20T10:01:30,080819382+01:00.png)
|
||||
|
||||
1. Split the lamina into elements parallel to the chosen axis
|
||||
2. Each element has area $\delta A = w\delta y$
|
||||
3. The moment of area ($\delta M$) of the element is $\delta Ay$
|
||||
4. The sum of moments of all the elements is equal to the moment $M$ obtained by assuing all the
|
||||
area is located at the centroid or:
|
||||
|
||||
$$Ay_c = \int_{area} \! y\,\mathrm{d}A$$
|
||||
|
||||
or:
|
||||
|
||||
$$y_c = \frac 1 A \int_{area} \! y\,\mathrm{d}A$$
|
||||
|
||||
- $\int y\,\mathrm{d}A$ is known as the first moment of area
|
||||
|
||||
<details>
|
||||
<summary>
|
||||
|
||||
##### Example 1
|
||||
|
||||
Determine the location of the centroid of a rectangular lamina.
|
||||
|
||||
</summary>
|
||||
|
||||
###### Determining Location in $y$ direction
|
||||
|
||||
![](./images/vimscrot-2021-10-20T10:14:17,688774145+01:00.png)
|
||||
|
||||
1. Take moments for area about $OO$
|
||||
|
||||
$$\delta M = y\delta A = y(b\delta y)$$
|
||||
|
||||
2. Integrate to find all strips
|
||||
|
||||
$$M = b\int_0^d\! y \,\mathrm{d}y = b\left[\frac{y^2}2\right]_0^d = \frac{bd^2} 2$$
|
||||
|
||||
($b$ can be taken out the integral as it is constant in this example)
|
||||
|
||||
but also $$M = (area)(y_c) = bdy_c$$
|
||||
|
||||
so $$y_c = \frac 1 {bd} \frac {bd} 2 = \frac d 2$$
|
||||
|
||||
###### Determining Location in $x$ direction
|
||||
|
||||
![](./images/vimscrot-2021-10-20T10:24:48,372189101+01:00.png)
|
||||
|
||||
1. Take moments for area about $O'O'$:
|
||||
|
||||
$$\delta M = x\delta A = x(d\delta x)$$
|
||||
|
||||
2. Integrate
|
||||
|
||||
$$M_{O'O'} = d\int_0^b\! x \,\mathrm{d}x = d\left[\frac{x^2} 2\right]_0^b = \frac{db^2} 2$$
|
||||
|
||||
but also $$M_{O'O'} = (area)(x_c) = bdx_c$$
|
||||
|
||||
so $$x_c = \frac{db^2}{2bd} = \frac b 2$$
|
||||
|
||||
</details>
|
||||
|
||||
### Horizontal Submereged Surfaces
|
||||
|
||||
![](./images/vimscrot-2021-10-20T10:33:16,783724117+01:00.png)
|
||||
|
||||
Assumptions for horizontal lamina:
|
||||
|
||||
- Constant pressure acts over entire surface of lamina
|
||||
- Centre of pressure will coincide with centre of area
|
||||
- $total\,force = pressure\times area$
|
||||
|
||||
![](./images/vimscrot-2021-10-20T10:36:12,520683729+01:00.png)
|
||||
|
||||
### Vertical Submerged Surfaces
|
||||
|
||||
![](./images/vimscrot-2021-10-20T11:05:33,235642932+01:00.png)
|
||||
|
||||
- A vertical submerged plate does experience uniform pressure
|
||||
- Centroid of pressure and area are not coincident
|
||||
- Centroid of pressure is always below centroid of area for a vertical plate
|
||||
- No shear forces, so all hydrostatic forces are perpendicular to lamina
|
||||
|
||||
![](./images/vimscrot-2021-10-20T11:07:52,929126609+01:00.png)
|
||||
|
||||
Force acting on small element:
|
||||
|
||||
\begin{align*}
|
||||
\delta F &= p\delta A \\
|
||||
&= \rho gh\delta A \\
|
||||
&= \rho gh w\delta h
|
||||
\end{align*}
|
||||
|
||||
Therefore total force is
|
||||
|
||||
$$F_p = \int_{area}\! \rho gh \,\mathrm{d}A = \int_{h_1}^{h_2}\! \rho ghw\,\mathrm{d}h$$
|
||||
|
||||
#### Finding Line of Action of the Force
|
||||
|
||||
![](./images/vimscrot-2021-10-20T11:15:51,200869760+01:00.png)
|
||||
|
||||
\begin{align*}
|
||||
\delta M_{OO} &= \delta Fh = (\rho gh\delta A)h \\
|
||||
&= \rho gh^2\delta A = \rho gh^2w\delta h \\
|
||||
\\
|
||||
M_{OO} &= F_py_p = \int_{area}\! \rho gh^2 \,\mathrm{d}A \\
|
||||
&= \int_{h1}^{h2}\! \rho gh^2w \,\mathrm{d}h \\
|
||||
\\
|
||||
y_p = \frac{M_{OO}}{F_p}
|
||||
\end{align*}
|
||||
|
||||
## Buoyancy
|
||||
|
||||
### Archimedes Principle
|
||||
|
||||
> The resultant upwards force (buoyancy force) on a body wholly or partially immersed in a fluid is
|
||||
> equal to the weight of the displaced fluid.
|
||||
|
||||
When an object is in equilibrium the forces acting on it balance.
|
||||
For a floating object, the upwards force equals the weight:
|
||||
|
||||
$$mg = \rho Vg$$
|
||||
|
||||
Where $\rho$ is the density of the fluid, and $V$ is the volume of displaced fluid.
|
||||
|
||||
### Immersed Bodies
|
||||
|
||||
As pressure increases with depth, the fluid exerts a resultant upward force on a body.
|
||||
There is no horizontal component of the buoyancy force because the vertiscal projection of the body
|
||||
is the same in both directions.
|
||||
|
||||
### Rise, Sink, or Float?
|
||||
|
||||
- $F_B = W$ \rightarrow equilirbrium (floating)
|
||||
- $F_B > W$ \rightarrow body rises
|
||||
- $F_B < W$ \rightarrow body sinks
|
||||
|
||||
### Centre of Buoyancy
|
||||
|
||||
Buoyancy force acts through the centre of gravity of the volume of fluid displaced.
|
||||
This is known as the centre of buoyancy.
|
||||
The centre of buoyancy does not in general correspond to the centre of gravity of the body.
|
||||
|
||||
If the fluid density is constant the centre of gravity of the displaced fluid is at the centroid of
|
||||
the immersed volume.
|
||||
|
||||
![](./images/vimscrot-2021-12-21T15:08:22,285753421+00:00.png)
|
||||
|
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