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---
author: Alvie Rahman
date: \today
title: MMME1048 // Fluid Dynamics
tags: [ uni, nottingham, mechanical, engineering, fluid_mechanics, mmme1048, fluid_dynamics ]
---
\newcommand\Rey{\mbox{\textit{Re}}}
\newcommand\textRey{$\Rey$}
# Introductory Concepts
These are ideas you need to know about to know what's going on, I guess?
## Control Volumes
A control volume is a volume with an imaginary boundry to make it easier to analyze the flow of a
fluid.
The boundry is drawn where the properties and conditions of the fluid is known, or where an
approximation can be made.
Properties which may be know include:
- Velocity
- Pressure
- Temperature
- Viscosity
The region in the control volume is analyed in terms of enery and mass flows entering and leaving
the control volumes.
You don't have to understand what's going on inside the control volume.
<details>
<summary>
### Example 1
The thrust of a jet engine on an aircraft at rest can be analysed in terms of the changes in
momentum or the air passing through the engine.
</summary>
![](./images/vimscrot-2021-11-03T21:51:51,497459693+00:00.png)
The control volume is drawn far enough in front of the engine that the air velocity entering can
be assumed to be at atmospheric pressurce and its velocity negligible.
At the exit of the engine the boundary is drawn close where the velocity is known and the air
pressure atmospheric.
The control volume cuts the material attaching the engine to the aircraft and there will be a force
transmitted across the control volume there to oppose the forces on the engine created by thrust
and gravity.
The details of the flows inside the control volume do not need to be known as the thrust can be
determined in terms of forces and flows crossing the boundaries drawn.
However, to understand the flows inside the engine in more detail, a more detailed analysis would
be required.
</details>
## Ideal Fluid
The actual flow pattern in a fluid is usually complex and difficult to model but it can be
simplified by assuming the fluid is ideal.
The ideal fluid has the following properties:
- Zero viscosity
- Incompressible
- Zero surface tension
- Does not change phases
Gases and vapours are compressible so can only be analysed as ideal fluids when flow velocities are
low but they can often be treated as ideal (or perfect) gases, in which case the ideal gas equations
apply.
## Steady Flow
Steady flow is a flow which has *no changes in properties with respect to time*.
Properties may vary from place to place but in the same place the properties must not change in
the control volume to be steady flow.
Unsteady flow does change with respect to time.
## Uniform Flow
Uniform flow is when all properties are the same at all points at any given instant but can change
with respect to time, like the opposite of steady flow.
## One Dimensional Flow
In one dimensional (1D) flow it is assumed that all properties are uniform over any plane
perpedenciular to the direction of flow (e.g. all points along the cross section of a pipe have
identical properties).
This means properties can only flow in one direction---usually the direction of flow.
1D flow is never achieved exactly in practice as when a fluid flows along a pipe, the velocity at
the wall is 0, and maximum in the centre of the pipe.
Despite this, assuming flow is 1D simplifies the analysis and often is accurate enough.
## Flow Patterns
There are multiple ways to visualize flow patterns.
### Streamlines
A streamline is a line along which all the particle have, at a given instant, velocity vectors
which are tangential to the line.
Therefore there is no component of velocity of a streamline.
A particle can never cross a streamline and *streamlines never cross*.
They can be constructed mathematically and are often shown as output from CFD analysis.
For a steady flow there are no changes with respect to time so the streamline pattern does not.
The pattern does change when in unsteady flow.
Streamlines in uniform flow must be straight and parallel.
They must be parallel as if they are not, then different points will have different directions and
therefore different velocities.
Same reasoning with if they are not parallel.
### Pathlines
A pathline shows the route taken by a single particle during a given time interval.
It is equivalent to a high exposure photograph which traces the moevement of the particle marked.
You could track pathlines with a drop of injected dye or inserting a buoyant solid particle which
has the same density as the solid.
Pathlines may cross.
### Streaklines
A streakline joins, at any given time, all particles that have passed through a given point.
Examples of this are line dye or a smoke stream which is produced from a continuous supply.
## Viscous (Real) Fluids
### Viscosity
A fluid offers resisistance to motion due to its viscosity or internal friction.
The greater the resistance to flow, the greater the viscosity.
Higher viscosity also reduces the rate of shear deformation between layers for a given shear stress.
Viscosity comes from two effects:
- In liquids, the inter-molecular forces act as drag between layers of fluid moving at different
velocities
- In gases, the mixing of faster and slower moving fluid causes friction due to momentum transfer.
The slower layers tend to slow down the faster ones
### Newton's Law of Viscosity
Viscosity can be defined in terms of rate of shear or velocity gradient.
![](./images/vimscrot-2021-11-17T14:14:05,079195275+00:00.png)
Consider the flow in the pipe above.
Fluid in contact with the surface has a velocity of 0 because the surface irregularities trap the
fluid particles.
A short distance away from the surface the velocity is low but in the middle of the pipe the
velocity is $v_F$.
Let the velocity at a distance $y$ be $v$ and at a distance $y + \delta y$ be $v + \delta v$.
The ratio $\frac{\delta v}{\delta y}$ is the average velocity gradient over the distance
$\delta y$.
But as $\delta y$ tends to zero, $\frac{\delta v}{\delta y} \rightarrow$ the value of the
differential $\frac{\mathrm{d}v}{\mathrm{d}y}$ at a point such as point A.
For most fluids in engineering it is found that the shear stress, $\tau$, is directly proportional
to the velocity gradient when straight and parallel flow is involved:
$$\tau = \mu\frac{\mathrm{d}v}{\mathrm{d}y}$$
Where $\mu$ is the constant of proportinality and known as the dynamic viscosity, or simply the
viscosity of the fluid.
This is Newton's Law of Viscosity and fluids that ovey it are known as Newtonian fluids.
### Viscosity and Lubrication
Where a fluid is a thin film (such as in lubricating flows), the velocity gradient can be
approximated to be linear and an estimate of shear stress obtained:
$$\tau = \mu \frac{\delta v}{\delta y} \approx \mu \frac{v}{y}$$
From the shear stress we can calculate the force exerted by a film by the relationship:
$$\tau = \frac F A$$
# Fluid Flow
## Types of flow
There are essentially two types of flow:
- Smooth (laminar) flow
At low flow rates, particles of fluid are moving in straight lines and can be considered to be
moving in layers or laminae.
- Rough (turbulent) flow
At higher flow rates, the paths of the individual fluid particles are not straight but disorderly
resulting in mixing taking place
Between fully laminar and fully turbulent flows is a transition region.
## The Reynolds Number
### Development of the Reynolds Number
In laminar flow the most influentialfactor is the magnitude of the viscous forces:
$$viscous\, forces \propto \mu\frac v l l^2 = \mu vl$$
where $v$ is a characteristic velocit and $l$ is a characteristic length.
In turbulent flow viscous effects are not significant but inertia effects (mixing, momentum
exchange, acceleration of fluid mass) are.
Interial forces can be represented by $F = ma$
\begin{align*}
m &\propto \rho l^3 \\
a &= \frac{dv}{dt} \\
&\therefore a \propto \frac v t \text{ and } t = \frac l v \\
&\therefore a \propto \frac {v^2} l \\
&\therefore \text{Interial forces} \propto \rho l^2\frac{v^2} l = \rho l^2v^2
\end{align*}
The ratio of internalforces to viscous forces is called the Reynolds number and is abbreviated to
Re:
$$\Rey = \frac{\text{interial forces}}{\text{viscous forces}} = \frac {\rho l^2v^2}{\mu vl} = \frac {\rho vl} \mu$$
where $\rho$ and $\mu$ are fluid properties and $v$ and $l$ are characteristic velocity and length.
- During laminar flow, $\Rey$ is small as viscous forces dominate.
- During turbulent flow, $\Rey$ is large as intertial forces dominate.
\textRey is a non dimensional group.
It has no units because the units cancel out.
Non dimensional groups are very important in fluid mechancics and need to be considered when scaling
experiments.
If \textRey is the same in two different pipes, the flow will be the same regardless of actual
diameters, densities, or other properties.
#### \textRey for a Circular Section Pipe
The characteristic length for pipe flow is the diameter $d$ and the characteristic velocity is
mean flow in the pipe, $v$, so \textRey of a circular pipe section is given by:
$$\Rey = \frac{\rho vd} \mu$$
For flow in a smooth circular pipe under normal engineering conditions the following can be assumed:
- $\Rey < 2000$ --- laminar flow
- $2000 < \Rey < 4000$ --- transition
- $\Rey > 4000$ --- fully turbulent flow
These figures can be significantly affected by surface roughness so flow may be turbulent below
$\Rey = 4000$.
# Euler's Equation
In a static fluid, pressure only depends on density and elevation.
In a moving fluid the pressure is also related to acceleration, viscosity, and shaft work done on or
by the fluid.
$$\frac 1 \rho \frac{\delta p}{\delta s} + g\frac{\delta z}{\delta s} + v\frac{\delta v}{\delta s} = 0$$
## Assumptions / Conditions
The Euler euqation applies where the following can be assumed:
- Steady flow
- The fluid is inviscid
- No shaft work
- Flow along a streamline
# Bernoulli's Equation
Euler's equation comes in differential form, which is difficult to apply.
We can integrate it to make it easier
\begin{align*}
\frac 1 \rho \frac{\delta p}{\delta s} + g\frac{\delta z}{\delta s} + v\frac{\delta v}{\delta s} &= 0
& \text{(Euler's equation)} \\
\int\left\{\frac{\mathrm{d}p} \rho + g\mathrm{d}z + v\mathrm{d}v \right\} &= \int 0 \,\mathrm{d}s \\
\therefore \int \frac 1 \rho \,\mathrm{d}p + g\int \mathrm{d}z + \int v \,\mathrm{d}v &= \int 0 \,\mathrm{d}s \\
\therefore \int \frac 1 \rho \,\mathrm{d}p + gz + \frac{v^2}{2} &= \text{constant}_1
\end{align*}
The first term of the equation can only be integrated if $\rho$ is constant as then:
$$\int \frac 1 \rho \,\mathrm{d}p = \frac 1 \rho \int \mathrm{d}p = \frac p \rho$$
So, if density is constant:
$$\frac p \rho + gz + \frac{v^2}{2} = \text{constant}_2$$
## Assumptions / Conditions
All the assumptions from Euler's equation apply:
- Steady flow
- The fluid is inviscid
- No shaft work
- Flow along a streamline
But also one more:
- Incompressible flow
## Forms of Bernoulli's Equation
### Energy Form
This form of Bernoulli's Equation is known as the energy form as each component has the units
energy/unit mass:
$$\frac p \rho + gz + \frac{v^2}{2} = \text{constant}_2$$
It is split into 3 parts:
- Pressure energy ($\frac p \rho$) --- energy needed to move the flow against the pressure
(flow work)
- Potential energy ($gz$) --- elevation
- Kinetic energy ($\frac{v^2}{2}$) --- kinetic energy
### Elevation / Head Form
Divide the energy form by $g$:
$$\frac\rho{\rho g} + z + \frac{v^2}{2g} = H_T$$
where $H_T$ is constant and:
- $\frac{p}{\rho g}$ --- static/pressure haed
- $z$ --- elevation head
- $\frac{v_2}{2g}$ --- dynamic/velocity head
- $H_T$ --- total head
- Each term now has units of elevations
- In fluids the elevation is sometimes called head
- This form of the equation is also useful in some applications
### Pressure Form
Multiply the energy form by $\rho$ to give the pressure form:
$$p + \rho gz + \frac 1 2 \rho v^2 = \text{constant}$$
where:
- $p$ --- static pressure (often written as $p_s$)
- $\rho gz$ --- elevation pressure
- $\frac 1 2 \rho v^2$ --- dynamic pressure
- Density is constant
- Each term now has the units of pressure
- This form is useful is we are interested in pressures
### Comparing two forms of the Bernoulli Equation (Piezometric)
$$\text{piezometric} = \text{static} + \text{elevation}$$
Pressure form:
\begin{align*}
p_s + \rho gz + \frac 1 2 \rho v^2 &= \text{total pressure} \\
p_s + \rho gz &= \text{piezometric pressure}
\end{align*}
Head form:
\begin{align*}
\frac{p_s}{\rho g} + z + \frac{v^2}{2g} &= \text{total head} \\
\frac{p_s}{\rho g} + z &= \text{piezometric head}
\end{align*}

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@ -1,506 +0,0 @@
---
author: Alvie Rahman
date: \today
title: MMME1048 // Fluid Mechanics Intro and Statics
tags: [ uni, nottingham, mechanical, engineering, fluid_mechanics, mmme1048, fluid_statics ]
---
# Properties of Fluids
## What is a Fluid?
- A fluid may be liquid, vapor, or gas
- No permanent shape
- Consists of atoms in random motion and continual collision
- 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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