Hydrostatic Pressure

Storyboard

In the case of saturated soil, porosity is filled with water. The presence of water implies additional mass and the existence of pressure as a function of depth. Both factors will affect the behavior of the soil.

>Model

ID:(368, 0)



Mechanisms

Concept

>Top



Code
Concept

Mechanisms

ID:(15201, 0)



Description of the water column

Concept

>Top


To study the behavior of liquids, it is useful to introduce the concept of a column of liquid. This column is an abstraction of a cylindrical container (such as a graduated cylinder) containing liquid, and allows us to study the force to which an object inside it is exposed.

Once this concept is introduced, we can think of its existence independently of the container that contains it. For example, a diver swimming in open sea is exposed to the weight generated by an 'imaginary' column of liquid that exists above them, from the surface of the liquid to their skin and the surface of the sea.



With the liquid column, we can introduce the measurements of the column height ($h$), the column Section ($S$), and the liquid density ($\rho_w$). This yields the mass of liquid column ($M$):

$ M = \rho_w S h $

ID:(2207, 0)



Force of water on the bottom of the column

Concept

>Top


Once the volume and thus the mass of the column is known, the force it exerts on its bottom can be calculated. It is important to note that this applies to liquids that are considered incompressible, which means that the lower layers of the liquid are assumed not to be compressed by the weight of the layers above them.



This principle can be applied to calculate the force exerted by any liquid, such as water or oil, and is particularly useful in hydraulic engineering and fluid mechanics.

In this way, we obtain the column force ($F$) from the mass of liquid column ($M$) and the gravitational Acceleration ($g$):

$ F_g = m_g g $

ID:(2208, 0)



Introduction of the concept of pressure

Concept

>Top


In mechanics, we describe how bodies with defined mass move. In the case of a liquid, its movement is not uniform, and each section of the liquid moves differently. However, these \\"sections\\" do not have a defined mass, as they are not defined or separate objects.

To address this issue, we can segment the liquid into a series of small, separated volumes and, if possible, estimate their mass using density. In this way, we can introduce the idea that forces define the movement of the liquid.

However, ultimately volumes are arbitrary, and what ultimately generates the movement is the force acting on the volume's face. Therefore, it makes more sense to introduce the concept of column force ($F$) per such column Section ($S$), which is called the water column pressure ($p_t$).

$ p \equiv\displaystyle\frac{ F }{ S }$

ID:(46, 0)



Water pressure on the bottom of the column

Concept

>Top


The the column force ($F$) acting on the bottom depends on the column Section ($S$) in the sense that if the latter varies, the force will vary in the same proportion. In this sense, the column force ($F$) and the column Section ($S$) are not interdependent; they vary proportionally. It makes sense to define this proportion as the pressure ($p$):



the pressure ($p$) can be expressed as a function of the liquid density ($\rho_w$), the gravitational Acceleration ($g$), and the column height ($h$) as follows:

$ p = \rho_w g h $

ID:(2085, 0)



Sum of column pressure and atmosphere

Concept

>Top


If it is considered that the column is influenced by the atmospheric pressure ($p_0$), then the contribution of the atmospheric pressure ($p_0$) must be added to the water column pressure ($p_t$) of the column, as shown here:



In this case, the pressure ($p$) can be expressed as a function of the liquid density ($\rho_w$), the gravitational Acceleration ($g$), the column height ($h$), and it should include the atmospheric pressure ($p_0$), as follows:

$ p = p_0 + \rho_w g h $



It is not always necessary to consider atmospheric pressure in the modeling:

In many cases, atmospheric pressure is present throughout the system, so pressure differences do not depend on it.

ID:(2210, 0)



Connecting two liquid columns

Concept

>Top


If two columns of water with different heights at their bases are connected, a situation arises where there is a pressure difference along the connecting tube.

This setup allows us to study how the pressure difference generates a liquid flow along the tube. We can consider an element of liquid with a certain length and a section equal to that of the tube, and estimate the corresponding mass using the density. With the section, we can also convert the pressure difference into a force difference and, ultimately, study how volumes in liquids are accelerated due to pressure differences.

ID:(933, 0)



Model

Concept

>Top



Variables

Symbol
Text
Variables
Units
$F$
F
Column force
N
$h$
h
Column height
m
$S$
S
Column Section
m^2
$V$
V
Column volume
m^3
$h_1$
h_1
Height or depth 1
m
$h_2$
h_2
Height or depth 2
m
$\Delta h$
Dh
Height or depth difference
m
$M$
M
Mass of liquid column
kg
$p_1$
p_1
Pressure in column 1
Pa
$p_2$
p_2
Pressure in column 2
Pa
$S$
S
Section or Area
m^2
$p_t$
p_t
Total pressure
Pa
$V$
V
Volume
m^3
$p_t$
p_t
Water column pressure
Pa

Parameters

Symbol
Text
Variables
Units
$p_0$
p_0
Atmospheric pressure
Pa
$g$
g
Gravitational Acceleration
m/s^2
$\rho_w$
rho_w
Liquid density
kg/m^3


Selected parameter

Symbol
Variables
Value
Units
MKS Value
MKS Units

Calculations

Symbol
Equation
Solved
Translated

Equation

#
Equation

$ \Delta h = h_2 - h_1 $

Dh = h_2 - h_1


$ \Delta p = p_2 - p_1 $

Dp = p_2 - p_1


$ \Delta p = \rho_w g \Delta h $

Dp = rho_w * g * Dh


$ F = S h \rho_w g $

F = S * h * rho_w * g


$ M = \rho_w S h $

M = rho_w * S * h


$ p \equiv\displaystyle\frac{ F }{ S }$

p = F / S


$ p = p_0 + \rho_w g h $

p = p_0 + rho_w * g * h


$ p = \rho_w g h $

p = rho_w * g * h


$ \rho_w = \displaystyle\frac{ M }{ V }$

rho_w = M / V


$ V = S h $

V = S * h

ID:(15220, 0)



Volume of the column

Equation

>Top, >Model


The column volume ($V$) is determined by the column Section ($S$) and the column height ($h$), and it is calculated as follows:

$ V = S h $

$h$
Column height
$m$
$S$
Column Section
$m^2$
$V$
Column volume
$m^3$



as long as the column Section ($S$) remains constant throughout the column height ($h$).

The section may change in its shape but not in its surface.

ID:(931, 0)



Density of a liquid

Equation

>Top, >Model


The the liquid density ($\rho_w$) is calculated from the mass of liquid column ($M$) and the column volume ($V$) using the equation:

$ \rho_w = \displaystyle\frac{ M }{ V }$

$\rho_w$
Liquid density
$kg/m^3$
$M$
Mass
$kg$
$V$
Volume
$m^3$

ID:(15091, 0)



Water column mass

Equation

>Top, >Model


Using the liquid density ($\rho_w$), the column Section ($S$), and the column height ($h$), you can calculate the mass of liquid column ($M$) with the formula:

$ M = \rho_w S h $

$h$
Column height
$m$
$S$
Column Section
$m^2$
$\rho_w$
Liquid density
$kg/m^3$
$M$
Mass of liquid column
$kg$

The mass of liquid column ($M$) can be calculated from the liquid density ($\rho_w$) and the column volume ($V$).

To calculate the liquid density ($\rho_w$), the following equation is used:

$ \rho_w = \displaystyle\frac{ M }{ V }$



And for the column volume ($V$), the equation is:

$ V = S h $



This way, the value of the mass of liquid column ($M$) is obtained by:

$ M = \rho_w S h $



This is valid as long as the column Section ($S$) remains constant throughout the column height ($h$).

The section may change in its shape, but not in its surface.

ID:(4340, 0)



Water column force

Equation

>Top, >Model


The mass of liquid column ($M$) exerts a force on its base due to the gravitational force acting upon it. This force can be calculated using the formula:

$ F_g = m_g g $



where 'm' is the mass of the liquid column, and 'g' is the acceleration due to gravity. Therefore, the the column force ($F$) generated by the mass of liquid column ($M$) is given by:

$ F = S h \rho_w g $

$F$
Column force
$N$
$h$
Column height
$m$
$S$
Column Section
$m^2$
$g$
Gravitational Acceleration
9.8
$m/s^2$
$\rho_w$
Liquid density
$kg/m^3$

As the mass of liquid column ($M$) depends on the liquid density ($\rho_w$), the column Section ($S$), and the column height ($h$) in the following manner:

$ M = \rho_w S h $



and the gravitational force is represented as:

$ F_g = m_g g $



the expression can be written as:

$ F = S h \rho_w g $

.

ID:(4248, 0)



Definition of pressure

Equation

>Top, >Model


To model the motion of liquid elements, it is necessary to move from a point-force and mass view to elements of volume exposed to forces on one of their faces and mass calculated with density.

Therefore, pressure is defined as force per unit area and is calculated using:

$ p \equiv\displaystyle\frac{ F }{ S }$

$F$
Force of the medium
$N$
$p$
Pressure
$Pa$
$S$
Section or Area
$m^2$

where P is pressure, F is force, and A is the area on which the force acts. The unit of pressure in the International System of Units is the pascal (Pa), which is defined as one newton per square meter (N/m²). Pressure can vary depending on depth, height of the liquid column, and other factors.

ID:(4342, 0)



Pressure of a column

Equation

>Top, >Model


If we consider the expression of the column force ($F$) and divide it by the column Section ($S$), we obtain the water column pressure ($p_t$). In this process, we simplify the column Section ($S$), so it no longer depends on it. The resulting expression is:

$ p = \rho_w g h $

$h$
Column height
$m$
$g$
Gravitational Acceleration
9.8
$m/s^2$
$\rho_w$
Liquid density
$kg/m^3$
$p$
Water column pressure
$Pa$

Since the force generated by a column of liquid is given by

$ F = S h \rho_w g $



and pressure is defined as

$ p \equiv\displaystyle\frac{ F }{ S }$

,

the pressure generated by a column of liquid is given by

$ p = \rho_w g h $

.

ID:(4249, 0)



Atmospheric pressure column pressure

Equation

>Top, >Model


When calculating the water column pressure ($p_t$) at a certain depth, it's important to consider that the liquid's surface is exposed to the atmospheric pressure ($p_0$), which can affect the pressure value at that point. Therefore, it's necessary to generalize the equation for the water column pressure ($p_t$) to include not only the liquid column the liquid density ($\rho_w$), the column height ($h$), and the gravitational Acceleration ($g$) but also the atmospheric pressure ($p_0$):

$ p = p_0 + \rho_w g h $

$p_0$
Atmospheric pressure
$Pa$
$h$
Column height
$m$
$g$
Gravitational Acceleration
9.8
$m/s^2$
$\rho_w$
Liquid density
$kg/m^3$
$p_t$
Total pressure
$Pa$

ID:(4250, 0)



Height difference

Equation

>Top, >Model


When two liquid columns are connected with the height of liquid column 1 ($h_1$) and the height of liquid column 2 ($h_2$), a the height difference ($\Delta h$) is formed, which is calculated as follows:

$ \Delta h = h_2 - h_1 $

$h_1$
Height or depth 1
$m$
$h_2$
Height or depth 2
$m$
$\Delta h$
Height or depth difference
$m$



the height difference ($\Delta h$) will generate the pressure difference that will cause the liquid to flow from the higher column to the lower one.

ID:(4251, 0)



Pressure difference

Equation

>Top, >Model


When two liquid columns are connected with the pressure in column 1 ($p_1$) and the pressure in column 2 ($p_2$), a the pressure difference ($\Delta p$) is formed, which is calculated according to the following formula:

$ \Delta p = p_2 - p_1 $

$p_1$
Pressure in column 1
$Pa$
$p_2$
Pressure in column 2
$Pa$
$\Delta p$
Variación de la Presión
$Pa$



the pressure difference ($\Delta p$) represents the pressure difference that will cause the liquid to flow from the taller column to the shorter one.

ID:(4252, 0)



Pressure difference between columns

Equation

>Top, >Model


The height difference, denoted by the height difference ($\Delta h$), implies that the pressure in both columns is distinct. In particular, the pressure difference ($\Delta p$) is a function of the liquid density ($\rho_w$), the gravitational Acceleration ($g$), and the height difference ($\Delta h$), as follows:

$ \Delta p = \rho_w g \Delta h $

$g$
Gravitational Acceleration
9.8
$m/s^2$
$\Delta h$
Height or depth difference
$m$
$\rho_w$
Liquid density
$kg/m^3$
$\Delta p$
Variación de la Presión
$Pa$

If there is the pressure difference ($\Delta p$) between two points, as determined by the equation:

$ \Delta p = p_2 - p_1 $



we can utilize the water column pressure ($p_t$), which is defined as:

$ p = p_0 + \rho_w g h $



This results in:

$\Delta p=p_2-p_1=p_0+\rho_wh_2g-p_0-\rho_wh_1g=\rho_w(h_2-h_1)g$



As the height difference ($\Delta h$) is:

$ \Delta h = h_2 - h_1 $



the pressure difference ($\Delta p$) can be expressed as:

$ \Delta p = \rho_w g \Delta h $

ID:(4345, 0)