Vaisala-Brunt Oscillation

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>Model

ID:(1525, 0)



BruntVäisälä frequency

Video

If a medium exhibits stratification, meaning it consists of layers with different densities, there is a possibility that the density difference becomes unstable, causing the layers to mix and the system to become homogeneous.

As long as the system remains stable, any disturbance will lead to oscillations that dissipate over time. The frequency associated with this behavior is known as the Brunt-Väisälä frequency, which exists in both the atmosphere and the ocean.

The following video shows a system with two different densities, where a cork is placed and oscillates in response to a disturbance, maintaining the order between the stable layers:

ID:(11754, 0)



Vaisala-Brunt Oscillation

Model

Variables

Symbol
Text
Variable
Value
Units
Calculate
MKS Value
MKS Units
$N$
N
Brunt-Väisälä frequency
Hz
$H$
H
Characteristic height
m
$R$
R
Characteristic size
m
$f$
f
Coriolis factor
rad/s
$\rho$
rho
Density
kg/m^3
$\Delta\rho$
Drho
Density variation
kg/m^3
$C_p$
C_p
Heat capacity at constant pressure
J/kg
$\Delta z$
Dz
Height variation
m
$U$
U
Horizontal speed
m/s
$\theta$
theta
Potential temperature
K
$\Delta\theta$
Dtheta
Potential temperature variation
K
$p$
p
Pressure
Pa
$p_{ref}$
p_ref
Reference pressure
Pa
$Re$
Re
Reynolds number
-
$\lambda_R$
lam_R
Rossby Radio
m
$T$
T
Temperature
K

Calculations


First, select the equation:   to ,  then, select the variable:   to 

Symbol
Equation
Solved
Translated

Calculations

Symbol
Equation
Solved
Translated

 Variable   Given   Calculate   Target :   Equation   To be used



Equations

The energy associated with the Coriolis force can be estimated by considering the Coriolis force and a characteristic length $L$. The Coriolis force is the product of mass $m$, the Coriolis factor $f$, and velocity $U$. On the other hand, the energy associated with the inertial force is simply the kinetic energy proportional to $mU^2$.

Based on this, the Rossby number is defined as:

$R_0 = \displaystyle\frac{m U^2}{ m f U L}$



Thus, the Rossby number represents the ratio between the fluid's kinetic energy and the effect of the Coriolis force.

$ R_0 =\displaystyle\frac{ U }{ f R }$

(ID 11753)

For the case in which the Rossby number

$ R_0 =\displaystyle\frac{ U }{ f R }$



with $U$ representing velocity, $f$ as the Coriolis factor, and $L$ as a characteristic length, which is of the order of unity, we can determine that the characteristic length is approximately given by:

$L \sim \displaystyle\frac{U}{f}$



The velocity $U$ can be modeled using the Brunt-V is l frequency

$ N = \sqrt{\displaystyle\frac{ g }{ \theta }\displaystyle\frac{ \Delta\theta }{ \Delta z }}$



where $g$ is the gravitational acceleration, $\Delta\theta/\theta$ represents the variation in potential temperature, and $\Delta z$ is the variation in height. In this case, the velocity can be expressed as:

$U\sim H N$



where $H$ denotes the height. Thus, the characteristic size can be obtained as:

$ \lambda_R = \displaystyle\frac{ N H }{ f }$

(ID 11760)


Examples

If a medium exhibits stratification, meaning it consists of layers with different densities, there is a possibility that the density difference becomes unstable, causing the layers to mix and the system to become homogeneous.

As long as the system remains stable, any disturbance will lead to oscillations that dissipate over time. The frequency associated with this behavior is known as the Brunt-V is l frequency, which exists in both the atmosphere and the ocean.

The following video shows a system with two different densities, where a cork is placed and oscillates in response to a disturbance, maintaining the order between the stable layers:

(ID 11754)


ID:(1525, 0)