CLIMATE/EARTH 401�Geophysical Fluid Dynamics�Dynamical Meteorology
Analysis Barotropic Wave: Problem
An equation for geopotential tendency
Start with the QG �vorticity equation
Use the definition of geostrophic wind
Plug this in, and we immediately have an equation for the time rate of change of the geopotential height
Consider a barotropic fluid
Form a perturbation equation
Barotropic height tendency equation
Divide wind into mean and perturbation, assume no mean north/south wind. The mean is taken around circle of latitude (zonal mean)
Substitute mean and perturbation, take average, form perturbation equation after linearizing.
Assume a “wave like solution”
Dispersion relation. Relates frequency and wave number to flow. Must be true for waves.
Stationary wave?
Wind must be positive, from the west, for a wave.
Think about this from a vorticity perspective
Rewrite the QG vorticity equation
Expand material derivative
Rewrite the QG vorticity equation
Use the
continuity equation
Combine the advection terms
Rewrite the QG vorticity equation
Advection of vorticity
Consider the vorticity advection
Advection of vorticity
Advection of relative vorticity
Advection of planetary vorticity
Exercise: Explore the role of wavelength more quantitatively
Assume that the geopotential takes the form of a wave
Horizontal wavenumber
Mean Ф Gradient in y
Wave
Mean
Use the relationship between geostrophic wind and geopotential
Using the proposed solution on previous page. Write out ug and vg
Divide the geostrophic wind into mean and perturbation
Divide wind into zonal mean and perturbation, assume no mean north/south wind.
Using the proposed wave-like solution, identify the mean and perturbation winds.
Prove that the zonal average of the perturbation is zero.
Plug our results into the advection of relative vorticity
Using the results from previous, calculate the advection of relative vorticity.
Plug our results into the advection of planetary vorticity
Using the results from previous, calculate the advection of planetary vorticity.
Compare advection of planetary and relative vorticity
For a wave with meridional wavelength of 1000 km, U = 10 m/sec, at what zonal wavelength are the relative and planetary vorticity of the same magnitude?
Compare advection of planetary and relative vorticity
Consider the geopotential tendency
For the zonal wavelength calculated in the previous question:
Consider these idealized charts
Geopotential Map (Northern Hemisphere)
Φ0 - ΔΦ
Φ0 + ΔΦ
Φ0
ΔΦ > 0
A
B
C
٠
٠
٠
x, east
y, north
L
L
H
Where is geostrophic approximation most accurate?
Where is the ageostrophic wind the strongest?
What is the sign of the geostrophic wind?
*
w
Geopotential Map (Northern Hemisphere)
ΔΦ > 0
A
B
C
٠
٠
٠
x, east
y, north
L
L
H
Φ0 - ΔΦ
Φ0 + ΔΦ
Φ0
*
w
At points A, B, C:
Geopotential Map (Northern Hemisphere)
ΔΦ > 0
A
B
C
٠
٠
٠
x, east
y, north
L
L
H
At Point W,
Φ0 - ΔΦ
Φ0 + ΔΦ
Φ0
*
w
End: Analysis Barotropic Wave: Problem