Title: The General Circulation of the Atmosphere
1The General Circulation of the Atmosphere
2Overview
- Definitions
- Potential Temperature
- Stream function
- Vorticity
- Angular Momentum
- Rossby number
- Geostrophic wind
- Gradient wind
- Baroclinic Instability
- Turbulence Eddies
- Hides Theorem
3Definitions
Inviscid Flow A fluid flow where viscous
(friction) forces are small in comparison to
inertial forces.
Meridional Along a meridian (N-S).
Zonal Along a latitude circle (E-W).
Axisymmetric Symmetrical about the axis of
planetary rotation that is, zonally symmetric
4Definitions
Reversible Process A processe which can be
reversed by means of infinitesimal changes in
some property of the system without loss or
dissipation of energy
Isentropic Process A process in which the
entropy of the system remains constant. It is
both adiabatic and reversible.
Macroturbulence Totality of irregular motions
of large scale eddies, characterised by a small
Rossby number.
Advection The horizontal movement of air or
atmospheric properties, solely by the motion of
the atmosphere
5Potential Temperature (?)
- The temperature an air parcel will have if
adiabatically and reversibly moved to a reference
pressure level p0. - For an ideal gas
- A conserved property for all dry adiabatic
processes.
6Stream Function
- A function whose contours are stream lines
- Helpful for visualization (i.e. plots)
- In 2D
7Angular Momentum
- For an air parcel in the atmosphere on a rotating
planet - M (O a cos(?) u ) a cos(?)
-
- a radius of planet
- O angular rotation rate
- ? latitude
- u zonal velocity
- Conserved, since tidal forces negligible
- Coriolis force deflects to the right in NH
conservation of angular momentum
8Vorticity
- ? ? x u
- Measures amount of rotation in a flow
- Can separate into 2 components
- planetary vorticity f 2 O cos(?)
- relative vorticity ? -(??(u cos ?)) / (a cos
?)
9Rossby number
- Measure of the relative importance of rotation
and advection - -or- of the importance of planetary vorticity vs.
relative vorticity - Ro U / fL
- f 2 O cos(?) (Coriolis parameter)
- U velocity scale
- L length scale
- Ro ltlt 1 Rotation dominant
- Ro 1 Rotation and advection important
- Ro gtgt 1 Advection dominant
10Geostrophic Wind
- If Ro ltlt1 and friction can be neglected gt
- Geostrophy Pressure gradient force balances
Coriolis force - Atmosphere is geostrophic to first approximation
- Wind is along pressure contours (pressure is
essentially the stream function for velocity)
11Gradient Wind
- Gradient-wind geostrophy centrifugal force
- adds a correction to geostrophic velocities,
depending on orientation of feature rotation
relative to planetary rotation -
12Baroclinic Instability
- Important for flows with Ro ltlt1
- How does differential heating of poles vs.
equator affect atmospheric flow?
http//www.gps.caltech.edu/tapio/papers/annrev06_
supp.html
13Turbulence Eddies
- Turbulence as a diffusive process
- Generally, turbulence occurs at all scales
- Often expressed as rotating structures (eddies)
- Cyclones an example of large-scale eddies
- can transfer energy from small to large scale
(inverse energy cascade)
14Hides Theorem
- Axisymmetry Diffusion of angular momentum (eg.
from small scale turbulence) - No extremum of angular momentum away from
boundaries - zonal winds weaker than that at surface
- Surface wind determined by boundary conditions
- M lt O a2
- u lt um Oa sin2 (?)/cos(?)
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