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Vorticity and Jets

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Vorticity and Jets
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METR 2413

12 April 2004









Vorticity and Jets

Review from quiz

Review



dp

Hydrostatic balance    g,

dz

Vertical pressure gradient force - 1 dp  g

 dz

Scale, g ~ 10 m/s2, vertical pgf ~ 10 m/s2



Horizontal pressure gradient force balanced by Coriolis force

1 p

 f cv

 x

f ~ 10-4 s-1, v ~ 10 m/s, Coriolis force ~ 10-3 m/s2

ρ ~ 1 kg/m3, Δp ~ 10 hPa ~ 1000 Pa, Δx ~ 1000 km ~ 106 m

Review from quiz

Thermal wind





In the presence of a horizontal temperature gradient,

the tilt of pressure surfaces increases with height.



u g g Tv



z f cTv y ug p=p2



Δz

p=p1





North

cold warm

Zonal wind increases with height in the NH because temperature decreases

towards the pole, giving increasing poleward height gradients.

Circulation and Vorticity:

Two primary measures of rotation in a fluid



By convention, both circulation and vorticity are positive in

the counterclockwise direction

(cyclonic in the Northern Hemisphere)



Circulation: Macroscopic measure of rotation for a finite

area of the fluid

= integration of the tangential component of velocity around

a closed path



Vorticity: The tendency to spin about an axis; Microscopic

measure of rotation at any point in the fluid

The tighter the spin, the larger the magnitude of the vorticity









On Earth there is:

1) Vorticity from Earth’s spin (planetary vorticity)

2) “Local” vorticity due to cyclonic/anticyclonic motion

(relative vorticity)

Absolute vorticity (total vorticity):

• measured with respect to the fixed stars

• includes Earth’s rotation (planetary vorticity) and

rotation of atmosphere relative to Earth’s surface (relative

vorticity)

• angular momentum is conserved, so absolute vorticity is

also conserved for frictionless motion



ζ a = ζ r + fc = constant



where f c is the Coriolis parameter = 2Ω sinΦ

(planetary vorticity)

Relative vorticity:

• measure of the rotation of the atmosphere about a vertical

axis relative to Earth’s surface

• units of sec-1

• Synoptic scale vorticity is analyzed and plotted on the 500

mb chart

• 500 mb vorticity may be referred to as “vertical vorticity”

(the spin is in relation to the vertical axis)



The vertical component of vorticity can be expressed as:

ζr = ∂v/∂x – ∂u/∂y

Typical magnitude of the relative vorticity for synoptic scale

flow, U ~ 10 m/s, L ~ 1000 km



ζ = ∂v/∂x - ∂u/ ∂y ≤ U/L ~ 10-5 sec-1



Typical magnitude of planetary vorticity f ~ 10-4 s-1

We’ve seen that relative vorticity is non-zero for two reasons:

1) Either streamlines of wind have curvature, or

2) The wind field has horizontal shear (or both)



Curvature vorticity: positive in troughs and negative in ridges

Positive and negative relative shear vorticity can be due to variations in

westerly wind speed with latitude



slow



Positive shear vorticity



fast









fast







slow Negative shear vorticity



Think of the above air flows as wide rivers – if you put a log oriented north-

south in the flow, the log would turn counterclockwise on the top, and

clockwise on the bottom because of the shear

Positive vorticity advection (PVA)

• found where air blows from regions of higher vorticity toward

lower vorticity

• significant because main mechanism to reduce vorticity is

divergence

• that is, in regions of PVA there tends to be divergence, which

implies upward motions beneath these areas, surface

convergence and surface pressure falls



Negative vorticity advection (NVA)

 found where air blows from regions of lower vorticity towards

higher vorticity

 main mechanism to increase vorticity is convergence

 when there is NVA in upper levels, there tends to be

downward motion below, surface divergence and surface

pressure rises

Low Vorticity Low Vorticity



Upper Level

Convergence









High Vorticity









Anticyclonic Vorticity Advection

- Moving from low vorticity to high vorticity requires

convergence aloft.

Jet streaks

• Jet streaks are localized regions of very fast winds

embedded within the jet stream. Sometimes these local

wind maxima reach speeds in excess of 160 knots.

• Jet streaks are important as they are indicative of rising

motion/falling pressures at the surface. The figure below

represents an idealized jet streak.

Height contour









Entrance Exit

Region Region

(Rear) (Front)



As air enters from the left, it must be accelerated as the height contours

are closer together and the pressure gradient force is stronger.

The stronger pgf causes an ageostrophic flow to the north, leading to

convergence to the north and a divergence to the south. As a result, air

sinks in the northern 'quadrant', and rises in the southern quadrant of a jet

entrance.

The force to accelerate the flow to the east is supplied by the Coriolis

force as air flows from the south to the north near the jet entrance,

leading to a force to the east (the right).

In the jet exit region, the opposite happens, as air flows from

north to south to create the force necessary to decelerate

the air as it leave the jet streak. The vertical motion resulting

from this leads to rising air in the north quadrant and sinking

air in the south of the jet exit.

CONV DIV





Exit

Entrance

Region

Region

(Front)

(Rear)



However, not all jet streaks are straight. In fact, most are

curved.

The ageostrophic flow and anticyclonic vorticity advection

cause convergence in the left entrance of the jet and the

ageostrophic flow and the cyclonic vorticity advection cause

divergence in the left exit region

The divergence and ascent ahead of the upper level trough

enhance the development of surface lows

Summary

• Vorticity is a measure of the local rotation in a fluid

• Planetary vorticity due to the rotoation of the earth

• Relative vorticity due to the rotation of air relative to the

surface, curvature vorticity and shear vorticity

• Absolute vorticity = planetary vorticity + relative vorticity

is conserved in the atmosphere

• Positive (cyclonic) vorticity advection leads to upper level

divergence, and rising motion

• Jet streaks are localized regions of very strong winds,

with poleward motion at the jet entrance and

equatorward flow at the jet exit

• Enhanced divergence at the left exit region of a cyclonic

curved jet, enhances development of surface low


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