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AOSS 401, Fall 2006 Lecture 18 October 24, 2007 Richard B. Rood (Room 2525, SRB) [email protected] 734-647-3530 Derek Posselt (Room 2517D, SRB) [email protected] 734-936-0502

AOSS 401, Fall 2006 Lecture 18 October 24 , 2007

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AOSS 401, Fall 2006 Lecture 18 October 24 , 2007. Richard B. Rood (Room 2525, SRB) [email protected] 734-647-3530 Derek Posselt (Room 2517D, SRB) [email protected] 734-936-0502. Class News. Final exam will be last day of class - PowerPoint PPT Presentation

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Page 1: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

AOSS 401, Fall 2006Lecture 18

October 24, 2007

Richard B. Rood (Room 2525, SRB)[email protected]

734-647-3530Derek Posselt (Room 2517D, SRB)

[email protected]

Page 2: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Class News

• Final exam will be last day of class

• Derek and I decided to think about good homework problems for another day.– No homework posted today.

Page 3: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Material from Chapter 4

• Vorticity, Vorticity, Vorticity

– Relative and planetary vorticity– Mid-latitude disturbances– Vorticity, divergence, in 3-D

Page 5: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Two important definitions

• barotropic – density depends only on pressure. And by the ideal gas equation, surfaces of constant pressure, are surfaces of constant density, are surfaces of constant temperature.

• baroclinic – density depends on pressure and temperature.

Page 6: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Absolute (or total) Vorticity

fy

u

x

veartha

vorticityabsolute

vorticityrelativevorticityplanetary vorticityabsolute

ukukUk

Page 7: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Relative and planetary vorticity

• Planetary vorticity is cyclonic is positive vorticity

• Planetary vorticity, in middle latitudes, is usually larger than relative vorticity

Page 8: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

We derived the vorticity equation

x

p

yy

p

x

z

u

y

w

z

v

x

w

y

v

x

uf

y

fv

t

11

)(

))((u

TERMS

DIVERGENCE

TILTING

SOLENOIDAL or

BAROCLINIC

Page 9: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Comments on the terms

• There are important dynamical features in the atmosphere where all of these terms are important.

• Baroclinic terms are due to there being gradients of temperature on pressure surfaces. (Are they explicitly there in pressure coordinates?) Like a thermodynamic “source” of rotation.

Page 10: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Tilting Term

rotation in, say, (y, z)

plane, “vorticity” in x

plane

as the wheel is turned there is a

component of “vorticity” in the z

plane

Page 11: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Divergence influence on vorticity

Page 12: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Divergence influence on vorticity

Page 13: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Scale factors for “large-scale” mid-latitude

s 10 /

m 10

m 10

! s cm 1

s m 10

5

4

6

1-

-1

UL

H

L

unitsW

U

1-1-11-

14-0

2

3-

sm10

10

10/

m kg 1

hPa 10

y

f

sf

P

Page 14: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Assume balance among terms of 10-10s-2

)(

0)(

y

v

x

uf

y

fv

yv

xu

t

y

fv

y

v

x

uf

yv

xu

t

Page 15: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

A nuance on vorticity and the scaled equation: potential vorticity

Page 16: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

A simple version of potential vorticity

0)( H

f

Dt

Dhorizontal

Integrate with height,z1 z2 over a layer of depth H.

Page 17: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

A simple version of potential vorticity

vorticitypotentialH

f

This is the potential vorticity under the set of assumptions that we used to derive the equation. Constant density, constant temperature so only in a shallow layer might this be relevant to the atmosphere.

Potential vorticity is a measure of absolute vorticity relative to the depth of the vortex.

Page 18: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Relative vorticity with change of depth

Page 19: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Vorticity and depth

• We can see that there is a relationship between depth and vorticity.

• As the depth of the vortex changes, the relative vorticity has to change in order to conserve the potential vorticity.

• This is the play between relative and planetary vorticity.

Page 20: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Scaled vorticity equation

))(()(

y

v

x

uf

Dt

fDhorizontal

Page 21: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

An observation

• The vorticity is dominated by the geostrophic component of the wind.

• The divergence requires the wind to be away from geostrophic balance.

• Generally vg/va >= 10

Page 22: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Let’s explicitly map these ideas to the Earth

Page 23: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Local vertical / planetary vorticity

Page 24: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

relative vorticity/planetary vorticity

relative vorticity

planetary vorticity

Page 25: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Compare relative vorticity to planetary vorticity

NumberRossby Ro

10

10

10

0

1

0

140

15

Lf

U

f

sf

sL

U

planetary vorticity

is usually larger than

relative vorticity

for large-scale and

middle latitudes

Page 26: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Relative and planetary vorticity

• Planetary vorticity is cyclonic is positive vorticity• Planetary vorticity, in middle latitudes, is usually

larger than relative vorticity• A growing cyclone “adds to” the planetary

vorticity.– Lows intense

• A growing anticyclone “opposes” the planetary vorticity.– Highs less intense

Page 27: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Compare relative vorticity to planetary vorticity and

to divergence

100

10

10

0

0

yv

xuf

yv

xu

f

Flow is rotationally dominated, but divergence is crucial to understanding

flow.

Page 28: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Consider our simple form of potential vorticity

vorticitypotential

0)(

H

fH

f

Dt

Dhorizontal

From scaled equation, with assumption of constant density and temperature.

Page 29: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Fluid of changing depth

Page 30: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Two things that we have learned about vorticity.

• Convergence and divergence in a column of fluid, impacts the vorticity throughout the column.– Specifically, divergence above causes low

pressure at the surface.

• Stretching and shrinking of a column of vorticity will change the relative vorticity.

Page 31: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Possible development of a surface low.

Earth’s surface

pressure surfaces

Page 32: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

pressure surfaces

warming

cooling

Page 33: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

pressure / height

surfacesrisewarming

cooling

pressure / height

surfacessink

Page 34: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warming

cooling

PGF H

L

Page 35: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warming

cooling

PGF H

L mass leaves

column / low forms at groundL

Page 36: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warming

cooling

PGF H

L mass leaves

column / low forms at groundL

mass enters column / high

forms at ground

H

Page 37: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warming

cooling

PGF H

L mass leaves

column / low forms at groundL

mass enters column / high

forms at ground

H PGF

Page 38: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Mass continuity?

• What are the implications of mass continuity?

• What is your law, your equation, your tool to answer that question?

Page 39: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Temperature

• Assuming the air moves isentropically, what happens to the temperature?

• What is your law, your equation, your tool to answer that question?

Page 40: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warming

cooling

PGF H

L

LH PGF

Page 41: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Simple Thermal Circulation

• There is the sense of the air moves to counter the heating.

• If the heating ended, then the circulation would end, acting to bring back the original equilibrium situation.

• This sort of low is cause by heating, is called a “thermal” low, warm core. It tends to damp out.

Page 42: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warmcore

coldcore

PGFHL

LH PGF

Page 43: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Simple Thermal Circulation

• This sort of low is cause by heating, is called a “thermal” low, warm core. It tends to damp out.– Remember the question about the hurricane

being warm core.

• What about the divergence and convergence?

Page 44: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Lets return to our simple problem

Earth’s surface

warmcore

coldcore

PGF HL

LH PGF

DIVERGENCE

CONVERGENCE

CONVERGENCE

DIVERGENCE

Page 45: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Simple Thermal Circulation

• What about the divergence and convergence?– Convergence and Divergence are aligning

over top of each other in the vertical.– Again, in this case there is a tendency for the

circulation to damp out.

Page 46: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Back to the earth again

Page 47: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Still in the atmosphere

Page 48: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Flow over a hill

HILL

Page 49: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Derived a simple form of potential vorticity

vorticitypotential

0)(

H

fH

f

Dt

Dhorizontal

From scaled equation, with assumption of constant density and temperature.

Page 50: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Flow over a hill(long in the north-south)(can’t go around the hill)

west east

Page 51: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Flow over a hill

HILL

west east

Dep

th,

H

Page 52: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Flow over a hill(assume flow is adiabatic)

HILL

west east

Dep

th,

H

θ

θ + Δθ

Page 53: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Flow over a hill(far upstream constant zonal flow)

HILL

west east

Dep

th,

H

θ

θ + Δθ

ζ=0

Page 54: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Derived a simple form of potential vorticity

vorticitypotential

0)(

H

fH

f

Dt

Dhorizontal

From scaled equation, with assumption of constant density and temperature.

Page 55: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air gets to hill?

HILL

west east

Dep

th,

H

θ

θ + Δθ

ζ=0

Page 56: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air gets to hill?

HILL

west east

Dep

th,

H

θ

θ + Δθ

ζ=0

Air is lifted. Lifting higher at ground than upper air.(pressure gradient force spreads it out)

Page 57: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air gets to hill?

HILL

west east

Dep

th,

H +ΔH

θ

θ + Δθ

ζ=0

Air is lifted. Lifting higher at ground than upper air.(pressure gradient force spreads it out)

Page 58: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air gets to hill?

HILL

west east

Dep

th,

H +ΔH

θ

θ + Δθ

ζ must increase

Air is lifted. Lifting higher at ground than upper air.(pressure gradient force spreads it out)

Page 59: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

How does vorticity increase?

Page 60: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens in these waves?

Gains cyclonic vorticity

Loses cyclonic vorticitySame as gains

anticyclonic vorticity

Page 61: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Or schematically

Cyclonic Anticyclonic

Rotational

Shear

Page 62: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air gets to hill?

HILL

west east

Dep

th,

H +ΔH

θ

θ + Δθ

ζ must increase

Air turns cyclonically to increase vorticity.In northern hemisphere turns north.

Page 63: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

In the (east-west, north-south) planeD

epth

, H

Dep

th,

H +ΔH

west easts

n

Page 64: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air goes over hill?

HILL

west east

Dep

th,

H -ΔH

θ

θ + Δθ

Air turns anti-cyclonically to decrease vorticity.In northern hemisphere turns south.

ζ must decrease

Page 65: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

In the (east-west, north-south) planeD

epth

, H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Page 66: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens as air goes down hill?

HILL

west eastD

epth

, H

+ΔH

θ

θ + Δθ

Air turns cyclonically to increase vorticity.In northern hemisphere turns north.

ζ must increase

Page 67: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

In the (east-west, north-south) planeD

epth

, H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Dep

th,

H +ΔH

Page 68: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What is happening with planetary vorticity?(In the (east-west, north-south) plane)

Dep

th,

H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Dep

th,

H +ΔH

f is greater for deflections to north

f is less for deflections to south

Page 69: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What is happening with planetary vorticity?(In the (east-west, north-south) plane)

Dep

th,

H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Dep

th,

H +ΔH

f + ζ is less than earth’s vorticity and wants to turn north.

Arrives here wanting vorticity. “Overshoots”

Page 70: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What is happening with planetary vorticity?(In the (east-west, north-south) plane)

Dep

th,

H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Dep

th,

H +ΔH

Page 71: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What happens if wind is from east?

HILL

west east

θ

θ + Δθ

Page 72: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

What is happening with planetary vorticity?(In the (east-west, north-south) plane)

Dep

th,

H

Dep

th,

H +ΔH

west easts

n Dep

th,

H -ΔH

Dep

th,

H +ΔH

Flow from east planetary and relative vorticity interact together, no overshoot or undershoot.

Page 73: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Excursion into the atmosphere

Page 74: AOSS 401, Fall 2006 Lecture  18 October  24 , 2007

Middle latitude cyclones