A Rotational View of the Atmoshere Chapter...

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A Rotational View of the Atmoshere

Chapter 4

Paul A. Ullrich

paullrich@ucdavis.edu

Part 2: The Vorticity Equation

Vorticity: Key Questions

Question: How is positive / negative vorticity generated?

Question: How do we describe the time rate of change of vorticity?

Question: How do we describe conservation of vorticity? Is vorticity actually conserved following the flow?

Question: What is the role of the Earth’s rotation?

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Start from the scaled horizontal momentum equation in z coordinates, no viscosity:

Take derivatives on both sides and compute:

The Vorticity Equation

Du

Dt

= �1

@p

@x

+ fv

Dv

Dt

= �1

@p

@y

� fu

@

@x

✓Dv

Dt

◆� @

@y

✓Du

Dt

◆@

@x

✓Dv

Dt

◆=

@

@x

✓@v

@t

+ u ·rv

@

@y

✓Du

Dt

◆=

@

@y

✓@u

@t

+ u ·ru

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

� @

@y

@u

@t

� @

@y

(u ·ru) = +@

@y

✓1

@p

@x

◆� @

@y

(fv)

+@

@x

@v

@t

+@

@x

(u ·rv) = � @

@x

✓1

@p

@y

◆� @

@x

(fu)

@⇣

@t

+ u ·r⇣ + (⇣ + f)

✓@u

@x

+@v

@y

+

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆+ v

@f

@y

= � @

@x

✓1

◆@p

@y

+@

@y

✓1

◆@p

@x

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

The Vorticity Equation

A  rather  long  deriva/on  

@⇣

@t

+ u ·r⇣ + (⇣ + f)

✓@u

@x

+@v

@y

+

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆+ v

@f

@y

= � @

@x

✓1

◆@p

@y

+@

@y

✓1

◆@p

@x

D

Dt

(⇣ + f) = �(⇣ + f)(rh · u)�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� (r↵⇥rp) · k

↵ =1

⇢With specific volume

Vorticity Equation

The Vorticity Equation

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

What are these terms?

The Vorticity Equation

Rate of change of the absolute vorticity following the motion

D

Dt

(⇣ + f) = �(⇣ + f)(rh · u)�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� (r↵⇥rp) · k

Divergence term Tilting or twisting term Solenoidal term

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

•  Remember that divergence is related to vertical motion (column integrated divergence gives the local vertical velocity)

•  We now see that it is also related to changes in vorticity…

�(⇣ + f)(rh · u)

The Vorticity Equation Take a closer look at the divergence term…

Absolute vorticity Horizontal divergence

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

d� = �✓⇥u

⇥x+

⇥v

⇥y

p

dp

Z �@ p=0

�@ ps

d� = �Z p=0

ps

✓⇥u

⇥x+

⇥v

⇥y

p

dp

�(p = 0)� �(ps) = �Z p=0

ps

✓⇥u

⇥x+

⇥v

⇥y

p

dp

�(ps) = �Z ps

p=0(⇥p · u)dp

Vertical Velocity Obtained from horizontal divergence

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

✓@u

@x

+@v

@y

p

+@!

@p

= 0

Continuity Equation in Pressure Coordinates

Vorticity and Divergence

Changes in vorticity are partially driven by divergence of the horizontal wind.

Vertical wind is related to the divergence of the horizontal wind. (which requires an ageostrophic component to the wind)

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Vorticity and Divergence This flow field is purely vortical (zero divergence)

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Vorticity and Divergence This flow field is purely divergent (zero vorticity)

Vorticity and Divergence

We can think about this like angular momentum

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Question: What is the effect of divergence on vorticity?

A Spinning Skater

Axis of rotation is in the vertical plane

Motion is in the (x,y) plane

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

A Spinning Skater Motion is in the

(x,y) plane Question: A skater that is spinning with a given radius then brings in her arms. What happens to her angular velocity?

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

A Spinning Skater

Answer: Since her radius decreases, conservation of angular momentum says that her angular velocity must increase.

Motion is in the (x,y) plane

Recall: Angular momentum is a conserved quantity. Its magnitude is given by

|L| = rm!

Question: How is this like divergence?

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Vorticity and Divergence Question: What is the effect of divergence on vorticity?

Answer: A divergent flow must lead to a decrease in angular velocity. A convergent flow must lead to an increase in angular velocity.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

The Vorticity Equation Divergence term only

D

Dt(⇣ + f) = �(⇣ + f) (rh · u)

Absolute vorticity Horizontal divergence

Question: What happens to absolute vorticity when the flow is (a) Divergent? (b) Convergent?

(rh · u) > 0

(rh · u) < 0

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

What are these terms?

The Vorticity Equation

Rate of change of the absolute vorticity following the motion

D

Dt

(⇣ + f) = �(⇣ + f)(rh · u)�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� (r↵⇥rp) · k

Divergence term Tilting or twisting term Solenoidal term

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Tilting and Twisting

Relative velocity:

3D vorticity vector:

Relative vorticity:

u = (u, v, w)

r⇥ u =

✓@w

@y

� @v

@z

,

@u

@z

� @w

@x

,

@v

@x

� @u

@y

⇣ = k · (r⇥ u) =

✓@v

@x

� @u

@y

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Recall how relative vorticity is obtained:

Tilting and Twisting

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆Tilting or twisting term

Tilting represents the change in the vertical component of vorticity by tilting horizontal vorticity into the vertical.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

x

y

z

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆Tilting or twisting term

Consider a long, thin cylinder of fluid aligned with the y-axis.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

x

y

z

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆Tilting or twisting term

Consider a long, thin cylinder of fluid aligned with the y-axis.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

The flow satisfies v=0 and is sheared in the vertical so that the vorticity vector is along the y axis.

Initial axis of rotation

> 0= 0

x

y

z

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆Tilting or twisting term

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

The flow also satisfies dw/dy>0 leading to an upward tilting of the cylindrical tube

Consider a long, thin cylinder of fluid aligned with the y-axis.

The flow satisfies v=0 and is sheared in the vertical so that the vorticity vector is along the y axis.

> 0= 0 > 0

x

y

z

✓@w

@x

@v

@z

� @w

@y

@u

@z

Tilting or twisting term

> 0= 0 > 0

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Tilting and Twisting

Tilting and Twisting

Rotation in the (y,z) plane. Vorticity vector points along the x axis.

As the wheel is turned there is a component of vorticity in the z plane.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

What are these terms?

The Vorticity Equation

Rate of change of the absolute vorticity following the motion

D

Dt

(⇣ + f) = �(⇣ + f)(rh · u)�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� (r↵⇥rp) · k

Divergence term Tilting or twisting term Solenoidal term

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Solenoidal / Baroclinic Terms

� @

@x

✓1

@p

@y

◆+

@

@y

✓1

@p

@x

◆= �@↵

@x

@p

@y

+@↵

@y

@p

@x

The solenoidal / baroclinic terms capture changes in vorticity due to the alignment of surfaces of constant density and pressure.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Definition: In a barotropic fluid density depends only on pressure.

Definition: In a baroclinic fluid density depends on pressure and temperature.

By the ideal gas law, this implies that surfaces of constant density are surfaces of constant pressure are surfaces of constant temperature.

Solenoidal / Baroclinic Terms

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

p-Δp

p-2Δp

p

ρ-2Δρ

ρ-Δρ

ρ

Barotropic: surfaces of constant density parallel to surfaces of constant pressure

Solenoidal / Baroclinic Terms

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

x

r↵⇥rp = 0

A barotropic fluid does not induce changes in vorticity

y

ρ-2Δρ

ρ-Δρ

ρ

Baroclinic: surfaces of constant density intersect surfaces of constant pressure

p-Δp

p-2Δp

p

x

Solenoidal / Baroclinic Terms

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

r↵⇥rp 6= 0

A baroclinic fluid induces a change in vorticity.

y

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Solenoidal / Baroclinic Terms

In the real atmosphere, the solenoidal terms are a primary driver of the development of low-level low pressure systems in the middle latitudes.

This term is also important in understanding circulation around fronts.

ρ-2Δρ

ρ-Δρ

ρ

p-Δp

p-2Δp

p

Cold air sinking behind front

x

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Warm air rising ahead of front

z

Aside: Baroclinic Fronts Note that this case has to do with the development of horizontal vorticity (perpendicular to x-z plane)

What are these terms?

The Vorticity Equation

Rate of change of the absolute vorticity following the motion

D

Dt

(⇣ + f) = �(⇣ + f)(rh · u)�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� (r↵⇥rp) · k

Divergence term Tilting or twisting term Solenoidal term

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

D

Dt(� + f) =

⇥t(� + f) + u

⇥x(� + f) + v

⇥y(� + f) + w

⇥z(� + f)

Advection of Vorticity

@f

@t

= 0@f

@x

= 0@f

@z

= 0

Advection of relative vorticity

Advection of planetary vorticity

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

D

Dt(⇣ + f) =

@⇣

@t+ u ·r⇣ + v

@f

@y

@⇣

@t

+ u ·r⇣ + (⇣ + f)

✓@u

@x

+@v

@y

+

✓@w

@x

@v

@z

� @w

@y

@u

@z

◆+ v

@f

@y

= � @

@x

✓1

◆@p

@y

+@

@y

✓1

◆@p

@x

Advection Divergence

Tilting Baroclinicity

The Vorticity Equation

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Changes in absolute vorticity are caused by:

Changes in relative vorticity are caused by: –  Divergence –  Tilting –  Gradients in density –  Advection

The Vorticity Equation Scale Analysis

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

Question: Which of these terms are the most important for large-scale flows?

Scale Analysis Typical scales associated with large-scale mid-latitude storm systems:

U ⇡ 10 m s�1

W ⇡ 0.01 m s�1

L ⇡ 106 m

H ⇡ 104 m

L/U ⇡ 105 s

Paul Ullrich Analysis of the Dynamical Equations March 2014

a ⇡ 107 m

g ⇡ 10 m s�2

⌫ ⇡ 10�5 m2 s�1

(Radius of Earth)

(Gravity)

(Kinematic Viscosity)

�P ⇡ 10 hPa = 1000 Pa

⇢ ⇡ 1 kg m�3

�⇢/⇢ ⇡ 10�2

f0 ⇡ 10�4 s�1

� = @f/@y ⇡ 10�11 s�1

Scale Analysis

⇣ =@v

@x

� @u

@y

⇡ U

L

⇡ 10�5 s�1Relative Vorticity:

Planetary Vorticity: f0 ⇡ 10�4 s�1

f0⇡ 10�1

Definition: The Rossby number of a flow is a dimensionless quantity which represents the ratio of inertia to Coriolis force.

f0⇡ U

f0L⌘ Ro

In the mid-latitudes planetary vorticity is generally larger than relative vorticity.

Paul Ullrich Analysis of the Dynamical Equations March 2014

Scale Analysis Time rate of change and horizontal advection of relative vorticity:

@⇣

@t

, u

@⇣

@x

, v

@⇣

@y

⇡ U

2

L

2⇡ 10�10 s�2

w@⇣

@z⇡ WU

HL⇡ 10�11 s�2

Vertical advection of relative vorticity:

Paul Ullrich Analysis of the Dynamical Equations March 2014

Scale Analysis

(⇣ + f)

✓@u

@x

+@v

@y

◆⇡ f0(rh · u) ⇡ 10�10 s�2

✓@w

@x

@v

@z� @w

@y

@u

@z

◆⇡ WU

HL⇡ 10�11 s�2

v@f

@y⇡ U� ⇡ 10�10 s�2

k · (r↵⇥rp) ⇡ �⇢�p

⇢2L2⇡ 10�11 s�2

Divergence term:

Tilting term:

Planetary vorticity advection:

Solenoidal term:

Paul Ullrich Analysis of the Dynamical Equations March 2014

Remaining Terms Recall this is smaller than U/L

The Vorticity Equation

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

“Large” terms (10-10 s-2)

“Small” terms (10-11 s-2)

@⇣

@t

+ u

@⇣

@x

+ v

@⇣

@y

+ v

@f

@y

+ (⇣ + f)

✓@u

@x

+@v

@y

= �w

@⇣

@z

�✓@w

@x

@v

@z

� @w

@y

@u

@z

◆� @↵

@x

@p

@y

+@↵

@y

@p

@x

The Vorticity Equation Scale Analysis

Divergence  term  dominates  along  with  horizontal  advec2on  and  the  local  2me  rate  of  change  of  rela/ve  vor/city.

Til2ng  term  important  where  there  is  a  large  shear  and  strong  horizontal  gradient  in  the  ver/cal  velocity  (boundary  layer,  smaller  scales).

Solenoidal  term  important  where  there  are  strong  density  (temperature)  gradients  that  intersect  lines  of  constant  pressure  (sea  breeze,  fronts).

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

f0⇣

⇡ 10⇣

rh · u ⇡ 10f0

rh · u ⇡ 100

The Vorticity Equation Relative Vorticity, Planetary Vorticity and Divergence

The  rota/on  of  the  Earth  is  about  10  /mes  larger  than  rela/ve  vor/city  and  100  /mes  larger  than  divergence.

Paul Ullrich Introduction to Atmospheric Dynamics March 2014

@⇣

@t

+ u

@⇣

@x

+ v

@⇣

@y

+ v

@f

@y

+ (⇣ + f)

✓@u

@x

+@v

@y

◆= 0

Definition: The horizontal material derivative is defined by the equation

Dh

Dt

=@

@t

+ u

@

@x

+ v

@

@y

Dh

Dt

(⇣ + f) = �(⇣ + f)

✓@u

@x

+@v

@y

The Vorticity Equation Retaining leading order terms…

Paul Ullrich Introduction to Atmospheric Dynamics March 2014