atmospheric waves chapter 6 - university of california,...
TRANSCRIPT
![Page 2: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/2.jpg)
Part 3: Internal Gravity Waves
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Internal Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
(Internal) gravity waves are generated by flow over topography, thunderstorms, other mesoscale systems
(Internal) gravity wave effects are: cloud streets, lenticularis clouds, rapid local temperature and pressure changes, clear air turbulence
They carry energy and momentum into the middle atmosphere (stratosphere, mesosphere)
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Atmospheric gravity waves can only exist when the atmosphere is stably stratified (N2 > 0)
Buoyancy force is the restoring force for gravity waves
In an incompressible fluid (e.g. ocean) gravity waves travel primarily in the horizontal plane, since reflection at lower and upper boundary occurs for vertically traveling waves.
In the atmosphere: Due to compressibility and stratification, gravity waves may propagate vertically and horizontally.
Internal Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
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Figure: Air moving over a mountain on an island triggers waves on the downwind (lee) side of the mountain, indicated by the cloud pattern
Topographic Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
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Undular Bore
Examples
Paul Ullrich Atmospheric Waves March 2014
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Mountain-generated waves (lee waves)
Examples
Paul Ullrich Atmospheric Waves March 2014
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Consider pure internal gravity waves: No rotation, no friction
Can be studied with the basic equations for 2D (x-z plane) motions with Boussinesq approximation (almost incompressible)
Internal Gravity Waves
@u
@t
+ u
@u
@x
+ w
@u
@z
+1
⇢
@p
@x
= 0
@w
@t
+ u
@w
@x
+ w
@w
@z
+1
⇢
@p
@z
+ g = 0
@u
@x
+@w
@z
= 0
@✓
@t
+ u
@✓
@x
+ w
@✓
@z
= 0
Paul Ullrich Atmospheric Waves March 2014
Four equations in five unknowns
![Page 9: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/9.jpg)
Take logarithms of both sides:
✓ = T
✓p0p
◆Rdcp
=p
⇢Rd
✓p0p
◆Rdcp
= Rdpcvcp ⇢�1p
Rdcp
0
ln ✓ =
cvcp
ln p� ln ⇢+ constant
Internal Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
Equations must be closed via an equation of state, such as the potential temperature equation:
![Page 10: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/10.jpg)
Linearize the basic equations by letting
⇢ = ⇢0 + ⇢0
p = p(z) + p0
✓ = ✓(z) + ✓0
u = u+ u0
w = w0
dp
dz= �g⇢0 ln ✓ =
cvcp
ln p� ln ⇢0 + constant
IGWs: Derivation (1)
Paul Ullrich Atmospheric Waves March 2014
Hydrostatic Balance
The basic state must satisfy:
Definition of Potential Temperature
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@u
@t
+ u
@u
@x
+ w
@u
@z
=@
@t
(u+ u
0) + (u+ u
0)@
@x
(u+ u
0) + w
0 @
@z
(u+ u
0),
=@u
0
@t
+ u
@u
0
@x
+ u
0 @u0
@x
+ w
0 @u0
@z
,
=@u
0
@t
+ u
@u
0
@x
Linearize the material derivative terms:
IGWs: Derivation (2)
Paul Ullrich Atmospheric Waves March 2014
Constant Constant Constant
Small Small
@w
@t
+ u
@w
@x
+ w
@w
@z
=@w
0
@t
+ (u+ u
0)@w
0
@x
+ w
0 @w0
@z
,
=@w
0
@t
+ u
@w
0
@x
Small Small
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@✓
@t
+ u
@✓
@x
+ w
@✓
@z
=@
@t
(✓ + ✓
0) + (u+ u
0)@
@x
(✓ + ✓
0) + w
0 @
@z
(✓ + ✓
0),
=@✓
0
@t
+ u
@✓
0
@x
+ u
0 @✓0
@x
+ w
0 @✓
@z
+ w
0 @✓0
@z
,
=@✓
0
@t
+ u
@✓
0
@x
+ w
0 @✓
@z
Linearize the thermodynamic equation:
IGWs: Derivation (2)
Paul Ullrich Atmospheric Waves March 2014
No ,me dependence
Small
No x dependence
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Linearize Remember some calculus: Linearization yields
1
⇢
@p
@z+ g =
1
⇢0 + ⇢0
✓@p
@z+
@p0
@z
◆+ g
1
⇢0 + ⇢0=
1
⇢0
1⇣1 + ⇢0
⇢0
⌘ ⇡ 1
⇢0
✓1� ⇢0
⇢0
◆⇢0
⇢0⌧ 1
IGWs: Derivation (3)
For
Paul Ullrich Atmospheric Waves March 2014
1
⇢
@p
@z+ g ⇡ 1
⇢0
@p
@z
✓1� ⇢0
⇢0
◆+
1
⇢0
@p0
@z+ g =
1
⇢0
@p0
@z+
⇢0
⇢0g
Use 1
⇢0
@p
@z= �g
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Potential temperature equation:
with
ln
✓
✓1 +
✓0
✓
◆�=
1
�ln
p
✓1 +
p0
p
◆�� ln
⇢0
✓1 +
⇢0
⇢0
◆�+ constant
� =cpcv
IGWs: Derivation (3)
ln ✓ =
cvcp
ln p� ln ⇢+ constant
Linearize via
Paul Ullrich Atmospheric Waves March 2014
✓ = ✓ + ✓0, p = p+ p0, ⇢ = ⇢0 + ⇢0
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Again, remember some calculus: Apply these rules to potential temperature equation:
To obtain linearized potential temperature equation:
ln(ab) = ln a+ ln b
ln(1 + ✏) ⇡ ✏ ✏ ⌧ 1
ln
✓
✓1 +
✓0
✓
◆�=
1
�ln
p
✓1 +
p0
p
◆�� ln
⇢0
✓1 +
⇢0
⇢0
◆�+ constant
✓0
✓⇡ 1
�
p0
p� ⇢0
⇢0⇢0 ⇡ �⇢0
✓0
✓+
p0
c2s c2s =p�
⇢0
IGWs: Derivation (3)
Speed of sound
Paul Ullrich Atmospheric Waves March 2014
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In gravity waves, density fluctuations due to pressure changes are small compared to those due to temperature changes: Therefore, to a first approximation, the potential temperature equation becomes:
����⇢0✓0
✓
���� �����p0
c2s
����
✓0
✓⇡ � ⇢0
⇢0
IGWs: Derivation (3)
Paul Ullrich Atmospheric Waves March 2014
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The linearized equation set for internal gravity waves becomes
✓@
@t
+ u
@
@x
◆u
0 +1
⇢0
@p
0
@x
= 0 (1)
✓@
@t
+ u
@
@x
◆w
0 +1
⇢0
@p
0
@z
� ✓
0
✓
g = 0 (2)
@u
0
@x
+@w
0
@z
= 0 (3)✓
@
@t
+ u
@
@x
◆✓
0 + w
0 @✓
@z
= 0 (4)
IGWs: Derivation (4)
Paul Ullrich Atmospheric Waves March 2014
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Leads to Now eliminate u’ from (5) by computing Leads to the equation:
✓@
@t
+ u
@
@x
◆✓@w
0
@x
� @u
0
@z
◆� g
✓
@✓
0
@x
= 0 (5)
@(5)
@x
+
✓@
@t
+ u
@
@x
◆@(3)
@z
✓@
@t
+ u
@
@x
◆✓@
2w
0
@x
2+
@
2w
0
@z
2
◆� g
✓
@
2✓
0
@x
2= 0 (6)
IGWs: Derivation (5) @(2)
@x
� @(1)
@z
Eliminate p’ by computing
Paul Ullrich Atmospheric Waves March 2014
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Yields single equation for
✓@
@t
+ u
@
@x
◆2 ✓@
2w
0
@x
2+
@
2w
0
@z
2
◆+
g
✓
@✓
@z
@
2w
0
@x
2= 0
✓@
@t
+ u
@
@x
◆(6) +
g
✓
@
2(4)
@x
2
Eliminate θ’ from (6) by computing
IGWs: Derivation (5)
Square of Brunt-Väisälä frequency: assume to be constant N 2
Paul Ullrich Atmospheric Waves March 2014
w0
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Consider wave-like solutions:
w = wr + iwi m = mr + imi � = kx+mz � ⌫t
✓@
@t
+ u
@
@x
◆2 ✓@
2w
0
@x
2+
@
2w
0
@z
2
◆+N 2 @
2w
0
@x
2= 0
IGWs: Derivation (6)
Paul Ullrich Atmospheric Waves March 2014
w
0= Re [w exp(i�)]
= Re [(wr + iwi) exp(i(kx+mrz � ⌫t)) exp(�miz)]
= [wr cos(Re(�))� wi sin(Re(�))] exp(�miz)
Horizontal wavenumber k is real, solution is always sinusoidal
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The vertical wavenumber m is complex – Real part mr describes the sinusoidal variation in z – Imaginary part mi describes the exponential decay or
growth of the wave amplitude in z, depending on the sign of mi (positive / negative).
If m is real, total wave number may be regarded as a vector directed perpendicular to line of constant phase, and in the direction of phase increase.
k =2⇡
Lx
m =2⇡
Lz = ki+mk
IGWs: Wavenumbers m = mr + imi
w0= [wr cos(Re(�))� wi sin(Re(�))] exp(�miz)
with
Paul Ullrich Atmospheric Waves March 2014
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IGW Frequency
Relative to the mean wind: – Positive (+) sign means eastward phase propagation – Negative (-) sign means westward phase propagation
(⌫ � uk)2(k2 +m2)�N 2k2 = 0
⌫ = uk ± Nkpk2 +m2
= uk ± Nk
IGWs: Dispersion w0
= Re [w exp(i�)]✓
@
@t
+ u
@
@x
◆2 ✓@
2w
0
@x
2+
@
2w
0
@z
2
◆+N 2 @
2w
0
@x
2= 0
Insert
into
IGW Dispersion Relation
Paul Ullrich Atmospheric Waves March 2014
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If we let k > 0 and m < 0, then lines of constant phase φ = (kx + mz) tilt eastward with increasing height
The choice of the positive root then corresponds to an eastward and downward phase propagation (relative to the mean flow).
The zonal and vertical phase speeds (positive root) are
+
⌫ = uk ± Nkpk2 +m2
= uk ± Nk
cx
=⌫
k= u+
Npk2 +m2
cz
=⌫
m=
uk
m+
Nk
mpk2 +m2
IGWs: Frequency
Paul Ullrich Atmospheric Waves March 2014
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Solutions for the other perturbation fields u’, p’, θ’ can be obtained by substituting w’ back into original linearized equations (let k > 0 and m < 0)
@u
0
@x
= �@w
0
@z
=) u
0 = �m
k
w
0
✓@
@t
+ u
@
@x
◆u
0 = � 1
⇢0
@p
0
@x
=) p
0 = ⇢0(⌫ � ku)
k
u
0
✓@
@t
+ u
@
@x
◆✓
0 = �w
0 @✓
@z
=) ✓
0 =i
(ku� ⌫)
@✓
@z
w
0
IGWs: Phase Relationships
Observe u’, w’, p’ are exactly in phase, with
However θ’ (or T’) out of phase by 1/4 wavelength: Warm air leads pressure ridge eastward
Transverse wave:
⌫ � ku > 0
k · u ⌘ ku0 +mw0 = w0hk⇣�m
k
⌘+m
i= 0
Perpendicular!
Paul Ullrich Atmospheric Waves March 2014
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If we let k > 0 and m < 0, then lines of constant phase φ = (kx + mz) tilt eastward with increasing height
Horizontal distance
Height
Phase velocity
Perturbation velocity field
W C
W
C
W C Temperature perturbation
H H L
H L Pressure perturbation
IGWs: Cross Section
⌫ � ku > 0Assume
L
Phase lines
Paul Ullrich Atmospheric Waves March 2014
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The zonal and vertical phase velocities are
Upper and lower signs chosen as above.
IGWs: Phase / Group Velocity
The components of the group velocity are
cx
=⌫
k= u± Np
k2 +m2
cz
=⌫
m=
uk
m± Nk
mpk2 +m2
Paul Ullrich Atmospheric Waves March 2014
cg,x
=@⌫
@k= u± Nm2
(k2 +m2)3/2
cg,z
=@⌫
@m= ⌥ Nkm
(k2 +m2)3/2
![Page 27: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/27.jpg)
The vertical component of group velocity has a sign opposite to that of the vertical phase speed.
That is, downward phase propagation implies upward energy propagation
IGWs: Phase / Group Velocity
cx
=⌫
k= u± Np
k2 +m2
cz
=⌫
m=
uk
m± Nk
mpk2 +m2
Paul Ullrich Atmospheric Waves March 2014
cg,x
=@⌫
@k= u± Nm2
(k2 +m2)3/2
cg,z
=@⌫
@m= ⌥ Nkm
(k2 +m2)3/2
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Horizontal phase and group velocities point in the same direction (no sign change)
Remarkable property of internal gravity waves: Group velocity travels perpendicular to the direction of the phase propagation
That is, in internal gravity waves energy travels parallel to the crests and throughs (in contrast to shallow water gravity waves)
IGWs: Phase / Group Velocity
Paul Ullrich Atmospheric Waves March 2014
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Height Phase velocity
Phase lines (only the crests are shown here)
Group velocity (energy travels in this direction)
α
Angle of phase lines to the local vertical:
α
IGWs: Phase / Group Velocity
Lx
LLz
Lx
cos↵ = ± L
Lx
= ± Lzp
L2x
+ L2z
= ±�2⇡m
�q�
2⇡k
�2+
�2⇡m
�2 = ± kpk2 +m2
= ±k
Paul Ullrich Atmospheric Waves March 2014
pL2x
+ L2z
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Consequence: gravity wave intrinsic frequency (relative to mean flow) must be less than buoyancy frequency
cos↵ = ± L
Lx
= ± Lzp
L2x
+ L2z
= ±�2⇡m
�q�
2⇡k
�2+
�2⇡m
�2 = ± kpk2 +m2
= ±k
⌫ = ⌫ � uk = ± Nkpk2 +m2
= ±Nk
⌫ ⌘ ⌫ � uk = ±N cos↵
IGWs: Frequency Angle of phase lines to the local vertical:
Frequency of internal gravity waves:
Intrinsic Frequency
Paul Ullrich Atmospheric Waves March 2014
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Propagation of an internal gravity wave packet
https://www.youtube.com/watch?v=cDsNmnpq9_o
http://www.youtube.com/watch?v=RpP62QSJM0g
Observed waves in the atmosphere
IGWs: Movies
Paul Ullrich Atmospheric Waves March 2014
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For example, idealized mountain height profile:
⌫ = �uk < 0
Topographic Gravity Waves Topographic gravity waves are stationary internal waves driven by topography (a lower boundary condition on w).
For stationary waves (ν=0) this means that the intrinsic frequency is (westward relative to the mean flow)
Wavelength k is determined by the wavelength of the topography (flow follows topography near the ground)
h(x) = hM cos(kx)
Paul Ullrich Atmospheric Waves March 2014
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For stationary waves, the dispersion relationship for IGWs ✓
@
@t
+ u
@
@x
◆2 ✓@
2w
0
@x
2+
@
2w
0
@z
2
◆+N 2 @
2w
0
@x
2= 0
✓@
2w
0
@x
2+
@
2w
0
@z
2
◆+
N 2
u
2 w
0 = 0
Topographic Gravity Waves Topographic gravity waves are stationary internal waves driven by topography (a lower boundary condition on w).
simplifies to
Paul Ullrich Atmospheric Waves March 2014
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Seek stationary ( ) wave solutions: yields the dispersion relationship
If , m2 > 0 (m must be real). Solutions have the form of vertically propagating waves (with constant amplitude):
⌫ = 0, ⌫ = uk
w0= Re [w exp(i�)] = wr cos�� wi sin�
w = wr + iwi, m = mr + imi, � = kx+mz
m2 =N 2
u2 � k2
|u| < N/k
w
0= w exp(i(kx+mz))
Topographic Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
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Wide (broad) mountain small k m real Ridges and trough lines slope with height, opposite to u Upward flow of energy and momentum
Intrinsic phase speed vector
Wave number vector (k,m)
Intrinsic group velocity vector
Absolute group velocity vector u
u
Paul Ullrich Atmospheric Waves March 2014
Vertically Propagating Waves
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If , m2 < 0 (m is purely imaginary). Solutions have the form of vertically trapped waves (that decay with height):
m2 =N 2
u2 � k2
Topographic Gravity Waves
Paul Ullrich Atmospheric Waves March 2014
|u| > N/k
w
0= w exp(ikx) exp(�miz)
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decay
Vertically Trapped Waves
Paul Ullrich Atmospheric Waves March 2014
Narrow mountain large k m imaginary Ridges and trough lines aligned with height No tilt, no momentum transport
w
0= w exp(ikx) exp(�miz)
![Page 38: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/38.jpg)
Paul Ullrich Atmospheric Waves March 2014
Topographic Gravity Waves
Ver$cal propaga$on of gravity waves is only possible when is less than the buoyancy frequency Stable stra,fica,on, wide ridges and rela,vely weak zonal flow provide favorable condi,ons for ver,cally propaga,ng gravity waves. If energy is transported upward, phase must be downward.
|uk| N
Summary
![Page 39: Atmospheric Waves Chapter 6 - University of California, Davisclimate.ucdavis.edu/ATM121/AtmosphericDynamics... · cv cp ⇢1p Rd cp 0 ln = c v c p ln p ln ⇢ +constant Internal Gravity](https://reader034.vdocument.in/reader034/viewer/2022042922/5f6df5dfc664604b897e0bc9/html5/thumbnails/39.jpg)
Figure: Circulation is more complex in real gravity waves: For example, rotors, breaking waves, wind shear, varying
More Realistic IGWs
N
Paul Ullrich Atmospheric Waves March 2014
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Figure: Lenticularis cloud forming on the lee side of the mountain
Lenticularis Cloud
Movie: https://www.youtube.com/watch?v=YKAfKHSeWZc
Paul Ullrich Atmospheric Waves March 2014