• Aucun résultat trouvé

J ( J ) « Gain » of Balance and Critical Level Absorption for Inertio Gravity Waves

N/A
N/A
Protected

Academic year: 2022

Partager "J ( J ) « Gain » of Balance and Critical Level Absorption for Inertio Gravity Waves"

Copied!
25
0
0

Texte intégral

(1)

« Gain » of Balance and Critical Level Absorption for Inertio Gravity Waves

F. Lott

LMD/CNRS, Ecole Normale Supérieure , Paris

C. Millet

Laboratoire de détection et de Géophysique, CEA-DAM Ile de France, Arpajon

J. Vanneste

Maxwell Institute, University of Edimburg

I Motivation: Emission of GWs from balanced flows

II Object : R and T of an IGWs propagating through critical levels III Interpretation: for large Richardson number

( J )

IV Triggering of very large disturbances via the valve effect at small

J

(2)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

(3)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(4)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

E

E

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(5)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

E

E

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(6)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

E

E

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(7)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

A re-examination of the inertial levels in vertically sheared rotating stratified flows

I Motivation: Emission of GWs from balanced flows

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(8)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

A re-examination of the inertial levels in vertically sheared rotating stratified flows

I Motivation: Emission of GWs from balanced flows

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(9)

Lott, Plougonven and Vanneste, JAS 2010 and 2013.

Orr mechanism' in rotating vertically stratified and shear flow : SET Up : a 3D (x,y,z) PV anomaly is advected, Coriolis f =cte,

BV freq N=cte, wind vertical shear =cte).

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(10)

A re-examination of the inertial levels in vertically sheared rotating stratified flows

I Motivation: Emission of GWs from balanced flows

Question : Does the presence of the ground affect the results in terms of GWs emission, triggering of Sub-Synoptic instabilities?

Near the PV anomaly, can trigger non-geostrophic modes of baroclinic instabilities (next time!)

E

Ground

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(11)

A re-examination of the inertial levels in vertically sheared rotating stratified flows

I Motivation: Emission of GWs from balanced flows

Question : Does the presence of the ground affect the results in terms of GWs emission, or triggering of Sub-Synoptic instabilities?

E

Ground E

TE

RE

Ect if R ≠0

Far from the PV anomaly, one needs to analyse the

Transmission (T) and Reflection ( R ) of the gravity waves Emitted (E).

Gain of balance and critical level absorption for inertio gravity waves

I Motivation: Emission of GWs from balanced flows

(12)

No rotation f=0 cases with constant wind shear and constant buoyancy frequency N. Stable case: J=N2/2>0.25

Taylor Goldstein Eq. In Hydrostatic + Boussinesq:

d2W

dz2 J12

z2 W=0

w ' (x , y , z , t)=W (z)ei(kx+ly)

A doppler shift can always place the critical level in z=0:

where =l/k

Gain of balance and critical level absorption for inertio gravity waves

II Object: R & T of an IGWs propagating through critical levels

(13)

No rotation f=0 cases with constant wind shear and constant buoyancy frequency N. Stable case: J=N2/2>0.25

Taylor Goldstein Eq. In Hydrostatic + Boussinesq:

d2W

dz2 J12

z2 W=0

w ' (x , y , z , t)=W (z)ei(kx+ly)

A doppler shift can always place the critical level in z=0:

where =l/k

Upward propagating wave above:

Wz=z1/2i where =

J 12−0.25

Analytic continuation below z=0:

Wz=−i∣z1/2i e 

R = 0, T = e

− 

Exponential factor

z=zei

A re-examination of the inertial levels in vertically sheared rotating stratified flows

II Object: R & T of an IGWs propagating through critical levels

This is an upward wave, there is no reflected wave:

Gain of balance and critical level absorption for inertio gravity waves

II Object: R & T of an IGWs propagating through critical levels

(14)

Case with rotation and f=cte (Jones 1967, Yamanaka et Tanaka 1984, YT84)

1−2 2

dd2W2

232i

2

W

J12 22i3

W=0

Where=k z f

Three critical levels, in

The critical level =0 is regular.

The two inertial levels (ILs) in are irregular

(intrinsic phase speed kΛz equal (+-) f )

=− 1, 0,1

=±1

The 0-PV condition for a monochromatic disturbance gives

A re-examination of the inertial levels in vertically sheared rotating stratified flows

II Object: R & T of an IGWs propagating through critical levels

Gain of balance and critical level absorption for inertio gravity waves

II Object: R & T of an IGWs propagating through critical levels

(15)

The exact solution

W

involves Hypergeometric functions (F1, F2, F3...)

>>1: 1/2+i(upward GW)

Connection in =-1 Connection in =1

C 1

>1: F1(1--2)

1: A F2(2)+B F3(2))

1: CF4(1--2) +D F5(1--2)

A re-examination of the inertial levels in vertically sheared rotating stratified flows

II Object: R & T of an IGWs propagating through critical levels

Gain of balance and critical level absorption for inertio gravity waves

II Object: R & T of an IGWs propagating through critical levels

: C|1/2-i+D|1/2+i

(Downward GW+Upward GW) Two (often) non-propagating

solutions

(16)

The exact solution

W

involves Hypergeometric functions (F1, F2, F3...)

>>1: 1/2+i(upward GW)

: C|1/2-i+D|1/2+i

(Downward GW+Upward GW)

>1: F1(1--2)

1: A F2(2)+B F3(2))

1: CF4(1--2) +D F5(1--2)

'=  A' ' B e− 

'= A ' ' B

A− ' ' B= ' ' ' C' D e 

A−' ' B=' ' ' C' D

Connection in =-1 Connection in =1

The valve effect is an amplification of the incoming wave for =l/k>0

It is attenuated back at the higher inertial level

A re-examination of the inertial levels in vertically sheared rotating stratified flows

II Object: R & T of an IGWs propagating through critical levels

Gain of balance and critical level absorption for inertio gravity waves

II Object: R & T of an IGWs propagating through critical levels

Extremely involved

R C

0, T 1

=e

− 

(17)

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

Mathematical explanation for R and T insensitive to rotation

1−2 2

dd2W2

232i

2

W

J12 22i3

W=0

The 0-PV equation Becomes

for large

d2W

d2 J12

2 W=0

The Taylor Goldstein Eq.

As between the path near along the real axis and a path at

large distance from the critical levels there is no singularities

the solutions in the far field are the same (Jones 1967)

But how can we explain that variations in e (so dependent of the orientation and independent of J) becomes attenuations in e (strongly

ν

(18)

WKB expansion for large W =

W01W1...

e

=± 1

1−2 , W0=−1

1 4i

21

1 4−i

2 , W1=...

=

J 12

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

(19)

WKB expansion for large W =

W01W1...

e

=± 1

1−2 , W0=−1

1 4i

21

1 4−i

2, W1=...

WIII=iW0 e−  eilog2−1

W II=1i

2 W0 e  e−asin

W I=W 0 eilog∣∣2−1

=

J 12

ie− 1/2i

~

1/2i

~

Upward GW

≈∞

−1e− 

≈0

~

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

(20)

WKB expansion for large W =

W01W1...

e

=± 1

1−2 , W0=−1

1 4i

21

1 4−i

2, W1=...

WIII=i W0 e− eilog2−1

WII=1i

2 W0 e /2 e−

asin 2

WI=W0 eilog∣∣2−1

Valve effect

decaying solution

~Quasi Geostrophic solution

=

J 12

ie− 1/2i

~

1/2i

~

Upward GW

≈∞

≈−∞

−1e− 

≈0

~

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

(21)

WKB expansion for large W =

W01W1...

e

=± 1

1−2 , W0=−1

1 4i

21

1 4−i

2, W1=...

WIII=i W0 e− eilog2−1

WII=1i

2 W0 e /2 e−

asin 2

WI=W eilog∣∣2−1

Valve effect

decaying solution

~Quasi Geostrophic solution

=

J 12

The value of the evanescent solution in =+1 is T,the transmission coefficient

ie− 1/2i

~

Upward GW

1/2i

~

Upward GW

≈∞

−1e− 

≈0

~

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

(22)

Verification: Exact versus WKB solution, J=5, =0.1

Real (solid) and Imag (dashed) of W

ξ

2 0 -2 -4 -6 -8 -10

0 -0.2 -0.4 -0.6 -0.8 -1

ξ

Zoom

Lower Inertial level

Decaying solution Propagating

solution

Gain of balance and critical level absorption for inertio gravity waves

III Interpretation: for large Richardson number (J)

(23)

Gain of balance and critical level absorption for inertio gravity waves

IV Triggereing of very large disturbances via the valve effect when (J<1)

When J<1, The decay of the solution can largely be dominanted by the valve effect when ν>>1:

The solutions between the inertial layers become very large

The two solutions between the inertial layers have now comparable amplitudes and can sustained substantial EP fluxes (non-propagating solutions need to be in

pair to sustain momentum fluxes)

e−  e1−J

20

10

0

-10

-20

ξ ξ

Exact solution and EP-flux

J=0.5, =2

Zoom

Negative EP flux Very large positive EP flux due to the

interaction

between two solutions Very small negative EP flux due to the transmitted wave

1.5

0

-1.5

(24)

Gain of balance and critical level absorption for inertio gravity waves

IV Triggereing of very large disturbances via the valve effect when (J<1)

When J<1,Very large EP flux between the inertial layers

This will tend to restore the mean wind shear to returns to J>1 conditions (e.g. inertially stable conditions).

EP flux=100 J=1 Flux = 1

ming)

ν =l/k

Log 10 of EP-Flux between the ILs

ν=0

(25)

Gain of Balance and Critical Level Absorption For Inertio Gravity Waves

Exact results for all J : R and T as in the non-rotating case Inertially stable case (J>1), interpretation of R & T:

The incoming gravity wave becomes evanescent (« gain of balance »)  at the lowest inertial level, the disturbance amplitude at the upper inertial level is then

exponentially small, and this represents the absorptive property of the shear layer.

This is somehow reminiscent of a tunelling effect, but no reflections are needed at the turning altitudes, because the presence of critical levels allows jumps in

EP fluxes.

Inertially unstable case ((J<1) and valve effect:

the valve effect can yield very large disturbances between the inertial levels.

There, the disturbance is made of two solutions that interact and

Références

Documents relatifs

Although small near surface incident winds naturally occur in fronts via combination of the thermal wind balance and of the boundary layer, they pose at least two problems in

At local level, the increase in time spent working in the agricultural sector when farmers fear crime-related violence seems to be balanced out by an increase in the workers’

B: Straight-line interfaces that exhibit several vertical o ffsets (roughness zero for an individual sub-interface). C: Smooth interface that accounts for data uncertainty and

Second, excepted the first generations of fluorescent agonist and antagonist peptides useful for fluorescence microscopy techniques applied to the investigation of receptor

- Adjusted to UPDRSIII-score PD patients had different levels of striatal denervation - We showed that the COMT-genotype impacts on clinical severity of motor symptoms - We

This is remedied to some extent by the addition of the Tycho Catalogue (named in honour of Tycho Brahe’s sig- nificant contributions to astrometry) wherein phase space data

We have implemented a treatment of the UV radiative transfer including the atomic hydrogen lines Lyα, Lyβ, and the two- photon continuum in order to solve for self-irradiated

interval, i.e., the galaxy stellar mass function (GSMF), is often used to study the evolution of the total stellar mass in the universe. The low-mass ends of the GSMFs are