forces Coriolis f. deviation to the RHS in q high - - PDF document

forces coriolis f deviation to the rhs in q high pressure
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forces Coriolis f. deviation to the RHS in q high - - PDF document

Applied Talks PhD @ HW Surface Semi Equations geo strophic - Lisei Stefania 02/05/18 of naturally Geophysical Fluid fluid dynamics Dynamics : flows Occur ing atmosphere such a as oceans , Dynamics dominated by : Rotation


slide-1
SLIDE 1

Applied

PhD

Talks

@ HW Surface Semi

  • geo strophic

Equations

Stefania Lisei

02/05/18

Geophysical

Fluid

Dynamics

:

fluid

dynamics

  • f naturally
Occur ing

flows

,

such

as
  • ceans
a

atmosphere

Dynamics

dominated

by

:

Pressure

gradient

Rotation

f. µ

Coriolis forces

⑤←

deviation

to q

the

RHS

in

/

high pressure

horizontal N

. atmosphere .

f=2R

sine

pressure

gradient

⇒ f-
  • along

equator

slide-2
SLIDE 2

Geographic

behave

:

Coriolis

force

deviates pressure

gradient

by

It

, so

dynamics

along

isobars

Limitation

:

friction

!

gn

Friction weakens

Coriolis force

high

pr%

before

cyclones

a

anticyclones

We need

a

model for atmosphere

&

  • ceans

with better

approximation

than

apostrophe balance

:
  • quasi
  • apostrophe

equations

(

QG )

: easier

but

less precise ,
  • semi
  • goo strophic

equations

I

SG ) : more

complex

I fully

nonlinear )

but better

approximation for

some

dynamics

I eg fronts

formation )

.
slide-3
SLIDE 3

Semi

  • goo strophic

equations

Iincompressible

, in viscid

)

:

I ft the

. D)

igtffuz

fu )at

to

=
  • ff
t =

fzp

I

= Ig t

Ia

ages strophic

full

wind

velocity

thestrophic

div

I

= wind

fig

=

f- dyp

, 2×10)

to

= pressure ,

f= buoyancy

anomaly

I ft the

. D) t =
  • f
=

Coriolis

frequency

, assumed

constant

Ig

is

the solution

in

the

genestrophic

balance

.

Important quantity

: Rossby

number Ro

.

Ro

measures

how

strong

the

effect

  • f

Earth

rotation

is

for

the

dynamics

.

Ro

= ¥

I

dimensionless )

.

Ro

=

corresponds

to

apostrophe

behave

I

no

friction I QG

a SQ have

physical meaning

when Ro

is small .
slide-4
SLIDE 4

Some references

:
  • Eliasson
' 48 :

into

SG .
  • Hoskins

A

Bretherton

' 72 : SG is

useful for

large-scale

dynamics

a

front genesis

  • Hoskins
' 75 :

intro

SSG

and

apostrophe

coordinates

.
  • Cullen

A

Purser

' 84 :

results

  • n

Lagrangian

space

.
  • Cullen
9

Shuts

I 87 : stability principle
  • Cullen
' 06 :

book

  • n

henge

scale

atmospheric

loonie flows

.
  • Benemou

A Brenier

' 98 :

week solutions

  • f
SG in

apostrophe

coordinates

through Optimal Transport

.
  • Ambrosio
, Colombo , De Philipp is , Figolli ' 12 , ' 16 : week

solutions

  • n

special

domains

.
  • Bad
in A Regine 46 : numeric
  • n
SSG .
slide-5
SLIDE 5

Surface

semi

  • Geestrophic

Equations

Hoskins

I

' 75 )

intro

word

tnensf

  • n
D= IR2 x

lol )

think

that

)

=

III.

3151

Use

X= IX. 42 )

for guest

coordinates

.

A

new

stream function

I

is

def

  • n
X sit .

DX

IH1H

=

Dap

IHIIXI

't )

new eg

for E.

Assuming

constant PV t

b.

as

ftttw

.

0/0=0

  • n

IR2

¥

THIN Issa Given f.

define

formally

TITI

=

4 if

4--5/2=1

and

DE

=

2xx$2yy§

  • l2xy$ )
'

am

slide-6
SLIDE 6

Need

to

define

rigorously

T

.

Thm I

L ,

Wilkinson

' 18 ) .

There

exists a constant

Go

st .

given

EC

"

CITY

smell ,

there

exists a

solution

EE0Y

  • f
IBVP ) .

Moreover

, § is

unique

  • n
a small ball .

Idea

  • f proof
: BFPT t

elliptic

theory

for the linear BVP

Thm

It

, Wilkinson ' 18) :

For

smell foe
  • d. TTY

It

>
  • sit
there exists a

unique

classical solution

to ISSG )
  • n

IT4

6II

Notes written on Good notes