lecture10_stability

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Lecture 10
Static Stability
General Concept
An equilibrium state can be stable or
unstable
Stable equilibrium: A displacement induces a
restoring force

i.e., system tends to move back to its original
state
Unstable equilibrium: A displacement induces
a force that tends to drive the system even
further away from its original state
A More Realistic Scenario
Equilibrium
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Small Displacement
Stable.
Large Displacement
Large Displacement
Large Displacement
Large Displacement
Large Displacement
Large Displacement
Unstable.
Idea of Previous Slides
There may be a critical displacement
magnitude
displacement < critical  stable
displacement > critical unstable
(More about this shortly)
Atmospheric Stability
Unsaturated Air
Consider a vertical parcel displacement, z

Assume displacement is (dry) adiabatic
Change in parcel temperature = -d z
Denote lapse rate of environment by 
T=T0 - dz
T = T0 - z
Temp of displaced parcel
 temp of environment
z
T = T0
Parcel
T = T0
Environment
Two Cases
Parcel temp. > environment temp.
 parcel less dense than environment
 parcel is buoyant
Parcel temp. < environment temp.
 parcel denser than environment
 parcel is negatively buoyant
Lapse Rates
Tparcel = T0 - dz
Tenv = T0 - z
Tparcel > Tenv if T0 - dz > T0 - z
  > d
Tparcel < Tenv if T0 - dz < T0 - z
  < d
Stability
 > d  resultant force is positive
 parcel acceleration is upward (away from
original position)
 equilibrium is unstable
 < d  resultant force is negative
 parcel acceleration is downward (toward
original position)
 equilibrium is stable
Graphical Depiction
Temp of rising parcel
z
Stable lapse rate
Unstable lapse
rate
Temperature
Saturated Air
Recall: Vertically displaced parcel
cools/warms at smaller rate

Call this the moist-adiabatic rate, m
Previous analysis same with d replaced
by m


Equilibrium stable if  < m
Equilibrium unstable if  > m
General Result
Suppose we don’t know whether a layer of
the atmosphere is saturated or not
 > d   > m  equilibrium is unstable,
regardless

Equilibrium is absolutely unstable
 < m   < d  equilibrium is stable,
regardless

Equilibrium is absolutely stable
Continued
Suppose m <  < d
Layer is stable if unsaturated, but unstable
if saturated
Equilibrium is conditionally unstable
Absolutely
stable
Conditionally
unstable
m
Absolutely
unstable
d

Application
If a layer is unstable and clouds form, they
will likely be cumuliform
If a layer is stable and clouds form, they
will likely be stratiform
Example: Mid-Level Clouds
Suppose that clouds form in the middle
troposphere
Unstable  altocumulus
Stable  altostratus
Altocumulus
Altostratus
Deep Convection
Previous discussion not sufficient to
explain thunderstorm development
Thunderstorms start in lower atmosphere,
but extend high into the troposphere
Physics Review: Energy
Object at height h
h
Physics Review: Energy
Remove support: Object
falls
h
Physics Review: Energy
Let z(t) = height a time t
z(t)
It Can Be Shown …
1
2
m v  mgz  mgh
2
kinetic energy
potential energy
(v = speed)
As object falls, potential energy is
converted to kinetic energy.
Available Potential Energy
Object may have potential energy, but it
may not be dynamically possible to
release it
Technically, PE = mgh,
but lower energy state
is inaccessible.
The energy is
unavailable.
h
Energy Barriers
To get from a to b, energy must be
supplied to surmount the barrier.
Energy needed: mghb
hb
a
h
b
Energy Barriers
Now, ball can roll down hill.
a
h
b
Energy Barriers
Amount of PE converted to KE: mg(h + hb)
Net release of energy: mg(h + hb) – mghb = mgh
hb
a
h
b
CAPE, CIN
CAPE: Convective Available Potential
Energy

(Positive area)
CIN: Convective Inhibition

(Negative area at bottom of sounding)
Sounding
Dry adiabat
Saturated adiabat
Positive area
Negative area
LCL
CAPE, CIN
CIN is the energy barrier
CAPE is the energy that is potentially
available if the energy barrier can be
surmounted
Isolated Severe Thunderstorms
Suppose CIN and CAPE are large
Consider a population of incipient
thunderstorms
Few of these storms will surmount the
energy barrier, however …
Those that do will have a lot of energy
available.
Sudden Outbreaks of Severe
Weather
Start with a high energy barrier
(large CIN)
Sudden Outbreaks of Severe
Weather
Now, suppose energy barrier
decreases.
Sudden Outbreaks of Severe
Weather
Disturbances that previously couldn’t
overcome the barrier now can.
If CAPE is large, storms
could be severe.
Level of Free Convection (LFC)
Level of Free Convection (LFC):
When a parcel ceases to be colder and denser than
surrounding air (environment), and instead becomes
positively buoyant.
On a thermo diagram, this occurs when the moist adiabat
being followed by the parcel crosses from the cold side of
the environmental profile to the warm side.
The level at which this crossover occurs is the LFC.
Equilibrium Level (EL)
Thermals will continue to rise until their temperature
matches that of the environment. The level at which this
occurs is called the equilibrium level (EL).
Also called level of neutral buoyancy. At that point, parcels
may overshoot a little, becoming colder than environment
and ultimately falling back to their EL.
Convective Inhibition (CIN)
CIN 
Z LFC
f
B
( z )dz
fB = Buoyancy force
0
 T ( z )  T ( z ) 
f B ( z)  
g

 T ( z ) 
T(z) temp of rising parcel, T’(z) temp of environment at same level.
CIN   g
z LFC

0
 T ( z )  T ( z ) 
 T ( z )  dz


Buoyant force is negative by definition, minus sign in front of integral.
Convective Inhibition (CIN)
Invoking hydrostatic approximation, and ideal gas law:
LFC
CIN  Rd


T
(
p
)

T
( p)d ln p

P0
CAPE
LFC
CIN  Rd
 T ( p)  T ( p)d ln
p
[J /kg]
P0
Once the parcel has overcome the energy barrier, CIN, and reached its
LFC, CAPE is the energy that may be released by resulting buoyant
ascent.
EL
CAPE  Rd


T
(
p
)

T
( p)d ln p

[J /kg]
LFC
CIN represents the energy barrier to initiation of free convection.
CAPE is the maximum possible energy that can be released after CIN
has been overcome.
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