Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

32
Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms

Transcript of Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Page 1: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms

Page 2: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Take away concepts and ideas

Why does the air cool as you climb a mountain?

Why are hurricanes so powerful ?

Heat convection vs. conduction

Atmospheric lapse rate

Pressure as a function of altitude

Convection in a dry vs. wet atmosphere

Atmospheric heat transport

Moist convection and CISK

Page 3: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

All “weather” takes place in the troposphere (<10 km)

Why does temperature decrease with altitude in the troposphere?

Why is it warm at the bottom of the troposphere?

Why does it rain?

How does rain affect the vertical temperature profile?

Page 4: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Very poor conductor

Very good convection

Important radiation properties

Atmosphere

Page 5: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Convection..

• Why does water in a kettle heat up to boil?• Why is air on the ceiling warmer than the floor?• Why does smoke rise?• Why does lava ooze out of cracks on the ocean

floor?• How do clouds form?

Page 6: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

“State” Properties of Air

The interdependence of air temperature, pressure, and density

Page 7: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Why does temperature decrease with height in the troposphere ?

1) Solar (radiative) heating at Earth surface2) Atmospheric convection (hydrostatic balance)

Page 8: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Temperature and Pressure profiles of the atmosphere

Page 9: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Thermodynamic properties of Dry Air

Assume (for now) the atmosphere has no water.

Dry air pressure (P), Temperature, and Density all linked through

Ideal Gas Law

Hydrostatic balance

Page 10: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

A. “Ideal Gas Law” P V = n R T

“Ideal Gas Law” = “Equation of State”(just “perfect” gas with no other phases, like water)

n / V = density =

so can rewrite as: P = R T

Pressure

VolumeNumberof molecules

Constant

Temperature

Page 11: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

R = constantPressure (P, force exerted by gas molecular motion)Temperature (T, energy of molecular motion)Density ( number of atoms per unit volume, n/V)

P = R Tor

P V = n R T

Page 12: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Rigid walls

Flexible walls

= constant

P = constant

Page 13: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

constant P = ∆ R ∆T

Link

Cooling a balloon in liquid nitrogen (-∆T) increases the density (+∆)

Page 14: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

B. Hydrostatic equation

The atmosphere under gravity - hydrostatic balance

Gravity “pushes down”

… the atmosphere “pushes back”

When equal, this is Hydrostatic balance equation

ΔP = - ρ g Δz

where g = grav. accel. (9.8 m/s2)

Page 15: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

The decrease of pressure with height

ΔP = - ρ g Δz

or

ΔP / Δz = - ρ g

Page 16: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Impress your friends!

You can calculate lapse rate knowing planet’s gravity!

Easy as 1…2…3:

1) 1st Law of Thermodynamics∆Heating = ∆internal energy + ∆work∆Q = ∆U + ∆W (conservation of energy, signs are right here)

No heating for an adiabatic process, therefore:

0 = ∆U + ∆W

Page 17: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

2) 0 = ∆U + ∆W0 = (change in temperature * air heat capacity) + (pressure * change in volume)

0 = n cv ∆T + P ∆V

Combining, 0 = Cp ∆T + ∆P/ρ (Cp is heat cap of air)

Rearranging, ∆T/∆P = -1 / ( Cp ρ)

Now, substitute into hydrostatic equation (∆P = - g ∆z)

You’ve derived the Dry Adiabatic Lapse Rate equation

Rearrange…

∆T/∆z = g / Cp

∆T/∆z = (9.8 m/s2) / (1004 J/kg/K)

= 9.8 K per km <-- Dry Lapse Rate !!

Page 18: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Atmospheric temperature profile:

Surface warmingBy conduction

Adiabatic = No heat is lost or gained within a parcel of airDiabatic = Heat is lost or gained within a parcel of air

Heat transfer byDRY convection= 9.8°C / km

Page 19: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Now just add water…

Wet Convection

So far we’ve just considered a “dry atmosphere”

Dry adiabatic lapse rate: -9.8 °C/km

typical adiabatic lapse rate: - 6 °C/km

why aren’t they the same?

Water vapor!

Page 20: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Dry Air and Dry Convection

Think of a “parcel” of air…

If the air is heated, how does its density change?

P = ∆ R ∆T

Is the parcel stable or unstable relative to adjacent parcels?

… dry air convection!

(no clouds just yet…)

7°C/km 9.8°C/km

Page 21: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Thermodynamic properties of moist air

The atmosphere in most places isn’t dry.

Energetics of water phase changes:

Liquid --> Vapor requires 540 cal/gram H2O

(Latent heat of evaporation; takes heat AWAY)

Vapor --> Liquid releases 540 cal/gram H2O

(Latent heat of condensation; ADDS heat)

Page 22: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Phase changes of water

Direction of phase change Thermodynamic effect

going to lower energy phase (vapor->liquid->ice)

Examples: rain, ice-formation

heat is released (warms air)

going to higher energy phase (ice->liquid->vapor)

Examples: Ice-melting, evaporation

heat is absorbed (cools air)

Page 23: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Temperature Controls Water Vapor Saturation in Air

Warm air holds A LOT more water than cold air.

What is saturation?

Saturation water vapor

content increases

exponentially with temperature

Clausius-Clapeyron relation -->

Page 24: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Consider a rising parcel of air, but this time it has water vapor (typically 0.5% by weight)…

1. Air parcel rises… starts to cool2. Follows DRY ADIABATIC lapse rate until 1st

condensation (cloud)3. 1st condensation --> release of latent heat of

condensation inside of parcel4. Warming in parcel offsets cooling, so5. Rising parcel no longer follows dry adiabatic lapse rate

of -9.8°C/km, but follows the MOIST ADIABATIC lapse rate of -6-7 °C/km

Tropical atmosphere follows MOIST adiabatPolar atmosphere follows DRY adiabat

Page 25: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Moisture affects stability

DRY PARCEL rising in warm environmentMOIST PARCEL rising in warm environment

-9.8 °C/km-7 °C/km-6.5 °C/km-7 °C/km

unstable stable

Page 26: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Comparing the dry and moist lapse rates

Page 27: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

California Coastal Range

Coast Desert

Page 28: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Moist adiabatic lapse rate = 7°C/km

Dry adiabatic lapse rate = 9.8°C/kmup

down

Page 29: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

unstable

Page 30: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Why Hurricanes are so powerful

CISK = Convective Instability of the Second Kind

Page 31: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.

Galveston, TX: Hurricane of 1900

Page 32: Thermal Structure of the Atmosphere: Lapse Rate, Convection, Clouds, Storms.