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Chapter 1: Measures of atmospheric composition

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Let’s look at the Sun through the atmosphere…

Radiation intensity

wavelength λ

visible:

0.4-0.7 μm

UV

IR

incident radiation

air molecule

~0.3 nm

absorption

transmission

scatter

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Scattering of solar radiation�by air molecules

The atmosphere seen from the space station

Visible solar radiation

wavelength λ = 0.4 µm

0.5

0.6

0.7

  • Size of air molecules ~ 0.3 nm << λ
    • more scattering in blue (small λ)

Sun is yellow

Sky is blue

Sunset is red

scatter

scatter

cloudy sunset

Sun seen from space station

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Aerosols and clouds: the visible part of the atmosphere

Pollution off U.S. east coast

Dust off West Africa

California fire plumes

Aerosols are suspended solid or liquid particles, typically 0.1-1 µm in size

Cloud droplets (1-100 μm in size) form by condensation on particles when relative humidity exceeds 100%

They scatter or absorb visible radiation efficiently

Visible radiation is nearly 100% scattered

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Atmospheric gases are “visible” too… if you look in UV or IR

Visible

0.4-0.7 µm

Nitrogen dioxide (NO2 ) observed by satellite in the UV

Fraction of solar radiation

absorbed by

atmospheric

gases

Ultraviolet (UV)

Infrared (IR)

Nitrogen dioxide (NO2) observed from satellite

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Measure of relative concentration: mole fraction (mixing ratio) CX [mol mol-1]

remains constant when air density changes

stable measure of atmospheric composition

SPECIES

Mole fraction

(dry air)

[mol mol-1]

Nitrogen (N2)

0.78

Oxygen (O2)

0.21

Argon (Ar)

0.0093

Carbon dioxide (CO2)

420x10-6

Neon (Ne)

18x10-6

Ozone (O3)

(0.01-10)x10-6

Helium (He)

5.2x10-6

Methane (CH4)

1.9x10-6

Krypton (Kr)

1.1x10-6

Trace

gases

Air also contains variable H2O vapor (10-6-10-2 mol mol-1),

aerosol particles, and many trace gases at < 1x10-6 mol mol-1

Trace gas concentration units:

1 ppm = 1 µmol mol-1 = 1x10-6 mol mol-1

1 ppb = 1 nmol mol-1 = 1x10-9 mol mol-1

1 ppt = 1 pmol mol-1 = 1x10-12 mol mol-1

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Atmospheric concentrations of greenhouse gases

Concentration units: parts per million (ppm) and parts per billion (ppb)

Stable gases like CO2 and methane are generally reported as mole fractions

https://gml.noaa.gov/

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Measure of absolute concentration [X]: mass or moles per unit volume of air

Proper measure for absorption of radiation by atmosphere

Proper measure of concentration for

  • reaction rates
  • optical properties of atmosphere

nX and CX are related by the ideal gas law:

(obeyed within 1% at atmospheric pressure)

  • Mass concentration (g cm-3):

na = air number density

A = Avogadro’s number

p = pressure

R = Gas constant

T = temperature

MX= molar mass of X [g mol-1]

  • Number density nX [molecules cm-3]

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Gas-phase reaction rates depend on number densities

A

B

AB*

C

D

reactants

products

activated

complex

rate constant

product of number densities,

proportional to collision frequency

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Aerosol concentrations are often expressed as mass per unit volume,�typically in units of [μg m-3]

Surface PM2.5 fine particulate matter < 2.5 μm diameter

EPA air quality standard: 9 μg m-3 (annual mean)

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Daily PM2.5 concentrations

Surface PM2.5 fine particulate matter < 2.5 μm diameter

EPA air quality daily standard: 35 μg m-3

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Extinction of radiation depends on column concentration

Radiation flux at top of atmosphere

surface

absorption at altitude z

is proportional to nXdz

dz

Total atmospheric extinction is proportional to column concentration (often just called column):

unit area

Extinction = absorption + scatter

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Monitoring the ozone column from satellite

Method: UV solar backscatter

Reflection by

Earth surface

λ1

λ2

Ozone layer

Ozone

absorption

spectrum

λ1

λ2

Thickness of ozone layer is measured

as a column concentration

http://ozonewatch.gsfc.nasa.gov/

Sun

0

50

100

150

Ozone column, 1017 molecules cm-2

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Absolute concentration of gas can also be measured as partial pressure px [Pa]

The partial pressure pX of a gas X in a mixture is the pressure that the gas would exert if all other gases in the mixture were removed.

Proper measure for phase change

(such as condensation of water vapor)

T2 > T1

pH2O = pH2O,SAT(T2)

> pH2O,SAT(T1)

T1

pH2O = pH2O,SAT(T1)

head space

liquid water

Thought experiment: consider a pan of water with a lid:

Now heat the pan:

Dalton’s law

saturation vapor pressure

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Phase rule: defines the conditions for different phases �to be present at equilibrium in a multicomponent mixture

n = c + 2 - p

  • c = number of components
  • p = number of phases at equilibrium
  • n = number of degrees of freedom (independent variables) determining this equilibrium

Derivation: see chapter 1 of Introduction to Atmospheric Chemistry (2nd edition)

Example: consider the equilibrium of water between gas and liquid phases.

There are two variables determining the system: pH2O and T

For the gas and liquid phases to be at equilibrium we have

c = 1, p =2 n = 1 only one degree of freedom which can be either pH2O or T

(but not both)

This is expressed by pH2O,SAT = f(T)

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Clausius-Clapeyron equation: pH2O, SAT = f(T)

A = 6.11 hPa

B = - 5310 K

To = 273 K

pH2O,SAT (hPa)

T (K)

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Phase diagram for water

o

triple

point (n = 0)

gas-liquid

metastable

equilibrium

Clausius-Clapeyron curve

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Even at temperatures < 0 oC, water droplets may not freeze…�because creating an ice surface requires energy (surface tension)

Thought experiment: imagine an ice embryo forming in a cloud droplet

Ice molecules at the surface are not happy because they are not bound to their ice neighbors – producing these surfaces requires energy

Because of this, cloud droplets can remain supercooled liquid in metastable equilibrium down to temperatures as low as -40 oC

When supercooled cloud droplets hit surfaces, you get instant freezing because the freezing surface is provided: this produces rime ice

truck on Mt. Washington

Frosted trees near the top of Cannon Mt.

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Working with the phase diagram:

Dew point: Temperature Td such that pH2O = pH2O,SAT(Td)

o

Initial state (pH2O, T)

cooling

cloud

pH2O,SAT

Td

Relative humidity (%) = 100(pH2O/pH2O,SAT)

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RUNAWAY GREENHOUSE EFFECT ON VENUS

EARTH

VENUS

due to accumulation of water vapor (a powerful greenhouse gas)

from volcanic outgassing early in its history

…did not happen on Earth because farther from Sun; as water accumulated it reached saturation and precipitated, forming the oceans

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Solutes decrease the saturation water vapor pressure

water saturation vapor pressure

over pure liquid water surface

water saturation vapor pressure

over aqueous solution of water

mole fraction xH2O

An atmosphere of relative humidity RH can contain at equilibrium aqueous solution particles of water mole fraction

solute

molecules

in green

Raoult’s law

Aerosol particles therefore contain water even at RH < 100%, and that water content increases as RH increases so that particles increase in size

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Visibility is limited by light scattering by aerosol particles and air molecules

object

Background light

At high RH, aerosol particles grow by uptake of water, decreasing visibility (haze)

scatter

scatter

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Haze is a euphemism for air pollution

“winter haze” in Beijing

December 1952 London fog episode (The Crown, season 2)