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9.1 The Atmosphere and Atmospheric ChemistryThe atmosphere consists of the following on a dry basis: • 78.1% N2 • 21.0% O2 • 0.9% Ar • 0.04% CO2 • Low levels of noble gas helium, neon, k

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2010

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9.1 The Atmosphere and Atmospheric Chemistry

The atmosphere consists of the following (on a dry basis):

• 78.1% N2 • 21.0% O2 • 0.9% Ar • 0.04% CO2

• Low levels of noble gas helium, neon, krypton, xenon

• Trace gases (see Table 9.1)

Most of the mass of the atmosphere is very close to Earth’s surface relative to Earth’s diameter

• If Earth were a classroom globe, virtually all air would

be in a layer the thickness of the coat of varnish on the

globe!

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Photochemistry and Some Important Terms

Photochemical reactions occur in the atmosphere when molecules absorb energy in the form of photons

• Mostly in ultraviolet region of spectrum • E = hν

A chemical species in an excited (energized) state is

designated with an asterisk, *

The photochemical reaction of stratospheric ozone:

• O3+ hν(λ< 420nm) O*+ O2

•The O3 absorbs a photon of energy hν

• The O3 undergoes photodissociation

• The oxygen atom product is excited denoted O*

Free radicals with unpaired electrons shown with a dot, •

•H2O2+ hν→ HO • + HO •

Energy-absorbing third body , M, usually N2 molecule

•O + O2 + M O3+ M

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Gaseous Oxides in the Atmosphere

Low and variable levels of C, N, and S oxides

• Pollutants at elevated levels

• Discussed in Chapters 11 and 14

Atmospheric methane

• From anoxic bacteria and underground sources

• Significant greenhouse gas

• Influences levels of hydroxyl radical (HO • ), ozone,

stratospheric water vapor

Hydrocarbons and photochemical smog

• Hydrocarbons required for photochemical smog

formation (see Chapters 13 and 14)

Particulate matter (see Chapter 10)

Primary pollutants emitted directly

Secondary pollutants formed from reactions of primary pollutants

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Part of hydrologic cycle

Source of CO2 for plant photosynthesis

Source of N for plant growth, industrial chemicals

Variation of pressure and density with altitude

• Pressure and density decrease rapidly with increasing altitude

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Figure 9.1 Variation of air pressure and temperature with altitude

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Stratification of the Atmosphere

• Lower atmosphere, the troposphere

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Stratosphere and Upper Atmosphere

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9.4 Energy Transfer in the Atmosphere

Solar Flux

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Earth’s Atmospheric Heat Balance

See detail of Earth’s atmospheric

heat balance in text Figure 9.4

Re-absorption of outbound

infrared stabilizes atmospheric

temperature

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9.5 Atmospheric Mass Transfer, Meteorology,

Weather

Meteorology is the science of physical atmospheric

phenomena

Weather: Short-term variations in

• Temperature • Clouds • Winds • Humidity • Pressure

• Horizontal visibility • Precipitation type and quantity

Climate: Long-term weather conditions

Atmospheric Water in Energy and Mass Transfer

• Carries energy as latent heat released when water vapor condenses

Humidity is water content of air

• Relative humidity is % saturation level

Water condenses below dew point

• Condensation nuclei

Clouds are composed of microdroplets of water

• Coalesce to form larger droplets and precipitation

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Distinct air masses in the atmosphere

• Uniform temperature and water vapor content

• Horizontally homogeneous

• Conditions and movement affect pollutant reactions, effects, and dispersal

• Air masses separated by fronts

• Warm fronts • Cold fronts

• Wind is horizontally moving air

• Air currents are vertically moving air

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Figure 9.5 Circulation of air masses and water, uptake

and release of solar energy as latent heat in water vapor

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Global Weather

Figure 9.6 Global circulation of air in the northern hemisphere

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9.6 Inversions and Air Pollution 15

Figure 9.7 Pollutants trapped by a temperature

inversion and confining topography

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9.7 Global Climate and Microclimate

Climate

• Characteristic of a particular region

• Varies with season

Example: Alternating monsoons and dry seasons

• Ice age manifested by long-term change in climate

Humans may be modifying climate largely by pumping

carbon dioxide into the atmosphere causing warming

Microclimate

• Highly localized climate

Example: At soil surface shaded by plants

Effects of urbanization on microclimate

• Heat dome over cities

• City atmosphere up to 5˚C warmer

• Counteracting cooling effect from particulate matter

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9.8 Chemical and Photochemical Reactions

Study of atmospheric chemistry is complicated

• Effects of photochemical energy input

• Extreme dilution of species in air

• Container walls complicate laboratory study

Major categories of atmospheric chemical species

• Inorganic oxides (CO, CO2, NO2, SO2)

• Oxidants (O3, H2O2, HO • ,HO2 • , and ROO • radicals, NO3)

• Reductants (CO, SO2, H2S)

• Organics (such as CH4, most also reductants)

• Oxidized organics (carbonyls, organic nitrates)

• Photochemically active species (NO, formaldehyde)

• Acids (H2SO4), bases (NH3), salts (NH4HSO4)

• Unstable reactive species (NO2*, HO • )

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Fig 9.8 Atmospheric chemical and photochemical processes

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Photochemical Processes

Initiated when a molecule absorbs a photon of

electromagnetic radiation to produce an excited species, *

• NO2+ hν→ NO2*

• Usually in ultraviolet region

Loss of excess energy from an excited state may occur by several processes including

• Dissociation: NO2*NO+ O

• Luminescence: NO2* NO2 + hν

•Photoionization: N2*N2++ e

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Ions in the Atmosphere

Ionosphere above about 50 km

• From photoionization by solar ultraviolet

• Raises at night as ions recombine

Figure 9.9 Van

Allen belts of ions

encircling Earth (in

cross section)

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Free Radicals

Reactive species with unpaired electrons denoted •

Generally formed by photochemical reactions or reactions

of molecules with other free radicals

Two free radicals may react to form a stable species

Hydroxyl radical in the atmosphere

• HO • is the most important free radical in the atmosphere (see text Figure 9.10)

• Produced by many reactions such as

CH4 + O (from photodissociation of NO2) H3C • +HO •

• Removed by many reactions, especially with CO or CH4 Hydroperoxyl radical in the atmosphere

• HOO •

• Less important than HO • , but still significant

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Evolution of the Atmosphere

Atmospheric oxygen from photosynthesis

• CO2+ H2O+ hν→ {CH2O} + O2

•Evidence from iron oxide deposits

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9.9 Acid-Base Reactions in the Atmosphere

Rainwater weakly acidic from CO2

• CO2+ H2O H+ + HCO3

-Pollutant SO2 is more acidic than CO2

Strong acid H2SO4, HNO3, and HCl are responsible for

damaging acid rain

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9.10 Reactions of Atmospheric Oxygen, Figure 9.11

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Reactions of Atmospheric Nitrogen

N2 molecule is very stable

• No significant tropospheric chemical or photochemical reactions of N2

• N2 is the most common energy-absorbing third body, “M”,

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9.12 Atmospheric Water

Normal range 1-3% by volume

Vapor responsible for atmospheric temperature stability

Hydrologic cycle

Crucial in atmospheric energy transfer

Tropopause prevents water vapor transfer from

troposphere to stratosphere

Stratospheric water from following several-step process:

• CH4+ 2O2+ hν→ CO2+ 2H2O

Stratospheric water produces hydroxyl radical

•H2O+ hν→ HO • + H

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9.13 Influence of the Anthrosphere

Many air pollutants from the anthrosphere

• Particles affecting visibility

• Acid-forming gases such as SO2

•Nitrogen oxides and hydrocarbons forming photochemical smog

Two major kinds of species affecting global climate

• Chlorofluorocarbons that deplete stratospheric ozone

• Greenhouse gases that cause global warming

• Primarily CO2

• Other gases such as CH4

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9.14 Chemical Fate and Transport in Atmosphere

Considers the following regarding airborne pollutants

• Sources • Transport • Dispersal • Fluxes

Atmosphere/surface boundary interaction

• Rock/soil • Water • Vegetation

Transport and dispersal

• Movement of air masses • Diffusive and Fickian transport Long-range movement such as radionuclides from

Chernobyl reactor meltdown

Distillation of semivolatile organic pollutants to polar

regions

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Fig 9.12 Localized atmospheric chemical fate and transport from a point source

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