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Stratospheric Chemistry The Ozone Layer

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Filters harmful UV rays before they reach us ... This causes the Photolysis. O2 UV( 241nm) ... Results of O2 Photolysis. In and Above Stratosphere ... – PowerPoint PPT presentation

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Title: Stratospheric Chemistry The Ozone Layer


1
Stratospheric Chemistry The Ozone Layer
  • Chapter 2, Baird

2
Introduction The Ozone Layer
  • Earths natural sunscreen
  • Filters harmful UV rays before they reach us
  • Appearance of a large hole over Antarctica in
    mid-1980s
  • www.

3
Ozone, O3
  • Gas present in small conc throughout atmosphere
  • Total overhead amount expressed in terms of
    Dobson Units
  • 1DU 0.01 mm thickness of O3 when brought to
    ground level(1 atm) at 0oC
  • Normal amount is 350 DU at temperate latitudes
    (Thus, only a 3.5 mm thick )
  • RQ 2,3 AP 1 (Let Vol 1.8x1015L)

4
Ozone, O3
  • O3 conc varies seasonally.
  • Highest levels in early spring.
  • Lowest levels in the fall.

5
Ozone Hole
  • Began to notice in the late 70s over Antarctica.
    By 1980s there was a 50 drop from normal
    values.
  • See Fig 2-2

6
Minimum Concentration of Total Overhead O3 above
Antarctica in Sept-Oct of Recent Years-Fig 2-2
7
Variation with Year of the Size of the Ozone
Hole-Now about the Size of North America
8
Total Overhead O3 for NonPolar Regions(60oN-60oS)
Showing Some WorldWide Depletion
9
Chapter 2 Topics Emphasized
  • The Production of the Ozone Layer
  • How is it created and sustained?
  • Ozone Depletion
  • By what mechanism is it being depleted?

10
Regions of the Atmosphere
  • Earths atmosphere has evolved with time.
  • (Early atmosphere high conc of CO2)
  • Major change caused by photosynthesis
  • 6CO2 6H2O ? C6H12O6 6O2

11
Atmospheric Composition
  • Present Composition
    N2 78
  • O2 21
  • Ar 1
  • CO2 0.04
  • H2O variable

12
Atmospheric Layering
  • Thermosphere (above 90 km)
  • 90 km------------------Mesopause
  • Mesosphere(50 90 km)
  • 50 km-------------------Stratopause
  • Stratosphere(15 50 km)
  • 15 km-------------------Tropopause
  • Troposphere (See Fig 2-5)

13
Atmospheric Layering
  • Slope of curve of temp vs altitude is lapse
    rate
  • See Fig 2-5
  • RQ 4

14
Atmospheric Layering PicturedConceptsLapse
Rate, Temp. Inv.RQ 5
15
Atmospheric Temperature Inversion
  • This is a change from a neg. to a pos. lapse
    rate. The point at which the lapse rate changes
    marks a stable boundary between two physically
    distinct layers of air.
  • Warm air over Cooler air.

16
Atmospheric Temperatures Governing Factors
  • Absorption of Solar Energy
  • Peak intensity in Visible Region
  • Heat Production inside Earth
  • Radioactive decay
  • Energy Emission from Earth
  • Blackbody radiation in IR Region

17
Environmental Concentration
Units for Gases
  • Usually Pollutant gases have their conc.
    Expressed as either ppm or ppb.
  • Assuming PVnRT, Pressure, Volume, and Mole
    Fractions are all the same. Thus,
  • ppm is also ppmv.

18
Chemistry of the Ozone Layer
  • Light Absorption by Molecules
  • Principles of Photochemistry

19
The Electromagnetic Spectrum
  • With Ranges of Environmental Interest (RQ5)

20
Absorption Spectrum of O2
  • Far UVphotons of the sun are absorbed by O2
  • This causes the Photolysis
  • O2 UV(?lt241nm)?2O
  • Do a Calculation to prove this, if OO Energy is
    495 kJ/mol
  • RQ7,8,9 2-1,2-2,2-3

21
Results of O2 PhotolysisIn and Above
Stratosphere
  • This filters all of the UV light from 120-240
    nm. This also filters some, but not all UV in the
    220-240 nm range
  • No UV with ?lt220 nm reaches Earths
    surface(Protects life from UV damage)
  • Now O3 can form.

22
The Creation and Noncatalytic Destruction of Ozone
  • In the Stratosphere, conc of O2 molecules is
    relatively large and conc of atomic O is
    relatively small.
  • Thus, O3 can form via
  • O O2 M ? O3 M 105 kJ
  • Above reaction heats Stratosphere
  • What role does M play?

23
The Creation and Noncatalytic Destruction of Ozone
  • Ozone does efficiently absorb UV light with
    ?lt320. (See Fig 2-8 next slide)
  • It then dissociates
  • O3 UV(?lt320nm)?O2 O
  • The reaction O3 O?2O2 does occur somewhat but
    is slowed by a high activation energy.

24
Absorption Spectrum of O3
25
Solar UV Intensity Outside Atmosphere and at
Earths Surface
26
Creation and Noncatalytic Destruction of O3 The
Chapman Cycle
27
Chapman Cycle Condensed
  • O
  • ________________________
  • ? UV-C O2
    ?
  • O2 --------------?O-----------?O3
  • ???
    _________??
  • UV-B
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