Importance of stratospheric ozone

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The Importance of Ozone

The chemistry of the stratosphere is dominated by the chemistry of ozone.  Ozone is of importance because it absorbs damaging solar ultraviolet radiation in the 220 – 290 nm range (although the absorption tails off to wavelengths longer than 300 nm).  Nothing else present in the atmosphere absorbs in this region, and ozone, as we shall see has a somewhat tenuous existence.  We can see how well it protects the Earth's surface by considering absorption at 250 nm, the position of the ozone maximum.  Using the Beer-Lambert Law,

ln(I0/I) = σcl,

with σ ≈ 10-17 cm2 molecule-1, c ≈ 2.5 × 1019 molecule cm-3, and l ≈ 0.3 cm,

log(I/Isurface) = 10-17×0.3×2.5×1019/2.303 = 32.6

i.e., less than one part in 1032 of the radiation at λ = 250 nm reaches the Earth's surface.  Life on the surface of the planet could not survive without the protection of the ozone layer.  (See Wayne, pp. 665 − 673 for a description of the evolution of this aspect of the Earth's atmosphere.)


Oxygen-only Chemistry

Stratospheric ozone is generated from the photolysis of O2 in an oxygen-only scheme known as the Chapman Scheme

 O2        +        hν        →        O        +        O                (3.1)

        O2        +        O        +        M        →        O3        +        M                (3.2)

        O        +        O3        →        O2        +        O2                (3.3)

        O3        +        hν        →        O        +        O2                (3.4)

        [O        +        O        +        M        →        O2        +        M                (3.5)]

almost all conditions (it has a half-life of about 100 s even at 90 km).  At high altitudes, there is little O2 (pressure falls exponentially with altitude), while at low altitudes, there is plenty of oxygen, but radiation of the required energy has been absorbed.  The consequence is that it is only at intermediate altitudes that ozone is created in significant concentrations.  Hence the Ozone Layer.

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Atmospheric Photolysis

Determining the rate at which a molecule is photolysed requires a knowledge of the wavelength dependence of the photolysing radiation, and a quantitative knowledge of the spectroscopy and photochemistry of the molecule of interest.  The intensity of radiation is known as the Actinic Flux (I(z, λ)), and is wavelength and altitude dependent, as illustrated

The actinic flux is determined by the solar spectrum and the amount of radiation that has been absorbed by O2 (primarily below 200 nm) and O3 (between 220 and 290 nm).  The spectrum of the molecule is described by the (wavelength-dependent) Absorption ...

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