Photochemical air pollution consists of a complex mixture of gaseous pollutants and aerosols, some of which are photochemically produced. Among the gaseous compounds are the oxidizing species ozone, nitrogen dioxide, and peroxyacyl nitrate:
The member of this series most commonly found in the atmosphere is peroxyacetyl nitrate (PAN):
Photochemical smog is composed of mixtures of particulate matter and noxious gases, similar to those that occurred in the typical London-type “pea soup” smog. The London smog was a mixture of particulates and oxides of sulfur, chiefly sulfur dioxide. But the overall system in the London smog was chemically reducing in nature. This difference in redox chemistry between photochemical oxidant and
SO
x-particulate smog is important in several respects. Note in particular the problem of quantitatively detecting oxidant in the presence of sulfur dioxide. Because it is a reducing agent, SO
x tends to reduce the oxidizing effects of ozone and thus produces low quantities of the oxidant.
8.2.2. The Effect of NOx
It has been well established that if a laboratory chamber containing NO, a trace of NO2, and air is irradiated with ultraviolet light, the following reactions occur:
NO2+hv(3000A∘≤λ≤4200A∘)→NO+O(P3)
(8.1)
O+O2+M→O3+M
(8.2)
O3+NO→O2+NO2
(8.3)
The net effect of irradiation on this inorganic system is to establish the dynamic equilibrium
NO2+O2↔hvNO+O3
(8.4)
However, if a hydrocarbon, particularly an olefin or an alkylated benzene, is added to the chamber, the equilibrium represented by reaction
(8.4) is unbalanced and the following events take place:
1. The hydrocarbons are oxidized and disappear.
2. Reaction products such as aldehydes, nitrates, PAN, etc., are formed.
3. NO is converted to NO2.
4. When all the NO is consumed, O3 begins to appear. On the other hand, PAN and other aldehydes are formed from the beginning.
Basic rate information permits one to examine these phenomena in detail. Leighton
[2], in his excellent book
Photochemistry of Air Pollution, gives numerous tables of rates and products of photochemical nitrogen oxide–hydrocarbon reactions in air; this early work is followed here to give fundamental insight into the photochemical smog problem. The data in these tables show low rates of photochemical consumption of the saturated hydrocarbons, compared with the unsaturates, and the absence of aldehydes in the products of the saturated hydrocarbon reactions. These data conform to the relatively low rate of reaction of the saturated hydrocarbons with oxygen atoms and their inertness with respect to ozone.
Among the major products in the olefin reactions are aldehydes and ketones. Such results correspond to the splitting of the double bond and the addition of an oxygen atom to one end of the olefin.
Irradiation of mixtures of an olefin with nitric oxide and nitrogen dioxide in air shows that the nitrogen dioxide rises in concentration before it is eventually consumed by reaction. Since the photodissociation of the nitrogen dioxide initiates the reaction, it would appear that a negative quantum yield results. More likely, the nitrogen dioxide is being formed by secondary reactions more rapidly than it is being photodissociated.
The important point is that this negative quantum yield is realized only when an olefin (hydrocarbon) is present. Thus, adding the overall step
OO3}+olefin→products
(8.5)
to reactions
(8.1)–
(8.3) would not be an adequate representation of the atmosphere photochemical reactions. However, if one assumes that O
3 attains a steady-state concentration in the atmosphere, one can perform a steady-state analysis (see
Chapter 2, Section
2.4) with respect to O
3. Furthermore, if one assumes that O
3 is largely destroyed by reaction
(8.3), one obtains a useful approximate relationship:
(O3)=−(j1/k3)(NO2)/(NO)
where
j is the rate constant for the photochemical reaction. Thus, the O
3 steady-state concentration in a polluted atmosphere is seen to increase with decreasing concentration of nitric oxide, and vice versa. The ratio of
j1/
k3 approximately equals 1.2 ppm for the Los Angeles noonday condition
[2]. Reactions such as
O+NO2+M→NO3+M
do not play a part. They are generally too slow to be important.
Furthermore, it has been noted that when the rate of the oxygen atom–olefin reaction and the rate of the ozone–olefin reaction are totaled, they do not give the complete hydrocarbon consumption. This anomaly is also an indication of an additional process.
An induction period with respect to olefin consumption is also observed in the photochemical laboratory experiments, thus indicating the buildup of an intermediate. When illumination is terminated in these experiments, the excess rate over the total of the O and O3 reactions disappears. These and other results suggest that the intermediate formed is photolyzed and contributes to the concentration of the major species of concern.
Possible intermediates that fulfill the requirements of the laboratory experiments are alkyl and acyl nitrites and pernitrites. The second photolysis effect eliminates the possibility that aldehydes serve as the intermediate.
Various mechanisms have been proposed to explain these laboratory results. The following low-temperature (atmospheric) sequence based on isobutene as the initial fuel was first proposed by Leighton
[2] and appears to account for most of what has been observed:
O+C4H8→CH3+C3H5O
(8.6)
CH3+O2→CH3OO
(8.7)
CH3OO+O2→CH3O+O3
(8.8)
O3+NO→NO2+O2
(8.9)
CH3O+NO→CH3ONO
(8.10)
CH3ONO+hv→CH3O∗+NO
(8.11)
CH3O∗+O2→H2CO+HOO
(8.12)
HOO+C4H8→H2CO+(CH3)2CO+H
(8.13)
H+O2+M→HOO+M
(8.14)
HOO+NO→OH+NO2
(8.15)
OH+C4H8→(CH3)2CO+CH3
(8.16)
CH3+O2→CH3OO(as above)
(8.17)
2HOO→H2O2+O2
(8.18)
2OH→H2+O2
(8.19)
HOO+H2→H2O+OH
(8.20)
HOO+H2→H2O2+H
(8.21)
There are two chain-propagating sequences (reactions
(8.13) and
(8.14) and reactions
(8.15)–
(8.17)) and one chain-breaking sequence (reactions
(8.18) and
(8.19)). The intermediate is the nitrite, as shown in reaction
(8.10). Reaction
(8.11) is the required additional photochemical step. For every NO
2 used to create the O atom of reaction
(8.6), one is formed by reaction
(8.9). However, reactions
(8.10),
(8.11), and
(8.15) reveal that for every two NO molecules consumed, one NO and one NO
2 form—hence, the negative quantum yield of NO
2.
With other olefins, other appropriate reactions may be substituted. Ethylene would give
O+C2H4→CH3+HCO
(8.22)
HOO+C2H4→2H2CO+H
(8.23)
OH+C2H4→H2CO+CH3
(8.24)
Propylene would add
OH+C3H6→CH3CHO+CH3
(8.25)
Thus, PAN would form from
CH3CHO+O2→hvCH3CO+HOO
(8.26)
CH3CO+O2→CH3(CO)OO
(8.27)
CH3(CO)OO+NO2→CH3(CO)OONO2
(8.28)
and an acid could form from the overall reaction
CH3(CO)OO+2CH3CHO→CH3(CO)OH+2CH3CO+OH
(8.29)
Because pollutant concentrations are generally in the parts-per-million range, it is not difficult to postulate many types of reactions and possible products.
8.2.3. The Effect of SOx
Historically, the sulfur oxides have long been known to have a deleterious effect on the atmosphere, and sulfuric acid mist and other sulfate particulate matter are well established as important sources of atmospheric contamination. However, the atmospheric chemistry is probably not as well understood as the gas-phase photoxidation reactions of the nitrogen oxides
−hydrocarbon system. The pollutants form originally from the SO
2 emitted to the air. Just as mobile and stationary combustion sources emit some small quantities of NO
2 as well as NO, so do they emit some small quantities of SO
3 when they burn sulfur-containing fuels. Leighton
[2] also discussed the oxidation of SO
2 in polluted atmospheres, and an excellent review by Bulfalini
[3] has appeared. This section draws heavily from these sources.
The chemical problem here involves the photochemical and catalytic oxidation of SO2 and its mixtures with the hydrocarbons and NO; however the primary concern is the photochemical reactions, both gas-phase and aerosol-forming.
The photodissociation of SO2 into SO and O atoms is markedly different from the photodissociation of NO2. The bond to be broken in the sulfur compound requires about 560 kJ/mol. Thus, wavelengths greater than 2180 Å do not have sufficient energy to initiate dissociation. This fact is significant in that only solar radiation greater than 2900 Å reaches the lower atmosphere. If a photochemical effect is to occur in the SO2−O2 atmospheric system, it must be that the radiation electronically excites the SO2 molecule but does not dissociate it.
There are two absorption bands of SO2 within the range 3000–4000 Å. The first is a weak absorption band and corresponds to the transition to the first excited state (a triplet). This band originates at 3880 Å and has a maximum around 3840 Å. The second is a strong absorption band and corresponds to the excitation to the second excited state (a triplet). This band originates at 3376 Å and has a maximum around 2940 Å.
Blacet
[4], who carried out experiments in high O
2 concentrations, reported that ozone and SO
3 appear to be the only products of the photochemically induced reaction. The following essential steps were postulated:
SO2+hv→SO∗2
(8.30)
SO∗2+O2→SO4
(8.31)
SO4+O2→SO3+O3
(8.32)
The radiation used was at 3130 Å, and it would appear that the excited
SO∗2 in reaction
(8.30) is a singlet. The precise roles of the excited singlet and triplet states in the photochemistry of SO
2 are still unclear
[3]. Nevertheless, this point need not be of great concern since it is possible to write the reaction sequence
SO2+hv→S1O∗2
(8.33)
S1O∗2+SO2→S3O∗2+SO2
(8.34)
Thus, reaction
(8.30) could specify either an excited singlet or triplet
SO∗2. The excited state may, of course, degrade by internal transfer to a vibrationally excited ground state that is later deactivated by collision, or it may be degraded directly by collisions. Fluorescence of SO
2 has not been observed above 2100 Å. The collisional deactivation steps known to exist in laboratory experiments are not listed here, to minimize the writing of reaction steps.
Since they involve one species in large concentrations, reactions
(8.30)–
(8.32) are the primary ones for the photochemical oxidation of SO
2 to SO
3. A secondary reaction route to SO
3 could be
SO4+SO2→2SO3
(8.35)
In the presence of water a sulfuric acid mist forms according to
H2O+SO3→H2SO4
(8.36)
The SO
4 molecule formed by reaction
(8.31) would probably have a peroxy structure, and if
SO∗2 were a triplet, it might be a biradical.
There is conflicting evidence with respect to the results of the photolysis of mixtures of SO2, NOx, and O2. However, many believe that the following should be considered with the NOx photolysis reactions:
SO2+NO→SO+NO2
(8.37)
SO2+NO2→SO3+NO
(8.38)
SO2+O+M→SO3+M
(8.39)
SO2+O3→SO3+O2
(8.40)
SO3+O→SO2+O2
(8.41)
SO4+NO→SO3+NO2
(8.42)
SO4+NO2→SO3+NO3
(8.43)
SO4+O→SO3+O2
(8.44)
SO+O+M→SO2+M
(8.45)
SO+O3→SO2+O2
(8.46)
SO+NO2→SO2+NO
(8.47)
The important reducing effect of the SO2 with respect to different polluted atmospheres mentioned in the introduction of this section becomes evident from these reactions.
Some work
[5] has been performed on the photochemical reaction between sulfur dioxide and hydrocarbons, both paraffins and olefins. In all cases, mists were found, and these mists settled out in the reaction vessels as oils with the characteristics of sulfuric acids. Because of the small amounts of materials formed, great problems arise in elucidating particular steps. When NO
x and O
2 are added to this system, the situation is most complex. Bulfalini
[3] summed up the status in this way: “The aerosol formed from mixtures of the lower hydrocarbons with NO
x and SO
2 is predominantly sulfuric acid, whereas the higher olefin hydrocarbons appear to produce carbonaceous aerosols also, possibly organic acids, sulfonic or sulfuric acids, nitrate-esters, etc.”