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Botkin Environmental Science Earth as Living Planet 8th txtbk

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20.7 The Major Greenhouse G<strong>as</strong>es 443<br />

atmosphere, resulting in high internal fluxes. For example,<br />

in terms of the figure, the amount of IR absorbed at <strong>Earth</strong>’s<br />

surface from the greenhouse effect is approximately 88<br />

units, which is about twice the amount of shortwave solar<br />

radiation (45 units) absorbed by <strong>Earth</strong>’s surface. Despite<br />

the large internal fluxes, the overall energy balance remains<br />

the same. At the top of the atmosphere, the net downward<br />

solar radiation (70 units, 45 units 25 units) balances the<br />

outgoing IR from the top of the atmosphere (70 units).<br />

The important point here is recognizing the strength<br />

of the greenhouse effect. For example, notice in the figure<br />

that of the 104 units of IR emitted by the surface of <strong>Earth</strong>,<br />

only 4 go directly to the upper atmosphere and are emitted.<br />

The rest is reabsorbed and reemitted by greenhouse<br />

g<strong>as</strong>es. Of these, 88 units are directed downward to <strong>Earth</strong><br />

and 66 units upward to the upper atmosphere.<br />

All this may sound somewhat complicated, but if<br />

you read and study the points mentioned in Figures<br />

20.15 to 20.17 carefully and work through the balances<br />

of the various parts of the energy fluxes, you will gain<br />

a deeper understanding of why the greenhouse effect is<br />

so important. The greenhouse effect keeps <strong>Earth</strong>’s lower<br />

atmosphere approximately 33°C warmer than it would<br />

otherwise be and performs other important service functions<br />

<strong>as</strong> well. For example, without the strong downward<br />

emission of IR from the greenhouse effect, the land surface<br />

would cool much f<strong>as</strong>ter at night and warm much<br />

more quickly during the day. In sum, the greenhouse<br />

effect helps to limit temperature swings from day to<br />

night and maintain relatively comfortable surface temperatures.<br />

It is, then, not the greenhouse effect itself but<br />

the changes in greenhouse g<strong>as</strong>es that are a concern.<br />

20.7 The Major Greenhouse<br />

G<strong>as</strong>es<br />

The major anthropogenic greenhouse g<strong>as</strong>es are listed in<br />

Table 20.1. The table also lists the recent rate of incre<strong>as</strong>e<br />

for each g<strong>as</strong> and its relative contribution to the anthropogenic<br />

greenhouse effect.<br />

Carbon Dioxide<br />

Current estimates suggest that approximately 200 billion<br />

metric tons of carbon in the form of carbon dioxide (CO 2 )<br />

enter and leave <strong>Earth</strong>’s atmosphere each year <strong>as</strong> a result of<br />

a number of biological and physical processes: 50 to 60%<br />

of the anthropogenic greenhouse effect is attributed to this<br />

g<strong>as</strong>. Me<strong>as</strong>urements of carbon dioxide trapped in air bubbles<br />

in the Antarctic ice sheet suggest that 160,000 years before<br />

the Industrial Revolution the atmospheric concentration<br />

of carbon dioxide varied from approximately 200 to 300<br />

ppm. 12 The highest level or concentration of carbon dioxide<br />

in the atmosphere, other than today’s, occurred during<br />

the major interglacial period about 125,000 years ago.<br />

About 140 years ago, just before the major use of fossil<br />

fuels began <strong>as</strong> part of the Industrial Revolution, the atmospheric<br />

concentration of carbon dioxide w<strong>as</strong> approximately<br />

280 ppm. 13 Since then, and especially in the p<strong>as</strong>t few<br />

decades, the concentration of CO 2 in the atmosphere h<strong>as</strong><br />

grown rapidly. Today, the CO 2 concentration is about 392<br />

ppm, and at its current rate of incre<strong>as</strong>e of about 0.5% per<br />

year, the level may rise to approximately 450 ppm by the year<br />

2050—more than 1.5 times the preindustrial level. 13<br />

Table 20.1<br />

MAJOR GREENHOUSE GASES<br />

TRACE GASES RELATIVE CONTRIBUTION (%) GROWTH RATE (%/YR)<br />

CFC 15 a -25 b 5<br />

CH 4 12 a -20 b 0.4 c<br />

O 3 (troposphere) 8 d 0.5<br />

N 2 O 5 d 0.2<br />

Total 40–50<br />

Contribution of CO 2 50–60 0.3 e –0.5 d,f<br />

a W. A. Nierenberg, “Atmospheric CO 2 : Causes, Effects, and Options,” Chemical Engineering Progress 85, no.8 (August 1989): 27<br />

b<br />

J. Hansen, A. Lacis, and M. Prather, “Greenhouse Effect of Chlorofluorocarbons and Other Trace G<strong>as</strong>es,” Journal of Geophysical<br />

Research 94 (November 20, 1989): 16, 417.<br />

c Over the p<strong>as</strong>t 200 yrs.<br />

d H. Rodha, “A Comparison of the Contribution of Various G<strong>as</strong>es to the Greenhouse Effect,” <strong>Science</strong> 248 (1990): 1218, Table 2.<br />

e<br />

W. W. Kellogg, “Economic and Political Implications of Climate Change,” paper presented at Conference on Technology-b<strong>as</strong>ed<br />

Confidence Building: Energy and Environment, University of California, Los Alamos National Laboratory, July 9–14, 1989.<br />

f H. Abelson, “Uncertainties about Global Warming,” <strong>Science</strong> 247 (March 30,1990): 1529.

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