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First Assessment Report - IPCC

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2 Radiatn e Foi c mg of Climate 61<br />

Table 2.9: Example of use of Global Waiminq Potentials<br />

The table shows the mtegiated effects o\ei a 100 yeai time<br />

hoiizon of total emissions in 1990 i>i\en as a fiaction of<br />

the total effec t<br />

Trace Gas<br />

co 2<br />

CH4<br />

N20<br />

CFC-11<br />

CFC 12<br />

HCFC-22<br />

CFC 113<br />

CFC-114<br />

CFC 115<br />

CCI4<br />

CH3CCI3<br />

CO<br />

NO x<br />

NMHCs<br />

Current Man<br />

Made Emissions<br />

Tgyr-1<br />

26000<br />

300<br />

6<br />

03<br />

04<br />

01<br />

0 15<br />

0015<br />

0 005<br />

0 09<br />

081<br />

200<br />

66<br />

20<br />

Proportion of<br />

total effects<br />

%<br />

61<br />

15<br />

4<br />

2<br />

7<br />

04<br />

15<br />

02<br />

01<br />

03<br />

02<br />

1<br />

6<br />

05<br />

Carbon dioxide emissions given on CO2 basis,<br />

equivalent to 7 GtC yr"' Nitrous oxide<br />

emissions given on N2O basis, equivalent to 4<br />

MtN yr ' NO x emissions given on NO2 basis<br />

equivalent to 20 MtN yr '<br />

negative indirect effect of NO x emissions which would<br />

oppose the forcing due to increased troposphenc oiont<br />

formation<br />

As an example of the use of the Global Warming<br />

Potentials, Table 2 9 shows the integrated effects over a<br />

100 year time horizon for the estimated human-related<br />

greenhouse gas emissions in 1990 The derived cumulative<br />

effects, derived by multiplying the appropriate GWP by the<br />

1990 emissions rate, indicates that CO2 will account for<br />

61% of the radiative forcing over this time period<br />

Emissions of NO x , whose effect is entirely indirect is<br />

calculated to contribute 6% to the total forcing<br />

2.3 Other Radiative Forcing Agents<br />

231 Solar Radiation<br />

The Sun is the primary source of energy tor the Earth s<br />

climate system Variations in the amount of solar iadiation<br />

received by the I arth can affect our climate There are two<br />

distinct sources of this variability The first which acts<br />

with greatest impact on time-scales of 10,000 to 100,000<br />

years is caused by changes in the Sun-Earth orbital<br />

parameters The second comes from physical changes on<br />

the Sun itself, such changes occur on almost all time-scales<br />

2 3 11 Vai /ability due to 01 bital chanqes<br />

Variations in climate on time-scales ranging from 10,000 to<br />

100,000 years, including the major glacial/interglacial<br />

cycles during the Quaternary period, are believed to be<br />

initiated by variations in the Earth s orbital parameters<br />

which in turn influence the latitudinal and seasonal<br />

variation of solar energy received by the Earth (the<br />

Milankovitch Effect) Although the covariation of these<br />

orbital parameters and the Earth s climate provides a<br />

compelling argument in favour of this theory, internal<br />

feedback processes have to be invoked to explain the<br />

observed climatic variations, in particular the amplitude of<br />

the dominating 100,000 year period one such feedback<br />

could be the changes to the carbon cycle and the<br />

greenhouse effect of atmospheric CO2 (see Section 1)<br />

The radiative forcing associated with the Milankovitch<br />

Effect can be given for particular latitudes and months to<br />

illustrate that the rate of change of forcing is small<br />

compared to radiative forcing due to the enhanced<br />

greenhouse effect, of course, the climatic impact of the<br />

Milankovitch Effect results from the redistribution of solar<br />

energy, latitudinally and seasonally, so that a comparison is<br />

necessarily rather rough As an example, in the past 10,000<br />

years, the incident solar radiation at 60°N in July has<br />

decreased by about 35 Wm-2 ( e g , Rind et al , 1989), the<br />

average change in one decade is -0 035 Wm-2, compared<br />

with the estimate, in Section 2 2 5, that the greenhouse<br />

forcing over the most recent decade increased by 0 6<br />

Wm-2 more than 15 times higher than the Milankovitch<br />

forcing<br />

2 3 12 Vai lability due to chaises in total sola/ madiance<br />

Variations in the short-wave and radio-frequency outputs of<br />

the Sun respond to changes in the surface activity of the<br />

star and follow in phase with the 11-year sunspot cycle<br />

The greatest changes, in terms of total energy, occur in the<br />

short-wave region, and particularly the near ultraviolet At<br />

0 3 u.m, the solar cycle variation is less than 1%, since only<br />

about 1% of the Suns radiation lies at this or shorter<br />

wavelengths solar-cycle variations in the ultraviolet will by<br />

themselves induce variations of no more than 0 01% in<br />

total irradiance, although these may be important for<br />

atmospheric chemistry in the middle atmosphere<br />

Of greater potential importance, in terms of direct affects<br />

on climate are changes integrated over all wavelengths the<br />

total solai irradiance or the so-called solar constant<br />

Continuous spaceborne measurements of total irradiance<br />

have been made since 197S These have shown that on<br />

time-scales of days to a decade there are irradiance

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