01.08.2021 Views

Energy and Human Ambitions on a Finite Planet, 2021a

Energy and Human Ambitions on a Finite Planet, 2021a

Energy and Human Ambitions on a Finite Planet, 2021a

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

9 Climate Change 146<br />

change, but a hefty passenger.<br />

No greenhouse gases<br />

Greenhouse gases<br />

Figure 9.9: In the absence of greenhouse<br />

gases, infrared radiati<strong>on</strong> has no difficulty<br />

escaping to space (left). When greenhouse<br />

gases (GHGs) are present (right), most of<br />

the infrared radiati<strong>on</strong> is absorbed by GHG<br />

molecules. These molecules later release the<br />

absorbed energy as new infrared radiati<strong>on</strong>,<br />

but in a r<str<strong>on</strong>g>and</str<strong>on</strong>g>omized directi<strong>on</strong>, so that some<br />

energy is returned to the ground, thereby<br />

keeping the surface warmer than it would<br />

be without greenhouse gases.<br />

Naïvely speaking, going from 280 ppm v to 420 ppm v (an increase by a<br />

factor of 1.5), might be expected to turn the 8.6 ◦ C greenhouse effect from<br />

CO 2 into 12.9 ◦ C (1.5×) for a 4.3 degree human-caused warming. 24 But 24: This is not how it works.<br />

the CO 2 absorpti<strong>on</strong> feature at ∼ 15 μmissaturated,soasCO 2 is added, it<br />

becomes wider, but logarithmically rather than linearly as a functi<strong>on</strong> of<br />

CO 2 c<strong>on</strong>centrati<strong>on</strong>. Climate scientists often express the impact of various<br />

influences as a radiative forcing, measured in W/m 2 .<br />

Definiti<strong>on</strong> 9.2.1 Radiative forcing is used to describe the areal power (in<br />

W/m 2 ) of absorbed solar energy <str<strong>on</strong>g>and</str<strong>on</strong>g> infrared radiati<strong>on</strong> to space. Various<br />

influences or c<strong>on</strong>stituents each c<strong>on</strong>tribute their own radiative forcing. In<br />

equilibrium, a balance exists so that the net 25 radiative forcing is zero.<br />

25: . . . sum of all: positive <str<strong>on</strong>g>and</str<strong>on</strong>g> negative<br />

The average solar forcing is<br />

RF ⊙ 1360 W/m 2 × 0.707/4 ≈ 240 W/m 2 , (9.3)<br />

sharing substantial overlap with Eq. 9.2—the factors having been explained<br />

in that c<strong>on</strong>text. Without adding to the pre-industrial set of<br />

greenhouse gases (GHGs), we would solve for temperature 26 as<br />

26: . . . adding the baseline 33◦ C GHG c<strong>on</strong>tributi<strong>on</strong><br />

( ) 0.25 RF⊙<br />

T + 33, (9.4)<br />

σ<br />

evaluating to 288 K, or about 15 ◦ C. If we add (or deduct) radiative forcing<br />

from another source, it would add (subtract) in the numerator of Eq.<br />

9.4. The additi<strong>on</strong> of CO 2 over the original amount (CO 2,orig ; 280 ppm v )<br />

generates a radiative forcing of<br />

( )<br />

CO 2<br />

RF CO2 5.35 ln<br />

W/m 2 , (9.5)<br />

CO 2,orig<br />

where the ln() functi<strong>on</strong> is the natural logarithm. 27 At our present<br />

∼420 ppm v , the ratio of current CO 2 to CO 2,orig is 1.5 <str<strong>on</strong>g>and</str<strong>on</strong>g> RF CO2 ≈<br />

2.2W/m 2 , so that the new temperature (adding the new forcing to Eq.<br />

9.4)is<br />

( RF⊙ + RF CO2<br />

27: . . . capturing the logarithmic broadening<br />

of the width of the CO 2 absorpti<strong>on</strong><br />

feature at 15 μm inFigure 9.7<br />

T <br />

σ<br />

) 0.25<br />

+ 33 ≈ 288.6, (9.6)<br />

© 2021 T. W. Murphy, Jr.; Creative Comm<strong>on</strong>s Attributi<strong>on</strong>-N<strong>on</strong>Commercial 4.0 Internati<strong>on</strong>al Lic.;<br />

Freely available at: https://escholarship.org/uc/energy_ambiti<strong>on</strong>s.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!