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Energy and Human Ambitions on a Finite Planet, 2021a

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13 Solar <str<strong>on</strong>g>Energy</str<strong>on</strong>g> 208<br />

the sky near the equator, so panels there should lie flat. 48 But at high<br />

northern latitudes, the sun is lower toward the southern horiz<strong>on</strong>, so the<br />

panels should tilt up to best face the sun. Tilting at an angle equal to the<br />

latitude is the best compromise, as Figure 13.10 illustrates.<br />

sun view sun view side view<br />

flat panels titled panels titled panels<br />

48: . . . point mostly up<br />

Figure 13.10: The left globe shows the sun’s<br />

view of 21 panels of the same size sitting<br />

flat <strong>on</strong> the ground at their various sites. In<br />

the middle globe, the panels are all tilted<br />

up toward the equator. Notice the improvement<br />

in how much panel area is visible to<br />

the sun by doing this—especially at higher<br />

latitudes. At right is the side view, from<br />

which it is easier to appreciate why the best<br />

tilt angle is equal to the site latitude.<br />

Figure 13.11: Solar potential for flat panels<br />

tilted to latitude, oriented south—relevant<br />

to PV panel installati<strong>on</strong>s. The graphic is presented<br />

in units of kWh/m 2 /day, the breakpoints<br />

between colors running from 3.0 to<br />

6.5 kWh/m 2 /day in steps of 0.5. Annotati<strong>on</strong>s<br />

are added <strong>on</strong>ce in each color b<str<strong>on</strong>g>and</str<strong>on</strong>g> (in<br />

black or yellow) to indicate the equivalent<br />

measure in W/m 2 [87]. From NREL.<br />

Tilting panels toward the equator at an angle equal to site latitude<br />

optimizes annual yield, <str<strong>on</strong>g>and</str<strong>on</strong>g> the results are shown in Figure 13.11. Note<br />

that the numbers in Figure 13.11 are not strictly insolati<strong>on</strong>s, since that’s<br />

defined as what reaches flat ground. In this case, the area (square meters)<br />

is that of the panel, not of the l<str<strong>on</strong>g>and</str<strong>on</strong>g>.<br />

The fact that the numbers in Figure 13.11 are higher than in Figure 13.9 is<br />

not to say that the l<str<strong>on</strong>g>and</str<strong>on</strong>g> offers more solar energy if the panels are tilted:<br />

just that an individual panel can get more light. But in this case, panels<br />

need to be spaced out to avoid shadowing, 49 as Figure 13.12 illustrates.<br />

Some applicati<strong>on</strong>s need to track the sun, like those that c<strong>on</strong>centrate<br />

solar power, <str<strong>on</strong>g>and</str<strong>on</strong>g> <strong>on</strong>ly work when the sun is not blocked by clouds. 50<br />

This brings us to Figure 13.13, showing the potential per square meter of<br />

collector (mirror or lens) used for the c<strong>on</strong>centrati<strong>on</strong> (the topic of Secti<strong>on</strong><br />

13.8.2). The same pattern holds, in that the desert southwest dominates.<br />

But a look at the numbers indicates that the cloudier regi<strong>on</strong>s are not<br />

much better than just a flat panel facing upward (as is the case for Figure<br />

13.9). In the southwest, where skies are often cloud-free, the boost can<br />

49: . . . which can be more devastating than<br />

just fracti<strong>on</strong>al area blocked, due to series<br />

arrangement of cells in panel modules<br />

50: Photovoltaics still produce 10–50% of<br />

full capacity under cloudy skies during daylight<br />

hours, depending <strong>on</strong> how thick the<br />

clouds are: daylight still means phot<strong>on</strong>s.<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.

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