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electrical:solar:output [2023/02/04 12:50] frater_secessus [zenith angle] |
electrical:solar:output [2024/11/22 11:44] (current) frater_secessus [where and when] |
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Because the difference between lab and actual conditions is so large, some manufacturers also publish [[https:// | Because the difference between lab and actual conditions is so large, some manufacturers also publish [[https:// | ||
- | In practical terms, it's common to see a maximum of 75% of STC under good conditions, more under great conditions, and much less under poor solar conditions. | + | In practical terms, it's common to see a maximum of 75% of STC under good conditions, more under great conditions, and much less under poor solar conditions. |
+ | |||
+ | ===== where and when ===== | ||
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+ | The location and season both have profound effects on solar harvest. [[opinion: | ||
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+ | For more specific numbers you can estimate solar harvest using [[electrical: | ||
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===== lack of demand ===== | ===== lack of demand ===== | ||
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===== zenith angle ===== | ===== zenith angle ===== | ||
- | The sun will climb in the sky until it reaches its highest point for the day (local solar noon), then will start dropping again: | + | The sun will climb in the sky until it reaches its highest point for the day (local solar noon), then will start dropping again. This affects how much power you can harvest: |
{{ https:// | {{ https:// | ||
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Tip: you can work backwards from cosine calculations and observed power harvests to find your system' | Tip: you can work backwards from cosine calculations and observed power harvests to find your system' | ||
+ | ==== paradox of big solar ==== | ||
+ | |||
+ | All other things being equal, peak harvest will happen at local solar noon((rarely clock-noon)) when the sun is highest in the sky. | ||
+ | |||
+ | This leads to a paradox: | ||
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// | // | ||
- | * hours of seasonal daylight | + | * short term |
- | * clouds | + | * angle at which rays strikes the panel (angle of incidence) |
- | * rain, fog | + | * amount of atmosphere the rays have to penetrate (less at solar noon, more at other times or anytime sun is relatively lower on the horizon) |
- | | + | * clouds |
- | * amount of atmosphere the rays have to penetrate (less at solar noon, more at other times or anytime sun is relatively lower on the horizon) | + | * rain, fog |
- | * air quality: | + | |
* altitude (total irradiance ~+2.67%/ | * altitude (total irradiance ~+2.67%/ | ||
* humidity((https:// | * humidity((https:// | ||
+ | * long term - roughly speaking, you can expect ~half the harvest in winter compared to summer | ||
+ | * solar angle due to **time of year**. | ||
+ | * hours of seasonal daylight | ||
+ | |||
Even the altitude and type of clouds can affect harvest: | Even the altitude and type of clouds can affect harvest: | ||
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+ | ==== using PVWatts to find FSE and daily harvest ==== | ||
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+ | this subsection has been [[electrical: | ||
==== insolation maps ==== | ==== insolation maps ==== | ||
- | Insolation maps attempt to combine the effects of the variables above to estimate hours of **full sun((1000W/ | + | Insolation maps attempt to combine the effects of the variables above to estimate hours of **full sun((1000W/ |
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Pro: | Pro: | ||
- | * +30% daily harvest | + | * optimal tilt will increase |
- | * can be used to increase harvest if roof space is maxxed (cannot add more panel) | + | * can be used to further |
Con: | Con: | ||
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[[https:// | [[https:// | ||
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+ | ===== sensitivity to light spectrum ===== | ||
+ | |||
+ | Note: these differences exist but are of little practical effect. | ||
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+ | ==== differences in light ==== | ||
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+ | * direct sunlight is broad-spectrum (a mix of light wavelengths) | ||
+ | * when the sun is near the horizon the available light is more red (longer wavelengths) | ||
+ | * when skies are overcast or otherwise diffused the available light is more blue (shorter wavelengths) | ||
+ | |||
+ | Since the latter point is counterintuitive: | ||
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+ | >> at visible wavelengths, | ||
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+ | ==== differences in panel sensitivity ==== | ||
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+ | {{ https:// | ||
+ | Note: | ||
+ | |||
+ | * [redder end] | ||
+ | * CIGS (copper indium gallium selenide) thin-film panels have peak sensitivity around 950nm. | ||
+ | * monocrystalline silicon panels (mono, c-Si) tend to have maximal spectral response around 900nm | ||
+ | * polycrstalline silicon panels (poly, mc-Si, | ||
+ | * GaAs (gallium arsenide) thin-film panels have peak response around 825nm. | ||
+ | * CdTe (Cadmium Telluride) flex panels, the most popular thin-film type, have peak response around 750nm. | ||
+ | * amorphous silicon panels (a-Si, the original noncrystalline panel) - have peak response around 550nm. | ||
+ | * [ bluer end ] | ||
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