Solar spectrum outside atmosphere Solar spectrum at sea level Ultraviolet Visible Infrared 1000 1400 1800 Wavelength (nm) 200 600 2200 2600 3000 Increasing flux-

Fundamentals Of Analytical Chemistry
9th Edition
ISBN:9781285640686
Author:Skoog
Publisher:Skoog
Chapter25: Instruments For Optical Spectrometry
Section: Chapter Questions
Problem 25.16QAP
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Silicon has a band gap of 1.1 eV at room temperature.
(a) What wavelength of light would a photon of this energy
correspond to? (b) Draw a vertical line at this wavelength in
the figure shown, which shows the light output of the Sun
as a function of wavelength. Does silicon absorb all, none,
or a portion of the visible light that comes from the Sun?
(c) You can estimate the portion of the overall solar spectrum
that silicon absorbs by considering the area under the
curve. If you call the area under the entire curve “100%,”
what approximate percentage of the area under the curve is
absorbed by silicon?

Solar spectrum outside atmosphere
Solar spectrum at sea level
Ultraviolet
Visible Infrared
1000
1400
1800
Wavelength (nm)
200
600
2200
2600
3000
Increasing flux-
Transcribed Image Text:Solar spectrum outside atmosphere Solar spectrum at sea level Ultraviolet Visible Infrared 1000 1400 1800 Wavelength (nm) 200 600 2200 2600 3000 Increasing flux-
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