Are There Disproportionate IR Wavelengths in Sunlight Reaching the Atmosphere?

AI Thread Summary
The discussion focuses on the spectrum of sunlight as it reaches the upper atmosphere and the Earth's surface, highlighting the filtering effects of the atmosphere on various wavelengths. Above the atmosphere, sunlight retains its original spectrum, while atmospheric absorption significantly alters it, particularly affecting UV radiation due to the ozone layer. Participants express interest in whether specific infrared wavelengths are disproportionately represented when considering radiation reflected or emitted from the ground and surrounding gases. Historical research on solar spectra, dating back to the 1800s, is referenced to support the inquiry into these phenomena. Overall, understanding these spectral changes requires access to scientific literature and measurement resources.
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Can anyone speak on the spectrum of sunlight reaching the upper atmosphere and the surface ? Specifically I interested in finding out if there are any IR wavelengths disproportionally represented when compared to the original source.

Please limit responses to constructive ones.
 
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By "upper atmosphere" do you mean above the atmosphere? If you are above the Earth's atmosphere, the spectrum of sunlight reaching you would be almost exactly that as given off by the sun. If you are inside the Earth's atmosphere, then many wavelengths get filtered out by the atmosphere itself, including UV radiation being filtered out by the ozone layer.
 
Try this: http://en.wikipedia.org/wiki/Air_mass_(solar_energy)

The charts show solar radiation at the top of the atmosphere, the black body (ideal) spectrum for the sun, and the solar spectrum at the ground. Note the many gaps in the last - these are the wavelengths absorbed by the atmosphere.
 
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Thanks ultra, since this shows a nice smooth average decline I get the impression that this exclusively speaks to attenuation/absorption of incoming solar radiation. I am wondering if when we add the radiation reflected/emitted from the ground and the IR emitted from the surrounding excited gas molecules are there any wavelengths within the IR part of the spectrum that show unexpected peaks.

Making up numbers for an example would there be peaks at 75 micrometers and 150 micrometers that would correspond to the amount emitted by excited gas molecules.

Thanks
 
There has been a great deal of research on the solar spectrum at ground level, dating back probably well into the 1800's. Bunsen & Kirchoff began photographing stellar and solar spectra in 1860:
http://www.chemteam.info/Chem-History/Kirchhoff-Bunsen-1860.html

For an introduction to the measurement issues see:
http://www.newport.com/Introduction-to-Solar-Radiation/411919/1033/content.aspx

With the right concepts you should be able to find whatever interests you via any university library, or Google Scholar.
 
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