Exploring Sunlight in the Atmosphere: IR Wavelengths

In summary, there are many different wavelengths that get absorbed by the atmosphere, including IR radiation. This makes it difficult to measure certain parts of the spectrum, such as the ones emitted by excited gas molecules.
  • #1
atlstroke
8
0
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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  • #2
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.
 
  • #3
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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  • #4
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
 
  • #5
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.
 

1. What is infrared (IR) light and how does it differ from visible light?

Infrared light is a type of electromagnetic radiation with longer wavelengths than visible light. It is not visible to the human eye, but can be felt as heat. Unlike visible light, IR light has longer wavelengths and lower frequencies.

2. How does sunlight interact with the Earth's atmosphere and why is it important to study IR wavelengths?

Sunlight is composed of various wavelengths, including IR. As sunlight enters the Earth's atmosphere, it can be absorbed, reflected, or scattered by gases and particles in the atmosphere. Studying IR wavelengths can help us understand how the Earth's atmosphere affects the distribution of heat and energy on our planet.

3. What are some techniques used to explore IR wavelengths in the atmosphere?

One common technique is remote sensing, which uses instruments such as satellites and aircraft to measure and analyze IR radiation from the atmosphere. Other methods include ground-based measurements using spectrometers and radiometers.

4. How does the presence of greenhouse gases affect IR wavelengths in the atmosphere?

Greenhouse gases, such as carbon dioxide and methane, have the ability to absorb and trap IR radiation in the atmosphere. This leads to an increase in temperature, known as the greenhouse effect. Studying IR wavelengths can help us understand how greenhouse gases contribute to climate change.

5. What are some potential applications of studying IR wavelengths in the atmosphere?

Studying IR wavelengths can have various applications, such as monitoring weather patterns, tracking changes in the Earth's climate, and detecting air pollution. It can also aid in the development of more accurate climate models and inform strategies for mitigating the effects of climate change.

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