Gases I could expect to see using an IR receiver

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Discussion Overview

The discussion revolves around the types of gases detectable using an infrared (IR) receiver within the wavelength range of 110 to 330 nm, along with considerations for appropriate glass materials that would not interfere with measurements. The conversation includes aspects of infrared spectrometry and the setup required for effective detection.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Experimental/applied

Main Points Raised

  • One participant inquires about the types of gases detectable with an IR receiver in the specified wavelength range and seeks information on suitable glass types.
  • Another participant points out a potential error in the wavelength range, suggesting it falls within the blue end of the visible spectrum and into ultraviolet (UV).
  • A participant clarifies that they meant to refer to wavenumbers (cm^-1) instead of wavelengths.
  • Discussion includes the idea that weakly polyatomic molecules with heteronuclear bonds may exhibit vibrations and rotations detectable in the IR range.
  • Another participant requests sources for gas wavelength data and emphasizes the need for glass that does not affect results.
  • A suggestion is made to consult resources like "Sadtler" for data on far IR and to explore chemical and physical abstracts for specific compounds.
  • A later post discusses the requirements for infrared spectrometry, including the need for both an infrared source and a separate light source, and questions how to ensure sufficient infrared light reaches the detector after passing through various components.

Areas of Agreement / Disagreement

Participants express uncertainty regarding the initial wavelength range and its implications for gas detection. There is no consensus on the specific gases detectable or the optimal glass type, and the discussion remains unresolved regarding the technical setup for infrared spectrometry.

Contextual Notes

Participants have not fully established the assumptions regarding the wavelength range and its relation to gas detection. There are unresolved questions about the effectiveness of different glass types and the configuration of the spectrometer setup.

Who May Find This Useful

This discussion may be of interest to those involved in experimental physics, chemistry, or engineering, particularly in the fields of spectroscopy and gas detection technologies.

bertopolis
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Hi I was wondering if someone could tell me what kind of gases I could expect to see using an IR receiver between the wavelengths of 110 and 330 nm. As well as this id love to know what kind of glass could be used in order to not interfere with the actual results.
Thanks a million
 
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bertopolis said:
IR receiver ... 110 and 330 nm
Check your numbers. You've listed blue end of visible, and into UV.
 
sorry i meant cm^-1
 
Vibrations of weak bonds, rotations. Fill in the blanks for weakly polyatomic molecules with heteronuclear bonds.
 
Would you know anywhere that could be a source of the wavelength of gases in this interval? I've been trying to find what gases could be found here for various weeks, although my more pressing question is what glass type can be used in order for results to not be affected.
Thanks for all your help
 
You want a "Sadtler" for very far IR, into radar/microwave range?
There may be such, " http://www.lib.utexas.edu/chem/info/sadtler.html ," but if UT says it's beyond their budget, I'm sure it's beyond mine to even browse for compiled data. Your best bet is going to be Chem./Phys. Abstracts, or Sci. Cit. for specific compounds that interest you.
 
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Thanks a Million.
I just learned that when doing infrared spectrometry there must be an infrared source and another light source( eg. He Ne laser) but of course both these would need individual detectors, would this be done by placing a beam splitter at the exit of the spectrometer after the light has been "in contact" with the gas source?
And given that the source is a weak infrared diode and the infrared detector is a photo-diode, how can one insure there is sufficient infrared light reaching the detector once it has passed through the spectrometer/interferometer, source and possibly the beam splitter?
Thanks
 

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