What is self and air broadening effects?

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SUMMARY

Self and air broadening effects are critical phenomena in atmospheric modeling, particularly relevant to the pressure broadening or collisional broadening of spectral lines emitted by gases. These effects significantly impact remote sensing applications, especially in satellite microwave sounders and the study of dense plasma emissions. While there is no precise theory to fully describe these broadening effects, heuristic models provide adequate descriptions. For further understanding, resources such as Wikipedia's article on "Spectral Line" and Grant W. Petty's work on atmospheric radiation are recommended.

PREREQUISITES
  • Understanding of spectral line broadening concepts
  • Familiarity with atmospheric modeling techniques
  • Knowledge of remote sensing technologies
  • Basic principles of radiation interaction with gases
NEXT STEPS
  • Research "pressure broadening" in atmospheric physics
  • Explore "Doppler broadening" and its implications
  • Study the "Spectral Line" article on Wikipedia for foundational knowledge
  • Read Grant W. Petty's book on atmospheric radiation for in-depth insights
USEFUL FOR

Atmospheric scientists, remote sensing engineers, and researchers involved in modeling radiation interactions in dense gases will benefit from this discussion.

nordmoon
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What is self and air broadening effects? I have read that they appear in atmospheric modelling. Is this pressure broadening?
 
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nordmoon said:
What is self and air broadening effects? I have read that they appear in atmospheric modelling. Is this pressure broadening?

There is a "broadening" in spectral lines of emission of radiation from a gas. This is quite important for remote sensing by satellites with microwave sounders, and also for modeling how radiation interacts with the atmosphere. It is also relevant to study of emission lines in the spectrum from a dense plasma, such as the atmosphere of a star.

For problems relating to how thermal radiation interacts with an atmosphere, the relevant effect is called "pressure broadening" or "collisional broadening"; the collisions between atoms in a dense gas can alter the energy of radiation emission, which broadens the corresponding spectral line. It's a rather horribly complicated effect to model accurately; in fact I understand there is no exact theory to describe the broadening effects of pressure on spectral lines; although there are adequate heuristic descriptions.

Wikipedia gives a brief summary of the kinds of broadening of spectral lines that can occur; and this may help give pointer to where to find more detail from more technical sources of information. See Spectral line broadening and shift within the wikipedia article on "Spectral Line".

A good discussion is also available in http://www.sundogpublishing.com/AtmosRad/index.html, by Grant W. Petty (Published 2006, Sundog publishing). The link goes to a webpage for the book and you can browse the first edition for free. Pressure broadening and doppler broadening are discussed in chapter 9.

Cheers -- sylas
 

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