Astrophysics (index)

Absorption

(removal of photons from a beam of EMR)

The term Absorption is used in the study of Radiative Transfer (RT) and Spectroscopy to mean the removal of photons to a beam of Electromagnetic Radiation (EMR) (e.g., light), e.g., through interactions of photons and particles such as molecules, atoms, ions, or electrons. The term includes the removal effects of scattering. It is the inverse of Emission, the addition of photons to the beam. The concept is used widely in astrophysics, for explaining and modeling stars, for dealing with the effects of the Earth's Atmosphere, for explaining and modeling gas clouds, etc.

Absorption is complicated because of the many different processes that cause it, and varies by the density, the makeup, the Temperature, of the material the beam is passing through. Absorption Lines are a result of a type of absorption that is very sensitive to Wavelength.

A classification of types of absorption is based upon the status of an electron with the photon is interacting:

  • Bound-Bound - with an electron that is bound to an atom both before and after the interaction: this is the type of absorption that results in Spectral Lines.
  • Bound-Free - an electron being freed from an atom such as a neutral atom being ionized. This is called the Photoelectric Effect or Photoionization.
  • Free-Free - an electron absorbing a photon, which can only happen when near a charged particle such as an ion.
  • Electron Scattering - Thomson Scattering or Compton Scattering.

The last is also emission, and the other three all have an inverse which is emission.


(physics,EMR)
http://en.wikipedia.org/wiki/Absorption_(electromagnetic_radiation)

Referenced by:
Absolute Magnitude (M)
Absorption Coefficient
Absorption Line
Atomic Excitation
Bremsstrahlung
Methylidyne (CH)
Compton Scattering
Continuous Absorption
Cosmic Dust
Distance Modulus (u)
Earthshine
Emission
Emission Line
Extinction
Gunn-Peterson Trough
HITEMP
HITRAN
Kramers' Opacity Law
Line Broadening
Optical Depth (τ)
Oscillator Strength
Oxygen Lines
Photochemistry
Photoionization
Radiative Transfer (RT)
Radiative Transfer Code (RT Code)
Equation of Radiative Transfer (RTE)
Radiative Transfer Model (RTM)
Source Function (S)
Spectral Band
Spectral Line
State of Excitation
Transmission Spectroscopy
Water Lines

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