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Scattering

Scattering. Extinction: scattering + absorption Types of scattering: Single vs. multiple Conservative vs. non-conservative Elastic vs. inelastic (e.g., Raman) This lecture discusses three aspects of scattering: How much radiation is affected? Is there absorption too?

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Scattering

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  1. Scattering • Extinction: scattering + absorption • Types of scattering: • Single vs. multiple • Conservative vs. non-conservative • Elastic vs. inelastic (e.g., Raman) • This lecture discusses three aspects of scattering: • How much radiation is affected? • Is there absorption too? • Into which direction does the scattered radiation go?

  2. Question 1: How much radiation is affected? • Equation of radiative transfer: , where d=dz • Rearranging this gives: • Scattering coefficient () given by: • r = particle radius, n = number of particles • Q = scattering efficiency • Q depends on size parameter (x), given by •  = wavelength • How come Q > 1 ?

  3. Lord Rayleigh John William Strutt (third Baron Rayleigh) 1842-1919 Essex, Cambridge Nobel Prize in Physics in 1904 "for his investigations of the densities of the most important gases and for his discovery of argon in connection with these studies" Scattering by clear air Air molecules scatter light as dipoles Dipole induced

  4. Scattering • Two types of scattering are considered – molecular scattering (Rayleigh) and scattering from aerosols (Mie) • The equation for Rayleigh scattering can be written as • Where α is the polarizability

  5. Scattering by clear air 2 We know that In clean air, r remains constant, but  of interest may vary Consequences: (next slide) Which part of Q(x) curve applies? • ≈ 0.2 in blue • ≈ 0.03 in red Easy-to-calculate formulas available (will have code)

  6. Rayleigh scattering • Sky appears blue at noon, red at sunrise and sunset - why?

  7. Phase diagram for Rayleigh scattering

  8. Scattering by clear air 4 Red sky in the morning, sailors take warning. Red sky at night, sailors delight. Morning Evening

  9. Mie-Debye scattering • For particles which are not small compared with the wavelength one has to deal with multiple waves from different molecules/atoms within the particle • Forward moving waves tend to be in phase and this gives a large resultant amplitude. • Backward waves tend to be out of phase and this results in a small resultant amplitude • Hence the scattering phase function for a particle has a much larger forward component (forward peak) than the backward component

  10. Phase diagrams for aerosols

  11. Scattering by aerosol MODIS product Aerosol size (indicates composition)  is Angstrom exponent  ≈ 1.2 typical

  12. Aerosol size determination from space Visible Near-infrared Fine particles from smoke Coarse dust particles Fine particles from smoke

  13. Blue Moon May happen after volcanic eruptions, very rare

  14. Question 2: Is there absorption too? c speed of light H magnetic field E electric field  permittivity µ permeability (=1 for non-ferromagnetic materials) Maxwell’s equations Instead of r, i, we use mr and mi • Refractive index: m = mr + i mi • Imaginary part (mi): • If only absorption is considered: •  = absorption coefficient;  = density; s = path, k = absorption coefficient) • The value of mi depends on how easy it is to bounce • electrons to higher energy levels so that they don’t fall back. • Usually: small values + sharp peaks at a few wavelengths • (though learned about widening of absorption spectra) • Exception: metals: large  values (Why?) Meaning of real part later

  15. Single scattering albedo (a) • What portion of influenced radiation is scattered? (The rest is absorbed.) • Upper bound: 1.0 (why?) • Lower bound for large particles: 0.5 (why?) • Typical values for droplets at visible wavelengths: just below 1.0 • Some aerosols contain mix of water and carbon -> lower values • Wavelength-dependence of a: why decrease with size?

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