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Title: Todays lecture objectives:


1
ATMS 455 Physical Meteorology
  • Todays lecture objectives
  • Absorptivity and emissivity (WH 6.5)
  • Building the foundation for understanding the
    greenhouse effect

http//www.artcyclopedia.com/feature-2001-08.html
2
ATMS 455 Physical Meteorology
  • Todays lecture topics
  • Absorptivity and emissivity (WH 6.5)
  • Kirchhoffs law
  • Selective absorbers and emitters
  • Disposition of monochromatic radiation

3
Introduction
  • Blackbody radiation upper limit to the amount
    of radiation that a real substance may emit at a
    given temperature

4
Introduction
  • emissivity a measure of how strongly a body
    radiates at a particular wavelength. A blackbody
    has an emissivity equal to one.

http//ceos.cnes.fr8100/cdrom-97/ceos1/science/ba
phygb/chap3/chap3.htm
5
Introduction
  • If we neglect the dependence of emissivity on the
    wavelength (color) of radiation, we define a
    gray body emissivity

6
Introduction
  • We also define the quantities absorptivity (al)
    and gray body absorptivity (a) which are measures
    of the ratio of the irradiance absorbed by a
    particular body to that which is incident upon
    it. The absorptivity of a blackbody is equal to
    one at all wavelengths of radiation.

7
Kirchhoffs law
  • Proof of Kirchhoffs law
  • Two parallel plates, infinite in extent
  • Blackbody plate on left
  • Gray body plate on right with absorptivity (a)
    and emissivity (e)
  • Plates are in radiative and thermal equilibrium

8
Kirchhoffs law
  • In qualitative terms
  • Materials which are strong absorbers at a
    particular wavelength are also strong emitters at
    that wavelength
  • Materials which are weak absorbers at a
    particular wavelength are also weak emitters at
    that wavelength

? The validity of Kirchhoffs law is not
dependent upon whether a body is in thermal and
radiative equilibrium
? Applies for atmospheric gases up to altitudes
of 60km
9
Selective absorbers and emitters
  • In the moon example (Prob. 6.6, p. 292), the
    radiative equilibrium temperature of the gray
    surface is independent of the absorptivity
  • When absorptivity is a function of wavelength of
    radiation, the situation for radiative
    equilibrium temperature can be quite different ?
    Prob. 6.7, p. 293

10
Selective absorbers and emitters
  • Snow is a relatively weak absorber at visible and
    near-IR wavelengths, but is a strong absorber in
    the IR wavelengths

http//news.bbc.co.uk/1/hi/england/2639171.stm
11
Selective absorbers and emitters
  • How does a selectively absorbing gas behave? ?
    Prob. 6.8, p. 293

http//www.eballoon.org/pictures/alpine.html
12
Selective absorbers and emitters
  • Calculate the radiative equilibrium temperature
    of the earths surface
  • Atmosphere is a thin layer with a 0.1 for solar
    radiation and a 0.8 for terrestrial radiation
  • Earths surface behaves as a blackbody

13
Selective absorbers and emitters
  • Iterative method for solving Prob. 6.8, p. 293
  • Atmosphere is a thin layer with a 0.1 for solar
    radiation and a 0.8 for terrestrial radiation

14
Selective absorbers and emitters
  • Compare the surface temperatures for an earth
    system
  • Without an atmosphere (Prob. 6.5), Te 255 K
  • With an atmosphere (Prob. 6.8), Te 286 K

15
Selective absorbers and emitters
  • Whenever a gas that is a weak absorber in the
    visible and a strong absorber in the IR is a
    constituent of a planetary atmosphere, it
    contributes toward raising the surface
    temperature of the planet (greenhouse effect)
  • In order to satisfy radiation balance, the
    surface must compensate by emitting more
    radiation than it would in the absence of such an
    atmosphere (must radiate at a higher temperature)

16
Disposition of monochromatic radiation
  • incident upon an opaque (non-transparent)
    surface

17
Disposition of monochromatic radiation
  • Strong reflectors are weak absorbers (e.g. snow
    at visible wavelengths)
  • Weak reflectors are strong absorbers (e.g.
    asphalt at visible wavelengths)

18
Disposition of monochromatic radiation
  • Shortwave reflectivity of various surfaces

Petty 2004
19
Disposition of monochromatic radiation
  • incident upon a non-opaque (semi-transparent)
    layer

http//www.worldstar.com/collmer/
20
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