Title: Todays lecture objectives:
1ATMS 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
2ATMS 455 Physical Meteorology
- Todays lecture topics
- Absorptivity and emissivity (WH 6.5)
- Kirchhoffs law
- Selective absorbers and emitters
- Disposition of monochromatic radiation
3Introduction
- Blackbody radiation upper limit to the amount
of radiation that a real substance may emit at a
given temperature
4Introduction
- 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
5Introduction
- If we neglect the dependence of emissivity on the
wavelength (color) of radiation, we define a
gray body emissivity
6Introduction
- 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.
7Kirchhoffs 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
8Kirchhoffs 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
9Selective 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
10Selective 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
11Selective absorbers and emitters
- How does a selectively absorbing gas behave? ?
Prob. 6.8, p. 293
http//www.eballoon.org/pictures/alpine.html
12Selective 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
13Selective 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
14Selective 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
15Selective 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)
16Disposition of monochromatic radiation
- incident upon an opaque (non-transparent)
surface
17Disposition 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)
18Disposition of monochromatic radiation
- Shortwave reflectivity of various surfaces
Petty 2004
19Disposition of monochromatic radiation
- incident upon a non-opaque (semi-transparent)
layer
http//www.worldstar.com/collmer/
20(No Transcript)