Riccardo Rigon
IlSole,F.Lelong,2008,ValdiSella
Solar Radiation
Long wave radiation
R. Rigon
2
Or is used for photosynthesis
or other chemical reactions
Spectral response
R. Rigon
3
Earth “is” a gray body
Having a temperature emits radiation
A.Adams-Partofthesnakeriverpicture
Long wave radiation
R. Rigon
Gray Bodies
• Plank’s Law for gray bodies:
• The Stefan-Boltzmann equation for gray bodies:
W = ✏
2⇡c2
h 5
e
ch
KT 1
[Wcm 2
µm 1
]
W = ✏ T4
[Wcm 2
]
4
where ε is the average emissivity calculated over the entire electromagnetic
spectrum.
Long wave radiation
R. Rigon
Gray Bodies
The behavior of a real (gray) body is related to that of a black body by
means of the quantity ελ, known as the emission coefficient or
emissivity, which is defined as:
Kirchhoff (1860) demonstrated that a good “radiator” is also a good
“absorber”, that is to say:
✏ =
W (real body)
W (black body)
↵ = ✏ ⇢ + ⌧ + ✏ = 1
5
Long wave radiation
R. Rigon
Comparison of blackbody and gray body
6
In reality emissivity depends, at least, on wavelength. Earth should be
probably defined a selective radiator
Long wave radiation
R. Rigon
See the Earth as gray body
a n d g i v e n t h a t t h e
temperature of the Earth’s
surface is, on average,
about 288 K, it obviously
e m i t s a s p e c t r u m o f
radiation in the infrared
band.
7
Long wave radiation
R. Rigon
Radiation emitted by the Sun and the Earth
Yochanan Kushnir
8
Long wave radiation
R. Rigon
See the Earth as gray body
a n d g i v e n t h a t t h e
temperature of the Earth’s
surface is, on average,
about 288 K, it obviously
e m i t s a s p e c t r u m o f
radiation in the infrared
band.
A t m o s p h e r e i s n o t
anymore transparent to at
these wavelengths.
9
Long wave radiation
R. Rigon
The atmosphere is
warmed from below
Therefore the temperature is
higher at ground level than it
is at higher altitudes.
10
Long wave radiation
R. Rigon
Greenhouse Effect
In the absence of atmospheric absorption the average temperature of the Earth’s
surface would be about -170C.
11
Long wave radiation
R. Rigon
Instead the average temperature is about 15 0C
Greenhouse Effect
12
Long wave radiation
R. Rigon
Radiative heating
is completed by convective heat transfer, and by water vapor fluxes (latent and
sensible heat).
13But this you can see better on the energy budget slides.
Long wave radiation
R. Rigon
But now concentrate on the surroundings of a point
14
AfterHelbig,2009
Any point being at a certain temperature emits long wave radiation
which must be accounted for
Long wave radiation
R. Rigon
15
The atmosphere emits infrared itself
bacause of its temperature
Long wave radiation
R. Rigon
Long-wave radiation is given by the
balance of incident radiation from
the atmosphere and the radiation
emitted by the ground. Both values
are calculated with the Stefan-
Boltzmann law.
16
All the contributions
Long wave radiation
R. Rigon
Longwave radiation
coming from
surrounding
Radiation losses
by the area under
exam
Longwave radiation
coming from sky
Longwave (infrared) radiation
Topographic effects: angle of view
17
Long wave radiation
R. Rigon
Long-wave radiation
The first component should be
calculated by integrating the formula
over the entire atmosphere, but,
given how complex this process is,
typically an empirical formula is
used that uses the value of air
temperature as measured near
ground level (2m) and a value of the
atmospheric emissivity based on
specific humidity, temperature, and
cloudiness. The second component,
on the other hand, is function of the
s u r f a c e t e m p e r a t u r e a n d i t s
emissivity.
18
R. Rigon
The real process:
The hydrological parameterisation:
Long-wave radiation
19
Long wave radiation
Global emissivity of the
atmosphere
Temperature at 2 m
from ground
R. Rigon
The hydrological parameterisation:
εatm = εBrutsaert (1− N6
) + 0.979N4
Brutsaert (1975) + Pirazzini et al. (2000)
εatm = εBrutsaert (1+ 0.26N)
εatm = εIdso(1− N6
) + 0.979N4
εatm = εIdso,corr (1− N6
) + 0.979N4
Brutsaert (1975) + Jacobs (1978)
Idso (1981) + Pirazzini et al. (2000)
Hodges et al. (1983) + Pirazzini et al.
(2000)
Parameterisation of Long-wave radiation
20
Long wave radiation
where N is the fraction of sky covered by clouds
R. Rigon
21
Net Radiation
The sum of longwave and shortwave ratio
is called net radiation
R. Rigon
22
1Thank you for your attention !
G.Ulrici-2000?

6 i-longwave radiation

  • 1.
  • 2.
    R. Rigon 2 Or isused for photosynthesis or other chemical reactions Spectral response
  • 3.
    R. Rigon 3 Earth “is”a gray body Having a temperature emits radiation A.Adams-Partofthesnakeriverpicture Long wave radiation
  • 4.
    R. Rigon Gray Bodies •Plank’s Law for gray bodies: • The Stefan-Boltzmann equation for gray bodies: W = ✏ 2⇡c2 h 5 e ch KT 1 [Wcm 2 µm 1 ] W = ✏ T4 [Wcm 2 ] 4 where ε is the average emissivity calculated over the entire electromagnetic spectrum. Long wave radiation
  • 5.
    R. Rigon Gray Bodies Thebehavior of a real (gray) body is related to that of a black body by means of the quantity ελ, known as the emission coefficient or emissivity, which is defined as: Kirchhoff (1860) demonstrated that a good “radiator” is also a good “absorber”, that is to say: ✏ = W (real body) W (black body) ↵ = ✏ ⇢ + ⌧ + ✏ = 1 5 Long wave radiation
  • 6.
    R. Rigon Comparison ofblackbody and gray body 6 In reality emissivity depends, at least, on wavelength. Earth should be probably defined a selective radiator Long wave radiation
  • 7.
    R. Rigon See theEarth as gray body a n d g i v e n t h a t t h e temperature of the Earth’s surface is, on average, about 288 K, it obviously e m i t s a s p e c t r u m o f radiation in the infrared band. 7 Long wave radiation
  • 8.
    R. Rigon Radiation emittedby the Sun and the Earth Yochanan Kushnir 8 Long wave radiation
  • 9.
    R. Rigon See theEarth as gray body a n d g i v e n t h a t t h e temperature of the Earth’s surface is, on average, about 288 K, it obviously e m i t s a s p e c t r u m o f radiation in the infrared band. A t m o s p h e r e i s n o t anymore transparent to at these wavelengths. 9 Long wave radiation
  • 10.
    R. Rigon The atmosphereis warmed from below Therefore the temperature is higher at ground level than it is at higher altitudes. 10 Long wave radiation
  • 11.
    R. Rigon Greenhouse Effect Inthe absence of atmospheric absorption the average temperature of the Earth’s surface would be about -170C. 11 Long wave radiation
  • 12.
    R. Rigon Instead theaverage temperature is about 15 0C Greenhouse Effect 12 Long wave radiation
  • 13.
    R. Rigon Radiative heating iscompleted by convective heat transfer, and by water vapor fluxes (latent and sensible heat). 13But this you can see better on the energy budget slides. Long wave radiation
  • 14.
    R. Rigon But nowconcentrate on the surroundings of a point 14 AfterHelbig,2009 Any point being at a certain temperature emits long wave radiation which must be accounted for Long wave radiation
  • 15.
    R. Rigon 15 The atmosphereemits infrared itself bacause of its temperature Long wave radiation
  • 16.
    R. Rigon Long-wave radiationis given by the balance of incident radiation from the atmosphere and the radiation emitted by the ground. Both values are calculated with the Stefan- Boltzmann law. 16 All the contributions Long wave radiation
  • 17.
    R. Rigon Longwave radiation comingfrom surrounding Radiation losses by the area under exam Longwave radiation coming from sky Longwave (infrared) radiation Topographic effects: angle of view 17 Long wave radiation
  • 18.
    R. Rigon Long-wave radiation Thefirst component should be calculated by integrating the formula over the entire atmosphere, but, given how complex this process is, typically an empirical formula is used that uses the value of air temperature as measured near ground level (2m) and a value of the atmospheric emissivity based on specific humidity, temperature, and cloudiness. The second component, on the other hand, is function of the s u r f a c e t e m p e r a t u r e a n d i t s emissivity. 18
  • 19.
    R. Rigon The realprocess: The hydrological parameterisation: Long-wave radiation 19 Long wave radiation Global emissivity of the atmosphere Temperature at 2 m from ground
  • 20.
    R. Rigon The hydrologicalparameterisation: εatm = εBrutsaert (1− N6 ) + 0.979N4 Brutsaert (1975) + Pirazzini et al. (2000) εatm = εBrutsaert (1+ 0.26N) εatm = εIdso(1− N6 ) + 0.979N4 εatm = εIdso,corr (1− N6 ) + 0.979N4 Brutsaert (1975) + Jacobs (1978) Idso (1981) + Pirazzini et al. (2000) Hodges et al. (1983) + Pirazzini et al. (2000) Parameterisation of Long-wave radiation 20 Long wave radiation where N is the fraction of sky covered by clouds
  • 21.
    R. Rigon 21 Net Radiation Thesum of longwave and shortwave ratio is called net radiation
  • 22.
    R. Rigon 22 1Thank youfor your attention ! G.Ulrici-2000?