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Fig. 2.25 Comparison between
measured long-wave
radiation R lds under
various sky conditions
and radiation R ld
estimated by means of
Equations (2.80) and
(2.82) with a = 0 . 0496
and b = 2 . 45 and with
cloudiness values from
visual sky inspection.
(From Sugita and
Brutsaert, 1993.)
R ld (W m 2 )
the Great Plains by expressing a as an empirical sinusoidal function of month of the
year.
The downward long-wave radiation is affected by cloudiness. Several empirical
methods of incorporating this effect (see Bolz, 1949; Budyko, 1974) can be expressed
in the form
R ldc 1
am c
R ld =
+
(2.82)
where m c is the fractional cloudiness and a and b are (different) constants. On the
basis of measurements in Germany, Bolz (1949) obtained b
=
2 and different values
of a depending on cloud type, with an average of a
0.22. More recently, with visual
cloudiness observations in the Great Plains, Sugita and Brutsaert (1993) derived values
a
=
=
=
2.45, without consideration of cloud type, and different values of
a and b for different cloud types. Their analysis also showed that the standard error
of prediction with Equation (2.80) was of the order of 10-15 W m 2 for clear sky
conditions and of the order of 20-25 W m 2 for various sky (including cloudy) conditions
without cloudiness correction; incorporation of a cloudiness correction with (2.82) and
these constants improved the R ld estimate with (2.80), i.e. reduced the standard error,
by roughly5Wm 2 on average (see Figure 2.25), and by an additional amount of
roughly the same magnitude when also information was included on the type of cloud.
Deardorff (1978) proposed a simple weighting parameterization, namely an atmospheric
emissivity for cloudy sky given by
0.0496 and b
ε a =
[ m c +
(1
m c )
ε ac ]; this is equivalent to (2.82)
with a
=
[(1
ac )
1] and b
=
1.
 
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