Kippzonen BSRN Scientific Solar Monitoring System Manual do Utilizador Página 142

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Figure C 4.2. Relationship between the geometry of
pyrheliometers and radiance (The relationship
applies for a diffusometer when the sun is at zenith).
C 4.2 Irradiance in the instrument: Numerical
solutions
Since the relationship between the radiation
and the sensor continuously changes with
the solar zenith angle, exact com parability
happens only when the sun is at zenith. This
rare occasion nevertheless is useful to
develop the general case for which most
measurements are carried out.
C 4.3 Sun at zenith
The geometrical condition between radiance
and an instrument is illustrated in Figure C
4.2 for the sun at zenith. The same figure
represents both pyrheliometers and
diffusometers by swiching the frontal circle
between the opening and the shading disc
(or sphere). We consider a point on the
sensor which is located at a distance of r'
measured from the sensor centre. Radiance
at this point falls at a zenith angle of z'. We
r'
consider total irradiance F at this point
coming into the instrument (or blocked by the
shading disc). This calculation involves a
double integration, one from the normal to
the sensor to the edge of the opening (or disc)
whose angle to the normal is z, the other from
0º to 360º in azimuth:
where
r'
This irradiance F expected at r' on the sensor must be integrated for the entire sensor surface to
obtain the absolute amount of radiative flux (or the amount blocked by the shading disc):
where r = the radius of the sensor.
This radiative flux can be converted for a unit area to obtain the irradiance expressed in the
conventional unit.
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