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Principles of Radiometry and Photometry  273


              Source                Illumination, footcandles

           Direct sunlight              10,000
           Open shade                   1,000
           Overcast/dark day            10–100
           Twilight                     0.1–1.0
           Full moon                    0.01
           Starlight                    0.0001
           Dark night                   0.00001
                              (a)

              Material                  Reflectance

           Asphalt                      0.05
           Trees, grass                 0.20
           Red brick                    0.35
           Concrete                     0.40
           Snow                         0.85
           Aluminum building            0.65
           Glass window wall            0.70
           Parking lot with cars        0.40

                              (b)
        Figure 12.9 (a) Illumination levels produced by sources in
        nature. (b) Reflectance of a number of exteriors.





        special usages, and many such terms have survived. A tabulation of
        photometric units is given in Fig. 12.10.
          Photometric calculations may be carried out exactly as are radio-
        metric calculations, using the relationships presented in Secs. 12.2
        through 12.6. If lumens are substituted for watts in all the expres-
        sions, the computations are straightforward. When the starting and
        final data must be expressed in the special terminology of photometry
        (as opposed to what one might term the rational units of lumens,
        steradians, and square centimeters), then conversion factors may be
        necessary for each relationship. A very simple way of avoiding this dif-
        ficulty is to convert the starting data to lumens, steradians, and square
        centimeters, complete the calculation, and then convert the results into
        the desired units.
          For convenience, the basic relationships are repeated here in both
        radiometric (left column) and photometric (right column) form:
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