Page 215 - Algae
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198                                   Algae: Anatomy, Biochemistry, and Biotechnology


                                   Typical Values for Illuminance        (in lux)

                                   Sunlight                             100,000
                                   Skylight                              10,000
                                   Overcast daylight                      1,000
                                   Moonlight                                 0.1
                                   Starlight                                 0.01




                  LUMINANCE
                  Luminance is a photometrically weighted radiance. In terms of visual perception, we perceive lumi-
                  nance. It is an approximate measure of how “bright” a surface appears when we view it from a given
                  direction. Luminance used to be called “photometric brightness.” Luminance is measured in
                  lumens per square meter per steradian (lm m 22  sr 21 ).


                  LAMBERTIAN SURFACES
                  A Lambertian surface is referred to as a perfectly diffusing surface, which adheres to Lambert’s
                  cosine law. This law states that the reflected or transmitted luminous intensity in any direction
                  from an element of a Lambertian surface varies as the cosine of the angle between that direction
                  and the normal of the surface. The intensity I u of each ray leaving the surface at an angle u from
                  the ray in a direction perpendicular to the surface (I n ) is given by:

                                                    I u ¼ I n   cos u                       (5:22)

                     Therefore, even if the luminous intensity decreases with a factor cos(u) from the normal, the
                  projected surface decreases with the same factor; as a consequence, the radiance (luminance) of
                  a Lambertian surface is the same regardless of the viewing angle and is given by:

                                                    dI n   cos u  dI n
                                                 L ¼         ¼                              (5:23)
                                                     dA   cos u  dA
                     It is worthwhile to note that in a Lambertian surface the ratio between the radiant exitance and
                  the radiance is p and not 2p:

                                                      M
                                                         ¼ p                                (5:24)
                                                       L

                     This equation can be easily derived. Suppose we place an infinitesimal Lambertian emitter dA
                  on the inside surface of an imaginary sphere S. The inverse square law [Equation (5.15)] provides
                  the irradiance E at any point P on the inside surface of the sphere. However, d ¼ D   cos u, where D
                  is the diameter of the sphere. Thus:

                                                          I u
                                                   E ¼                                      (5:25)
                                                         2
                                                       D   cos u
                  and from Lambert’s cosine law [Equation (5.22)], we have:
                                                          I n
                                                      E ¼                                   (5:26)
                                                          D 2
                  which simply says that the irradiance (radiant flux density) of any point P on the inside surface of S
                  is a constant.
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