Intensity Profile of Lambert's Scatterer

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The intensity profile of a Lambertian scatterer shows that light intensity decreases with the viewing angle, yet the surface appears uniformly bright from any angle. This phenomenon occurs because the intensity of scattered light is proportional to the cosine of the angle between the incident light and the surface normal. As the surface tilts, the change in projected area offsets the decrease in intensity, resulting in a consistent brightness perception. This explains why objects like the moon and printer paper maintain a flat appearance regardless of the viewer's position. Understanding this relationship clarifies the visual consistency of Lambertian surfaces.
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I wish to understand the intensity profile of a lambertian scatterer.
how can a surface look the same when viewed from any angle, when its intensity profile shows that the intensity decreases with the viewing angle?
 
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A lambertian surface has the property that the intensity of scattered light varies linearly with the cosine of the angle between incidence and reflection.

Because this dependence is the same as the geometrical change of a surface element as it is tilted with respect to the line of sight (i.e. the projected area), the two terms cancel and the surface appears to have a constant brightness. Thus, the moon appears flat, and a piece of printer paper likewise appears to have constant brightness without regard to viewing angle.
 
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