Jump to content

User:SigmaJargon/math5110

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by SigmaJargon (talk | contribs) at 17:13, 11 December 2009. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Before anything else, let's go over a little about the eye, and how the pupil and iris work.

The pupil is an aperature in the middle of the iris that controls light entering the retina. In response to light (or the absense of light) on the pupil, the iris may expand or contract, allowing more more or less light into the pupil. This is very important, since if too much light enters the retina, it may be damaged, but if too little enters, it may not be able to form a good image.

The size of the human pupil ranges from 3 to 4 millimeters when fully contracted, and widens to 5 to 9 millimeters when fully dilated (1). The standard unit of illuminance used for measuring light hitting the human eye is the lux, which is analogous to watts per square meter, but weighted by wavelength to fit a standardized model of brightness perception. About 50 lux is the brightness in a family living room, 320-500 lux is office lighting, 10,000-25,000 lux is ambiant daylight, and direct sunlight is at least 32,000 lux (2).

Let's start with light actually entering the pupil. The intensity of light entering the pupil

For a given illuminance I (in lux), the amount of light L (in lumens) actually entering a pupil of radius P (in meters) would be

Now, how does a pupil contract or expand when exposed to a certain amount of light? There is some threshold value for light entering the eye. Too far above this value and the amount of light is painful or damaging, but too far below it is insufficiently bright to properly see. The further from this threshold, the faster the eye will want to dilate or contract. Further, the eye will want to contract more slowly if it is already strongly contracted, and dilate more slowly if it is already strongly dilated. Let's say our maximum pupil size is and our minimum pupil size is . Then, for a certain threshold t (in lumens), we can make a simple model:

This is somewhat simpler than reality. For example, eyes actually contract about three times faster than they dilate (3), and I am presuming that change on rate from all of these factors is linear.

A quick few notes on this model. k is a constant, a scaling factor that can be adjusted to model pupils that dilate more or less speedily. and are always positive, so the behavior (in terms of increasing or decreasing) is based solely upon the factor. If L is larger than t (that is to say, the expirienced illumination is greater than the threshold), then the eye will contract - if L is smaller than t, the eye will dilate. If the light is very dim (small I), then the term will diminish to zero as the eye dilates - if the light is dim enough, this term will go to zero before the term, indicating that the area is too dark to see in with the human eye. Likewise, with a sufficiently bright area (large I), the might diminish to zero before the term, indicating that the area is too bright.

Now we come to the fun bit. If I is fixed, it is easy to plot the above model on a time plane and find fixed points. However, in the problem we are given, I is not fixed. If P is large, it dilates so that it covers an additional light source, a small beam of light. For simplicity's sake, we'll treat this like a point, and have it communicate a certain number of lumens directly.

1. http://en.wikipedia.org/wiki/Pupil

2. http://en.wikipedia.org/wiki/Lux

3. Ellis, C. J. (1981). "The pupillary light reflex in normal subjects". British Journal of Ophthalmology 65 (11): pp. 754-759.