
The position of the Sun was found by determining the upper, lower, left and right bounds of the image of the Sun. The grey scale of the clips were "stretched" to make the grid lines and the Sun easier to see.

The grid coordinates of the Sun's image were used to find the Sun's altitude and azimuth as a function of the time. The height of the lens aperature was found by measurement to be 24.8 inches. A check against my longitude turned out to be worse than expected being almost 1 degree off. I set the wrist watch to UT just before starting the observations. Time was measured to the second so its precision was about 1 part in 3600. The μ coordinates were rather flat and so its errors were probably more significant. They may have thrown off the time of the peak slightly.
Supplemental (28 Jun 2011): The "platform" I used was warped being shaped somewhat like an inverted bowl. I noticed some curvature when leveling the platfrorm with a spirit level and tried to compensate for it. This is probably the major source of the error in the observed latitude and longitude since the measurements are relative to the platform and its grid system.
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