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Error analysis and corrections to pupil diameter measurements with Langley Research Center's oculometerFactors that can affect oculometer measurements of pupil diameter are: horizontal (azimuth) and vertical (elevation) viewing angle of the pilot; refraction of the eye and cornea; changes in distance of eye to camera; illumination intensity of light on the eye; and counting sensitivity of scan lines used to measure diameter, and output voltage. To estimate the accuracy of the measurements, an artificial eye was designed and a series of runs performed with the oculometer system. When refraction effects are included, results show that pupil diameter is a parabolic function of the azimuth angle similar to the cosine function predicted by theory: this error can be accounted for by using a correction equation, reducing the error from 6% to 1.5% of the actual diameter. Elevation angle and illumination effects were found to be negligible. The effects of counting sensitivity and output voltage can be calculated directly from system documentation. The overall accuracy of the unmodified system is about 6%. After correcting for the azimuth angle errors, the overall accuracy is approximately 2%.
Document ID
19800018576
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Fulton, C. L.
(Purdue Univ. Hampton, VA, United States)
Harris, R. L., Jr.
(NASA Langley Research Center)
Date Acquired
September 4, 2013
Publication Date
May 1, 1980
Subject Category
Aerospace Medicine
Report/Patent Number
NASA-TM-81806
Report Number: NASA-TM-81806
Accession Number
80N27075
Funding Number(s)
PROJECT: RTOP 505-35-23-01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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