| Literature DB >> 32331923 |
Patricia M Cisarik1, Lindsey Brise2, Greyson Ramos2.
Abstract
PURPOSE: Detection of anisocoria in those with dark irides is difficult, and failure to detect anisocoria can have dire consequences. Whether infrared pupillometry and gross measurement would yield different prevalence rates for anisocoria in those with dark irides is unknown. We compared the frequency of anisocoria in healthy adults with dark irides assessed with mm ruler versus infrared pupillometry.Entities:
Keywords: Anisocoria; Fotografía de Infrarrojos; Infrared photography; Pupillometry; Pupilometría
Year: 2020 PMID: 32331923 PMCID: PMC7520532 DOI: 10.1016/j.optom.2020.03.003
Source DB: PubMed Journal: J Optom ISSN: 1989-1342
Figure 1Ruler used for gross assessment of pupil size. The numbers adjacent to the black “half moons” indicate the pupil diameter in millimeters. Pupils of size determined to be between two of the “half moons” were assigned a size half way between the two. For example, if the pupil size was between that of number 4 and number 5, the size was assigned a value of 4.5 mm.
Figure 2Custom-build infrared light source used for digital pupillometry (Shazly et al.). The top photo was taken in normal room light with the infrared LEDs turned off. The bottom photo was taken with room lights off and the infrared LEDs turned on.
Figure 3The frequency of anisocoria ≥0.5 mm is plotted for two lighting conditions and two measurement techniques. For statistical comparisons, see text.
Analysis of cross-categorized frequencies of anisocoria.
| Conditions compared | Odds ratio | 0.95 confidence interval for odds ratio | Fisher's exact probability test, 2-tailed |
|---|---|---|---|
| Photo light vs. Ruler light | .2356 | .0467, 1.1884 | .084 |
| Photo dark vs. Ruler dark | NA | NA | .005 |
| Ruler light vs. Ruler dark | NA | NA | .496 |
| Photo light vs. Photo dark | 1 | .3253, 3.074 | 1.0 |
Comparison of observed frequencies of anisocoria with previously reported rates.
| Test condition | Expected proportion | Observed proportion | Cumulative probability of finding the same or fewer number of observed cases |
|---|---|---|---|
| Ruler, Light | 0.034 | 0.429 | |
| 0.057 | |||
| 0.15 | 0.004 | ||
| 0.20 | 0.0002 | ||
| Photo, Light | 0.05 | 0.130 | 0.99 |
| 0.707 | |||
| 0.427 | |||
| 0.13 | |||
| Ruler, Dark | 0 | 0.052 | |
| 0.10 | 0.002 | ||
| 0.15 | <0.0001 | ||
| 0.20 | <0.0001 | ||
| Photo, Dark | 0.05 | 0.135 | 0.986 |
| 0.856 | |||
| 0.472 | |||
| 0.157 | |||
Expected proportions highlighted in bold are those for which the observed proportions were NOT significantly different. See text for details.