Multipole-Based
CSF Estimates Predict Crack Detection Individual Differences
Albert
J. Ahumada and
Bettina L. Beard
NASA Ames Research Center
http://vision.arc.nasa.gov/personnel/al/ahumada.html
Introduction: For an airframe crack detection project (Beard, Jones, Chacon, and
Ahumada, 2005), we wanted to
measure the contrast sensitivity functions (CSFs) of the inspectors. We wanted
to use the same equipment, so we wanted to use stimuli that did not require
special techniques to present the threshold stimuli, so we decided against
windowed gratings. Klein (1989) had proposed using multi-pole stimuli to
estimate CSFs. Line segments (monopoles) are similar to the cracks that the
inspectors were asked to detect in airframe images. Figure 1 shows an airframe
crack image; Figure 2 shows the multipole experiment stimuli.
Figure
1. Example airframe crack detection images: (above or left) image with crack,
(below or right) image with crack removed.
Method: For our Sony Trinitron CRT
gamma function, it was possible to choose a line width (0.5 arc min) length (8
arc min), and duration (0.25 sec) such that below-threshold lines were easily
presented. Dipoles and quadapoles
require matching positive and negative levels, a condition not met exactly, but
the unwanted line components were well below threshold. Thresholds were estimated for 9 observers.
Figure
2. Multipole experiment images: square, line, dipole, and quadrapole.
Results: Two parameters were
estimated for each observer, the overall sensitivity factor and the
Difference-of-Gaussian CSF center frequency cutoff. These same two parameters were estimated for each observer using
contrast thresholds from crack detection in actual airframe images. There was agreement among the two sets of
parameters (Figures 3a and 3b, but there was a strong correlation between the
two crack detection parameters (Figure 3c), suggesting a single variable was
the source of the individual differences.


Question: For the Modelfest (2001)
data, what happens when you estimate the observer CSFs, from the multipole-like
stimuli separately and also estimate them from the fixed-width Gabors?
Methods: For each of the 16 observer,
the difference-of-Gaussian CSF center spread was estimated for three subsets of
the images:
1.The 10 fixed-width Gabors (Figure 4).
2.Seven non-periodic images: 4 Gaussian blobs and a
Gaussian-windowed edge, line, and dipole (Figure 5).
3.The line and the dipole.
Figure 4.
The first 7 of the 10 fixed-width Gabors
(the higher frequencies aliased badly).
Figure
5. Modelfest images 26-32, four sizes of Gaussian blobs and Gaussian-windowed
edge, line, and dipole.
Results: The median DoG CSF center
standard deviations in arc min for the 10 fixed-width Gabors were clustered
close to 1.5 min. The estimates based
on the 7 non-periodic images (26-32) were more spread out and had a larger
median (Figure 6a). The estimates based
on the line and the dipole (31, 32) were also larger (Figure 6b), suggesting
that the mediating variable is not simply spatial uncertainty.
Conclusions:
Within the context of visible contrast energy based CSF
estimation, multipoles with higher spatial frequency content are not as visible
as one would expect from the Gabor-derived CSFs.
Individual differences in multipole-derived CSFs seem likely
to be strongly affected by variables other than CSF shape.
References
Ahumada
& Beard (1998) A simple vision model for inhomogeneous image quality
assessment, SID Digest 29, 641-644.
Beard,
Jones, Chacon, and Ahumada (2005) Detection of blurred cracks: A step towards
an empirical vision standard, Final Report for FAA Agreement DTFA-2045.
Klein (1989) Visual multipoles and the assessment of visual
sensitivity to displayed images, SPIE Proc. 1077, 83-92.
ModelFest (2001) http://vision.arc.nasa.gov/modelfest/
Watson
& Ahumada (2005) A standard model for foveal detection of spatial contrast, Journal of Vision
(accepted).
Acknowledgement: Support provided by NASA
Aerospace Systems and the FAA.