scholarly journals Enhancing the dark side: Asymmetric gain of cone photoreceptors underpins their discrimination of visual scenes based on their skewness

2021 ◽  
Author(s):  
Matthew Yedutenko ◽  
Marcus H.C. Howlett ◽  
Maarten Kamermans
2021 ◽  
Author(s):  
Matthew Yedutenko ◽  
Marcus H.C. Howlett ◽  
Maarten Kamermans

Psychophysical data indicates humans can discriminate visual scenes based on their skewness - the ratio of dark and bright patches within a visual scene. It was also shown that on a phenomenological level this skew discrimination is described by the so-called Blackshot mechanism, which accentuates strong negative contrasts within a scene. Here we demonstrate that the neuronal correlate of the Blackshot mechanism is the asymmetric gain of the cone phototransduction cascade, which is higher for strong negative contrasts than for strong positive contrasts. We recorded from goldfish cone photoreceptors and found that the asymmetry in the phototransduction gain leads to higher amplitude of the responses to negatively than to positively skewed light stimuli. This asymmetry in the amplitude was present in the photocurrent, voltage response and cone synaptic output. Additionally, we found that stimulus skewness leads to a subtle change in photoreceptor kinetics. For negatively skewed stimuli, the cone's impulse response functions peak later than for positively skewed stimulus. However, stimulus skewness does not affect the cone's overall integration time.


Author(s):  
P.M. Rice ◽  
MJ. Kim ◽  
R.W. Carpenter

Extrinsic gettering of Cu on near-surface dislocations in Si has been the topic of recent investigation. It was shown that the Cu precipitated hetergeneously on dislocations as Cu silicide along with voids, and also with a secondary planar precipitate of unknown composition. Here we report the results of investigations of the sense of the strain fields about the large (~100 nm) silicide precipitates, and further analysis of the small (~10-20 nm) planar precipitates.Numerous dark field images were analyzed in accordance with Ashby and Brown's criteria for determining the sense of the strain fields about precipitates. While the situation is complicated by the presence of dislocations and secondary precipitates, micrographs like those shown in Fig. 1(a) and 1(b) tend to show anomalously wide strain fields with the dark side on the side of negative g, indicating the strain fields about the silicide precipitates are vacancy in nature. This is in conflict with information reported on the η'' phase (the Cu silicide phase presumed to precipitate within the bulk) whose interstitial strain field is considered responsible for the interstitial Si atoms which cause the bounding dislocation to expand during star colony growth.


2006 ◽  
Vol 40 (12) ◽  
pp. 30
Author(s):  
BARBARA J. HOWARD
Keyword(s):  

2008 ◽  
Author(s):  
Ivelina N. Naydenova ◽  
Warren H. Jones
Keyword(s):  

2008 ◽  
Author(s):  
Amanda Poole ◽  
Julie Carswell ◽  
Rhys Lewis ◽  
Deborah Powell ◽  
Bernd Marcus

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