| Literature DB >> 30538662 |
Manuel Spitschan1, Tom Woelders2.
Abstract
The human pupillary light response is driven by all classes of photoreceptors in the human eye-the three classes of cones, the rods, and the intrinsically photosensitive retinal ganglion cells (ipRGCs) expressing the photopigment melanopsin. These photoreceptor classes have distinct but overlapping spectral tuning, and even a monochromatic light with a wavelength matched to the peak spectral sensitivity of a given photoreceptor will stimulate all photoreceptors. The method of silent substitution uses pairs of lights ("metamers") to selectively stimulate a given class of photoreceptors while keeping the activation of all others constant. In this primer, we describe the method of silent substitution and provide an overview of studies that have used it to examine inputs to the human pupillary light response.Entities:
Keywords: color vision; ipRGC (intrinsically photosensitive retinal ganglion cell); melanopsin; metamers; pupil; pupillometry; silent substitution
Year: 2018 PMID: 30538662 PMCID: PMC6277556 DOI: 10.3389/fneur.2018.00941
Source DB: PubMed Journal: Front Neurol ISSN: 1664-2295 Impact factor: 4.003
Figure 1(A) Overlapping spectral sensitivities of the human photoreceptors. (B) Non-specificity of single-wavelength lights. Right panel: Pattern of photoreceptor responses to the single-wavelength light at 490 nm. (C) Principle of univariance. Right panel: Pattern of photoreceptor responses to the single-wavelength lights E1, E2, and E3 designed to elicit the same response in melanopsin. (D) Wavelength exchange between two short-wavelength lights E1 and E2 which stimulate S cones at the same level but yield different photoreceptor responses for melanopsin. Right panel: Pattern of excitations for lights E1 and E2.
Figure 2(A) Background spectrum (left panel) to which the observer is light-adapted, eliciting a pattern of responses in the photoreceptors (right panel). (B) Increase in emitted light near the melanopsin peak relative to the background spectrum (left panel; dashed line = background spectrum, red line = modulation spectrum) leads to an increase in the excitation of all photoreceptors (middle panel), or equivalently, positive contrast on the photoreceptors (right panel). (C) To balance the excitation of the S cones, a decrease in emitted short-wavelength light (left panel) leads to silencing of the S cones (middle panel), or equivalently, zero contrast on the S cones (right panel). (D) To balance the excitation of the L and M cones, a decrease in emitted medium-wavelength light (left panel) leads to a reduction in L and M cone activity (middle panel) but not yet zero contrast on the L and M cones (right panel); indeed, the contrast seen by the L and M cones is now negative. (E) To silence the excitation of the L and M cones, a decrease in emitted long-wavelength light (left panel) leads to balancing of the L and M cones (middle panel), or equivalently, zero contrast on the L and M cones (right panel). The contrast seen by melanopsin is 50%. (F) The modulation spectrum shown in (E) yields positive contrast relative to the background spectrum but the spectrum can also be “mirrored” around the background spectrum, thereby leading to a negative modulation of melanopsin (and rods).
Studies examining human pupil responses with silent substitution.
| Tsujimura et al. ( | 4 | 470, 500, 525, 615 nm ± 20–36 nm | Diffusing screen in front of integrating sphere | 20° field size | Melanopsin [−53%] | 301 cd/m2 to 642 cd/m2 to 982 cd/m2 | 6 | 10 min stimuli | Cones: CIEPO2006 |
| Viénot et al. ( | 5 | 473 ± 25 nm | Light booth with white paint | Ganzfeld | Melanopsin-only (cone and rod silent) [3.4%] | 35 cd/m2 | 10 | Measurement after 1 min of continuous exposure | Cones: CIEPO2006 |
| Tsijumura and Tokuda, ( | 4 | 468, 524, 599, and 633 nm (test) | Diffusing screen in front of integrating sphere | Annulus id 5 od 18° | 8% | 612 cd/m2 background1,109 cd/m2 test field | 6 | Sinusoidal & square wave stimuli | Cones: CIEPO2006, 10° |
| Spitschan et al. ( | 128 | n/a | Viewing of surface through lens | 27.5° circular, central 5° blocked | S, (L+M), melanopsin, (L+M+melanopsin) [50%] | 382–1,033 cd/m2 | 16 | Sinusoidal, 0.01 – 2 Hz | 10° Stockman–Sharpe/CIE cone fundamentals, melanopsin estimated by shifting Stockman-Sharpe nomogram to λmax = 480 nm, corrected for prereceptoral filtering (same as cones, optical density 0.3). |
| Barrionuevo et al. ( | 4 | 442, 516, 594, and 634 nm (one set) | Ganzfeld | 54° field | Mixed joint modulations, no melanopsin-isolaing modulation | 0.002–100 cd/m2 | 3 (authors) | Sinusoidal, 0.5–8 Hz | Smith–Pokorny cone fundamentals |
| Cao et al. ( | 5 | 456, 488, 540, 592, 633 | Maxwellian view | 30° circular, central 10.5° blocked | Experiment 1: S, M, L, Rod, Melanopsin [16%] | Experiment 1: 200 Photopic Td | 3 | Sinusoidal, 1 Hz | Smith–Pokorny cone fundamentals applied for the CIE 1964 10° Standard Observer |
| Barrionuevo and Cao, ( | 5 | 456, 488, 540, 592, 633 | Maxwellian view | 30° circular, central 10.5° blocked | Experiment 1: S, M, L, Rods, Melanopsin, (L+M+S) [17%], red-green [4% M,−4% L] | 2–20,000 Photopic Td | 3 (2 authors) | Sinusoidal, 1 Hz | Smith–Pokorny cone fundamentals applied for the CIE 1964 10° Standard Observer |
| Spitschan et al. ( | 56 | n/a | Viewing of surface through lens | 64° circular, central 5° blocked | 25–400% | 100–200 cd/m2 | 4 | Tapered pulses (3 s, 14–16 s ISI) | CIE 2006 parametric model |
| Woelders et al. ( | 5 | 465, 500, 515, 595 | Diffusing screen in front of LEDs | 24.68° horizontal, 12.13° vertical | S, M, L, Melanopsin [23%] | Background or average of 8.5 melanopic lux | 16 | Square-wave (0.25–4 Hz) | α-opic lux (Lucas et al.): Govardovski nomograms, λmax from Dartnall, optical densities 0.3, 0.38, 0.38 (S, M, L) |
| Murray et al. ( | 4 | 460, 524, 590, 635 | Ganzfeld | Central 7° of surface covered with disk of no reflective black material. | L, M, (L+M+S) [11% Weber] | 17 cd/m2 | 5 | Square-wave (1 s increment/ | Stockman Sharpe cone fundamentals |
| Zele et al. ( | 5 | 456, 488, 540, 592, 633 | Maxwellian view | 30° circular, central 10.5° blocked | Color:[7%, 22% or 24% Weber] | 2,000 photopic Td (detection thresholds and pupil) | 4 (2 authors) | Pupil: 1 Hz sinusoidal | Smith–Pokorny cone fundamentals applied for the CIE 1964 108 Standard Observer CIE 1951 scotopic luminosity function Enezi et al. melanopsin function |