Intro to Light & Vision Lecture 4 Jonathan Pillow Sensation - - PowerPoint PPT Presentation

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Intro to Light & Vision Lecture 4 Jonathan Pillow Sensation - - PowerPoint PPT Presentation

Intro to Light & Vision Lecture 4 Jonathan Pillow Sensation & Perception (PSY 345 / NEU 325) Princeton University, Spring 2015 1 (Chapter 1 leftovers) 2 Figure 1.16 Detecting a stimulus using the signal detection theory (SDT)


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SLIDE 1

Intro to Light & Vision

Lecture 4 Jonathan Pillow Sensation & Perception (PSY 345 / NEU 325) Princeton University, Spring 2015

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SLIDE 2

(Chapter 1 leftovers)

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Figure 1.16 Detecting a stimulus using the signal detection theory (SDT) approach (Part 2)

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SLIDE 4

d-prime - measure of sensitivity

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SLIDE 5

Figure 1.18 For a fixed dʹ″, all you can do is change the pattern of your errors by shifting the response criterion

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Signal Detection Theory Terms to know: “noise” distribution: values arising when stimulus not present “signal” distribution: values arising when signal + noise present Type I error: rate of “false alarms”, or false positives Type II error: rate of “misses”, or false negatives psychometric function: describes probability of saying “I heard it” as function of stimulus intensity

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Summary

  • Weber-Fechner law
  • Stevens’ power law
  • psychophysics
  • psychometric function
  • signal detection theory: threshold, criterion, Hit/

Miss, FA/CR, d’ = d-prime

  • brain regions, spikes, synapses, neurotransmitter

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SLIDE 8

Chapter 2:

First steps in Vision

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SLIDE 9
  • Light: A wave; a stream of photons, tiny particles

that each consist of one quantum of energy

Light: electromagnetic radiation within a narrow energy range

  • a wave: can be bent by lenses
  • a particle: “photons” - can travel through a vacuum, have

minimum energy that can be emitted/absorbed (quanta)

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SLIDE 10

Food for thought: Why are we sensitive to such a narrow range of the electromagnetic spectrum?

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Food for thought: Why are we sensitive to such a narrow range of the electromagnetic spectrum? Other solutions are possible:

  • bees: ultraviolet light
  • pit vipers: infrared light

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Light Physics What it all looks like. (Messy!)

  • each point in space has light from all angles passing through it

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  • without optics, light from

everything hits the whole retina/screen/film

  • with optics, we form an

image

  • i.e. light from a single point

in space hits a single spot

  • n the retina

Why do we need optics?

image pinhole camera

  • bject

screen

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Pinhole camera: problem of pinhole size

smaller aperture = fewer rays = sharper image = dimmer image

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Some pinhole images

big pinhole small pinhole tiny pinhole why?

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diffraction

slit = 1 x wavelength slit = 5 x wavelength

  • bending of waves around small obstacles or through small apertures

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SLIDE 17

diffraction

slit = 1 x wavelength slit = 5 x wavelength

  • bending of waves around small obstacles or through small apertures

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SLIDE 18

the eye (viewed from above)

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  • Cornea: The transparent “window” into the eyeball

(carries 2/3 of eye’s total refractive power)

  • Aqueous humor: watery fluid in behind cornea
  • Lens: allows changing of focus
  • Pupil: The dark circular opening at the center of the iris

in the eye, where light enters the eye

  • Vitreous humor: transparent fluid that fills main

cavity of the eye (gel-like; may contain “floaters”)

  • Retina: light-sensitive membrane in the back of the eye

that contains rods and cones.

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  • photic sneeze reflex

tendency to sneeze when walking from a dark room into bright light topic of debate:

  • Aristotle - “sun heats the nose.”
  • Bacon - closed eyes and didn’t sneeze!
  • current thinking: “crossed wiring”

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SLIDE 21

Image formation with a lens

Goal is to focus the light rays emanating from a single point to a single point on the imaging surface

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SLIDE 22

lenses

converging diverging

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Refraction: necessary to focus light rays, carried out by lens

  • Accommodation: process in which the lens changes

its shape, altering its refractive power

  • Emmetropia: no refractive error

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Figure 2.3 Optics of the human eye

  • too fat / powerful
  • eye is too long
  • too thin / not enough

accommodation

  • eye is too short

(near-sightedness) (far-sightedness)

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SLIDE 25

far away

  • bject

near

  • bject

Good Good

normal eye - accomodation

(courtesy ben backus)

min max

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SLIDE 26

far away

  • bject

near

  • bject

Good Good

normal eye - accomodation

(courtesy ben backus)

min max

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myopic (near-sighted) eye

far away

  • bject

near

  • bject

Good

min max

  • lens too powerful

can’t get far

  • bjects in

focus

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SLIDE 28

myopic (near-sighted) eye

far away

  • bject

near

  • bject

Good

min max

  • lens too powerful

can’t get far

  • bjects in

focus

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SLIDE 29

hyperopic (farsighted) eye

far away

  • bject

near

  • bject

Good

min max

  • lens not powerful enough

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hyperopic (farsighted) eye

far away

  • bject

near

  • bject

Good

min max

can’t get near

  • bjects in

focus

  • lens not powerful enough

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  • if you have an astigmatism, some lines will have lower contrast
  • Astigmatism: visual defect caused by the unequal

curving of one or more of the refractive surfaces of the eye, usually the cornea

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Camera analogy for the eye

  • Aperture (F-stop) = Iris/pupil. Regulates

the amount of light coming into the eye

  • Focus = Lens.

Changes shape to change focus

  • Film = Retina.

Records the image

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Summary

  • light, electromagnetic spectrum, visible spectrum
  • light as a wave / particle
  • pinhole cameras, lenses, image formation, blur,

diffraction, optics of the eye

  • anatomy of the eye (cornea, pupil, iris, aqueous, cilliary

muscle, lens, vitreous, fovea, retina, and who could forget the Zonules of Zinn!)

  • accommodation, emmetropia, refractive errors

(hyperopia, myopia, astigmatism)

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