Download presentation

Presentation is loading. Please wait.

Published byCameron Nixon Modified over 2 years ago

1
LIGHT AND THE RETINAL IMAGE: KEY POINTS Light travels in (more or less) straight lines: the pinhole camera’s inverted image Enlarging the pinhole leads to BLUR How a lens prevents blur: refraction reunites light rays by bending them Point-to-point projection from object to inverted image Refraction: which way is light bent? Slowing in glass: lifeguard analogy. The eye: retina, lens and cornea; fovea, periphery and blind spot Focus errors; distant vision and near vision Myopia, hypermetropria, emmetropia, accommodation; emmetropization Visual angle and image size: (in radians) = size/distance (in degrees) = (180/ ) * size/distance (minutes of arc) = 60 * (180/ ) * size/distance Point spread function: width is 1 minute in visual angle, or 5 microns (.005 mm) Sources of light spread making the image imperfect: focus error; chromatic aberration; other aberrations; diffraction Direct observation of the image: Helmholtz’s ophthalmoscope Quality of the image: spread is about 5 microns (1 minute of arc) Visual resolution limit: about 1 minute of arc or 30 cpd (for 20/20 vision) Can vision be perfected?? William’s magic mirror and laser surgery Aliasing through sampling by the photoreceptor mosaic: Nyquist limit (60cpd)

3
A Review of Optics Austin Roorda, Ph.D. University of Houston College of Optometry

4
(Most of) these slides were prepared by Austin Roorda, (UC Berkeley Optometry School) and used by permission.

5
Geometrical Optics Relationships between pupil size, refractive error and blur

6
Optics of the eye: Depth of Focus 2 mm4 mm6 mm

7
2 mm4 mm6 mm In focus Focused in front of retina Focused behind retina Optics of the eye: Depth of Focus

8
7 mm pupil Bigger blur circle Courtesy of RA Applegate

9
Smaller blur circle 2 mm pupil Courtesy of RA Applegate

10
Demonstration Role of Pupil Size and Defocus on Retinal Blur Draw a cross like this one on a page, hold it so close that is it completely out of focus, then squint. You should see the horizontal line become clear. The line becomes clear because you have made you have used your eyelids to make your effective pupil size smaller, thereby reducing the blur due to defocus on the retina image. Only the horizontal line appears clear because you have only reduced the blur in the horizontal direction.

11
Physical Optics The Wavefront

12
What is the Wavefront? converging beam = spherical wavefront parallel beam = plane wavefront

13
What is the Wavefront? ideal wavefront parallel beam = plane wavefront defocused wavefront

14
What is the Wavefront? parallel beam = plane wavefront aberrated beam = irregular wavefront ideal wavefront

15
What is the Wavefront? aberrated beam = irregular wavefront diverging beam = spherical wavefront ideal wavefront

16
The Wave Aberration

17
What is the Wave Aberration? diverging beam = spherical wavefront wave aberration

18
Wave Aberration of a Surface

19
Diffraction

20
Diffraction “Any deviation of light rays from a rectilinear path which cannot be interpreted as reflection or refraction” Sommerfeld, ~ 1894

21
Diffraction and Interference diffraction causes light to bend perpendicular to the direction of the diffracting edge interference due to the size of the aperture causes the diffracted light to have peaks and valleys

22
rectangular aperture square aperture

23
Airy Disc circular aperture

24
The Point Spread Function

25
The Point Spread Function, or PSF, is the image that an optical system forms of a point source. The point source is the most fundamental object, and forms the basis for any complex object. The PSF is analogous to the Impulse Response Function in electronics.

26
Airy Disc The Point Spread Function The PSF for a perfect optical system is the Airy disc, which is the Fraunhofer diffraction pattern for a circular pupil.

27
Airy Disk

28
0 0.5 1 1.5 2 2.5 12345678 pupil diameter (mm) separatrion between Airy disk peak and 1 st min (minutes of arc 500 nm light) As the pupil size gets larger, the Airy disc gets smaller.

29
Point Spread Function vs. Pupil Size 1 mm2 mm3 mm4 mm 5 mm6 mm7 mm

31
Small Pupil Little spreading due to defocus or aberrations So diffraction is limiting

32
Larger pupil: Less diffraction (not shown) But more blur and more aberrations

34
Aberrations

36
1 mm2 mm3 mm4 mm 5 mm6 mm7 mm Point Spread Function vs. Pupil Size Perfect Eye (Diffraction Limited)

37
pupil images followed by psfs for changing pupil size 1 mm2 mm3 mm4 mm 5 mm6 mm7 mm Point Spread Function vs. Pupil Size Typical Eye with aberrations

38
Demonstration Observe Your Own Point Spread Function

39
Resolution

40
Rayleigh resolution limit Unresolved point sources Resolved

41
Keck telescope: (10 m reflector) About 4500 times better than the eye! “Pupil” is 10M: almost no diffraction Wainscott

42
Compound eye: Each facet must be large to fight diffraction Many facets (pixels) needed to capture details

43
Convolution with the PSF

44
Convolution

45
Simulated Images 20/40 letters 20/20 letters

46
MTF Modulation Transfer Function

47
low mediumhigh object: 100% contrast image spatial frequency contrast 1 0

48
The modulation transfer function (MTF) indicates the ability of an optical system to reproduce (transfer) various levels of detail (spatial frequencies) from the object to the image. Its units are the ratio of image contrast over the object contrast as a function of spatial frequency. It is the optical contribution to the contrast sensitivity function (CSF).

49
MTF: Cutoff Frequency 0 0.5 1 050100150200250300 1 mm 2 mm 4 mm 6 mm 8 mm modulation transfer spatial frequency (c/deg) cut-off frequency Rule of thumb: cutoff frequency increases by ~30 c/d for each mm increase in pupil size

50
Effect of Defocus on the MTF Charman and Jennings, 1976 450 nm 650 nm

51
Relationships Between Wave Aberration, PSF and MTF

52
Retinal Sampling

53
Projected Image Sampled Image 5 arc minutes 20/20 letter Sampling by Foveal Cones

54
5 arc minutes 20/5 letter Projected Image Sampled Image Sampling by Foveal Cones

55
Nyquist Sampling Theorem

56
Photoreceptor Sampling >> Spatial Frequency I 0 1 I 0 1 nearly 100% transmitted

57
I 0 1 I 0 1 Photoreceptor Sampling = 2 x Spatial Frequency

58
I 0 1 I 0 1 nothing transmitted Photoreceptor Sampling = Spatial Frequency

59
Nyquist theorem: The maximum spatial frequency that can be detected is equal to ½ of the sampling frequency. foveal cone spacing ~ 120 samples/deg maximum spatial frequency: 60 cycles/deg (20/10 or 6/3 acuity)

Similar presentations

OK

Ch 25 1 Chapter 25 Optical Instruments © 2006, B.J. Lieb Some figures electronically reproduced by permission of Pearson Education, Inc., Upper Saddle.

Ch 25 1 Chapter 25 Optical Instruments © 2006, B.J. Lieb Some figures electronically reproduced by permission of Pearson Education, Inc., Upper Saddle.

© 2017 SlidePlayer.com Inc.

All rights reserved.

Ads by Google

Ppt on gujarati culture family Ppt on bank lending interest Ppt on difference between mission and vision Ppt on law against child marriage statistics Ppt on mind reading computer free download Free ppt on degrees of comparison Ppt on obesity diet children Ppt on environmental degradation in india Ppt on area of trapezium Ppt on film industry bollywood songs