Lecture 23, 24 - Wavefront abberations of the eye Flashcards

1
Q

Main factors affecting quality of retinal image:

A

• Diffraction
• Defocus
• Aberrations
• Scatter

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2
Q

What are aberrations?

A

• Important as they reduce the retinal image quality of the eye and therefore reduce visual acuity
• During subjective refraction optometrists are correcting a combination of defocus and aberrations. However they are unable to correct aberrations completely with spherical and astigmatic lenses.

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3
Q

What are the two types of abberations:

A

• Chromatic
• Monochromatic

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4
Q

Define Ray and Wavefront

A

• Ray
Lines normal to the wavefront at every point on the intersection
• Wavefront
A surface over which an optical disturbance has a constant phase

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5
Q

Chromatic aberrations cause:

A

• Results from the fact that the refractive index of materials change with the wavelength of light

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6
Q

Chromatic aberration

A

• The velocity of light in a medium (hence the refractive index) varies with its wavelength.
• Thus the image of a source of white light (consisting of a wide range of wavelengths) is extended along the optical axis.
• The refractive index of blue light is higher than red light, making a lens more powerful when blue light is travelling through it

Short wavelengths come to focus before longer wavelengths

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7
Q

Two types of chromatic abberation

A

• Longitudinal
- describes the fact that the blue image will be formed in front of the red

• Transverse
- describes the lateral displacement of the red and blue light

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8
Q

Chromatic aberration cause

A

• Results from the fact that the refractive index of materials change with the wavelength of light

• Result: Coloured fringes around objects

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9
Q

Chromatic aberration: How much?

A

More than 1.5 dioptres from one extreme of the visible spectrum to the other.

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10
Q

Chromatic aberration: Why don’t we notice coloured fringes?

A

• The eye is much less sensitive to wavelengths towards the ends of the spectrum - fringes will be relatively dim
• ? Neural filtering, lens filtering
• CA may cause some image degradation but correcting it is impractical

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11
Q

Monochromatic aberrations cause:

A

• Paraxial rays are rays that are near the axis
• Therefore the sine of the angle and the angle expressed in radians is very similar
• However the eye is not a paraxial optical system and a more accurate relationship is needed to define the aberrations

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12
Q

Five monochromatic aberrations are:

A

• Spherical Aberration
• Coma
• Oblique Astigmatism
• Curvature
• Distortion

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13
Q

Contour plots:

A

• The wavefront aberration or error is the distance between the actual and reference wavefronts as a function of position in the pupil
• This is typically shown as a contour map
• The contours join points in the exit pupil where the wavefront aberration has the same value
• Closely packed contours suggest large amounts of aberration and a poor image
• No contour = ideal non aberrated system

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14
Q

Spherical aberration:

A

• Rays entering through the periphery of the pupil are refracted more than the paraxial rays
• Only monochromatic aberration which occurs when both the object and image points lie on the optical axis of a centred system
• In the eye positive SA occurs when marginal rays intersect the optical axis in front of the paraxial rays
• Positive SA is commonly found in the eye

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15
Q

Spherical aberration cause:

A

This causes some “blurring” of the image

Spherical aberration in the eye is only about 0.6D for a 5mm pupil as a result of:

• Aspherical cornea
• Refractive index gradient of the crystalline lens

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16
Q

How is spherical aberrations reduced?

A

• The effects of spherical aberration are further reduced by the Stiles-Crawford effect
• Light entering through the centre of the pupil is more likely to be absorbed by a photoreceptor than light entering through the periphery

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17
Q

The Stiles-Crawford effect:

A

• Cones act like waveguides (see pic)
• Cones are “aimed” at the centre of the pupil - less likely to absorb light coming from the periphery of the pupil

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18
Q

Describe “Coma” aberration

A

• Occurs only for off-axis object points in a centred optical system
• Produces a characteristic comet shaped image
• The tail of the comet points towards the optical axis in negative coma (away in positive)
• The length of the tail increases as the object and image points go further off axis

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19
Q

Results from Coma

A

• Results from the displacement of rays passing through different parts of the annulus
• Rays travelling through peripheral parts of the lens form a ring image that is displaced in comparison to the paraxial image
• Ring images get larger as the radius increases

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20
Q

Coma affects depending on axis?

A

• As an off-axis aberration coma would not be expected to influence foveal visual performance to any great extent
• But the eye is not perfectly centred and therefore coma can occur along the visual axis of some individuals

21
Q

Oblique astigmatism:

A

• Arises from off-axis object points
• Caused by differences in the refractive power in the saggital and tangential planes of an optical system

22
Q

Field curvature:

A

• Arises because the in-focus image of an optical system does not usually lie on a plane
• It usually lie on a curve (the Petzyal surface)
• Further from the lens axis in the object plane (eg B) the distance from the object to the first principal point of the lens increases
• Image distance also gets shorter in +ve lenses and in the eye
• The wavefront aberration for any image point corresponds to a simple shift in focus to give a circular wavefront contour
• Field curvature is compensated to some extent in the eye as the retina is also curved

23
Q

Distortion:

A

• Results from differences in magnification with variations in the distance from the optical axis
• Pincushion= magnification increases with distance from axis
• Barrel= magnification decreases with distance from axis
• For any image point a lateral displacement corresponds to a simple tilt of a flat wavefront
• results in a wavefront map that show equispaced straight line contours parallel to the saggital section and a tilted isometric view
• Not usually considered to be a problem in the eye (visual system can adapt to this)

24
Q

Terminology used to assess optical quality

A

• Point spread function (PSF)
• Modulation transfer function (MTF)
• Phase transfer function (PTF)
• Optical transfer function (OTF)

25
Q

Point spread function:

A

• Is the light distribution in the image of a point at or close to the paraxial image plane
• This distribution depends on both the level of aberration in the beam and diffraction (both are dependent upon the wavelength of light)
• General Rule: the smaller the PSF width the better the image quality
• Line spread function is similar but is a line instead of a point

26
Q

Point spread function: with pupil diameter

A

• In the case of diffraction: the PS decreases in width with an increase in size of the pupil
• But the PSF will increase in diameter with increasing pupil size due to aberrations
• Therefore there is an optimum pupil width where the PS is minimum (2-6mm)
• The shape and size of the PSF will vary with the type of aberrations present

27
Q

Modulation transfer function (MTF)

A

• MT is related to the PSF
• Describes the loss of contrast suffered when an image is cast of a sinusoidal grating object
• The ratio of image contrast to object contrast captures the blurring effects of optical imperfections
• The variation of this ratio with spatial frequency and orientation of the grating object is called the MTF

28
Q

Methods of measuring abberations:

A

• A number of methods have been employed since the 19th century to measure aberrations
• We will discuss four of the most common methods

• Examples include
- Tscherning Aberroscope
- Hartmann shack wavefront sensor
- Ray tracing
- Retinoscopy principle

29
Q

Tscherning abberoscope

A

• A grid of laser spots is used to form an image on the retina
• The grid travels through the optics of the eye and the end point image will be distorted due to the aberrations
• The deviation of each spot from its perfect position is measured and processed to give the wavefront aberration

30
Q

Hartmann shack wavefront sensor:

A

• Currently the most popular method

• Unlike aberroscope and ray tracing techniques in that it is essentially a ray trace from a retinal point out of the eye

• a narrow beam from a laser is imaged by the eye and the light passed back from the fundus travels through a wavefront sensor consisting of many microlenses (lenslets) to the CCD camera

• These lenslets focus the rays into spots which define the wavefront pattern

• The amount that the lenslet image is displaced from the ideal image position indicates the level of aberration

31
Q

Principles of the Shack-Hartmann Wavefront sensor:

A

• The local slope (or the first derivative) of the wavefront is determined at each lenslet location

• The corresponding wavefront is determined by a least squares fitting of the slopes to the derivative of a polynomial selected to fit the wavefront

• Zernike polynomial is the most commonly used

32
Q

Retinoscopy Principle

A

• An infra-red slit scans through the pupil measuring the refractive power of the eye
• The wavefront is calculated by determining the changes in refractive power across the area of the pupil

33
Q

What are Zernike polynomials

A

• set of basic shapes that are used to fit the wavefront
• analogous to the parabolic x2 shape that can be used to fit 2D data

34
Q

How bad is the eye? Static abberations

A

• For the most part, aberrations in the eye are random. When you average enough eyes together, most terms are no different from zero. The only high order aberrations that is non-zero is spherical aberration, which averages to a small positive value.
• Overall, the eye’s high order aberrations reduce with pupil size. The dashed line indicates the effective diffraction limit, according to Marachel’s criterion.

35
Q

What can change wave aberrations in the eye?

A

• Dynamic Changes in the wave aberrations are caused by
- accommodation
- eye movement
- eye translation
- tear film

36
Q

Clinical instruments to measure aberration:

A

• Tscherning based: Allegretto (Wavelight laser)
•Hartmann Shack: Zywave (Bausch and Lomb)
•Ray Tracing; Tracey (Tracey technologies)
• Retinoscopy: OPD/ARK-1000 (Nidek)

37
Q

Differences in measurements of instruments caused by…

A

• Comparison between instruments has revealed a poor level of agreement between higher order aberration measures

Could be due to differences in
•accommodation control
• Method of measurement
•Differences in the maths

38
Q

Why measure abberations?

A

• Imaging the internal eye structures
• Analysis and correction of visual performance

39
Q

Analysis and correction of visual performance:

A

• Aberrations can reduce the visual performance of the eye
• Correction of aberrations will therefore have the potential to improve visual performance
• Refractive surgery, intraocular lenses and contact have all been developed to try to correct aberrations

40
Q

Intra-ocular lenses

A

• IOLs are implanted as a replacement to the crystalline lens following cataract surgery
• They can potentially produce high levels of wavefront aberration (especially SA)
• This again creates problems such as reduced visual performance especially at night
• Measurement of wavefront aberrations prior to surgery will help in the development and design of IOLs that reduce wavefront aberration levels

41
Q

Contact lenses:

A

• Contact lenses produce reasonably predictable wavefront aberrations
• Visual performance can be improved when lens design is modified to reduce wavefront aberration
• Disadvantage of contact lenses is that they are likely to rotate on the eye
• The rotation can limit the accuracy of the wavefront correction
• Contact lenses do have the advantage of being reversible and easily modified

42
Q

Can we create supernormal vision using adaptive optics?

A

• Contrast sensitivity has already been shown to be enhanced 6 fold
• Visual acuity limits have been increased from 6/4 to 6/2
• The retinal image of a point object is 8 times brighter when corrected
• The theoretical limit on image quality for the eye equals an acuity of ~ 6/1

43
Q

• Basic science imaging applications
• Pre-clinical applications

A

Basic science imaging applications
- reveal properties of single cells in living eyes
- correlate properties of cellular structure in living eyes with visual performance
- nonlinear imaging of structure and function

Pre-clinical applications
- faciliate longitudinal tests on animal models
- test outcomes of drugs and treatments for eye disease
- correlate phenotypes with genotypes

44
Q

• Clinical imaging applications

A
  • provide early diagnosis for retinal or other systemic diseases
  • better understand the etiology of retinal disease for which little is known
  • discover more sensitive biomarkers for retinal disease
  • track progression of eye disease
  • measure response at cellular level to therapies that treat disease
  • preselect patients or diseases that may benefit best from therapies or treatments
45
Q

Functional imaging applications

A
  • facilitate better relationships between structure and function
  • reveal properties of cell networks in living eyes (ie retinal circuitry)
46
Q

• Vision applications
• Dynamic applications

A

• Vision applications
Vision Applications
- pre-test the benefits of aberration correction on vision develop optimal aberration profiles for long depth of focus test possible signals that drive accommodation and/or eye growth
- reveal the optical retinal and neural limits of human vision
• Dynamic applications
- measure properties of blood flow in small capillaries
- measure scattering changes in response ot light stimulation
- measure eye motion with high accuracy and frequency

47
Q

• Light delivery applications

A
  • track and stimulate single cells or networks of cells for electrophysiology expts
  • microperimetry
  • targeted laser treatment (photocoagulation, or uncaging drugs)
  • track eye movement responses to stimulation
  • study role of eye movements for vision
48
Q

Imaging the internal eye structures

A

• Taking account of the ocular aberrations allows clinical instruments to gain better resolution when examining the internal structures of the eye
• This ability to compensate for optical aberrations has an important role in research and in the early detection of various ocular pathologies