Optics III: Advanced imaging techniques

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Last updated 5:34 AM on 8/5/26
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39 Terms

1
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Lateral resolution (∆x)

  • Ability to resolve structure across the retina

  • Limited by PSF size or airy disk size

    • Pupil size → Diffraction + Aberrations

<ul><li><p>Ability to resolve structure across the retina</p></li><li><p>Limited by PSF size or airy disk size</p><ul><li><p>Pupil size → Diffraction + Aberrations</p></li></ul></li></ul><p></p>
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Axial resolution (∆z)

  • Resolve structure along the Z-axis (In and out) of the retina

    • Depth

  • Limited by the imaging method used

<ul><li><p>Resolve structure along the Z-axis <sub>(In and out)</sub> of the retina</p><ul><li><p>Depth</p></li></ul></li><li><p>Limited by the imaging method used</p></li></ul><p></p>
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What size lateral and axial resolution is best?

  • Low (∆z) and low (∆x)

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How to determine lateral resolution in diffraction-limited system

Rayleigh criterion

  • f → Focal length (mm)

  • D → Aperture diameter

<p><em>Rayleigh criterion</em></p><ul><li><p>f → Focal length (mm)</p></li><li><p>D → Aperture diameter</p></li></ul><p></p>
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Rayleigh criterion states…

  • Two point sources can be identified if they are separated by the radius of their airy disks

<ul><li><p>Two point sources can be identified if <u>they are separated by the radius of their airy disks</u></p></li></ul><p></p>
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For 550 nm light, what is the optimal pupil diameter for rayleigh criterion?

Assume: 22mm focal length

∆x = 1.22 * f * λ / D AND Foveal cones are 2.5 microns

  • The optimal pupil size is 6mm (Image)

    • Without aberrations

<p><span style="background-color: transparent;"><em>∆x = 1.22 * f * λ / D </em><strong><em><u>AND </u></em></strong></span><em>Foveal cones are 2.5 microns</em></p><ul><li><p>The optimal pupil size is 6mm <sub>(Image)</sub> </p><ul><li><p>Without aberrations</p></li></ul></li></ul><p></p>
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Imaging cones

  • Refers to individual foveal cones being used as a benchmark for imaging

  • Foveal cone size = 2.5 microns or 0.5 arc mins

  • Requirements

    • 6mm pupil

    • Diffraction-limited system (Rayleigh criterion)

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Requirements to resolve one “cycle”

One black-white pair needs to fall on two adjacent cones

  • ∆x of…

    • 5 microns

    • 1 min arc

    • 60 CPD

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Is it easier imaging cones in the periphery or fovea?

Peripheral cones!

Why?

  • They get bigger as you move away from the fovea

    • Time to reclass bro

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Absorption of macular pigment

  • 400nm to 550nm light

    • Peak near 458nm

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Absorption of melanin in the RPE and choroid

  • Absorption ↓ as wavelength ↑

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Absorption patterns of retinal vasculature

  • Blood absorbs between 400 and 450nm light

  • Light between 520nm and 590nm is dependent on oxygenation of hemoglobin

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Is foveal or parafoveal reflectance greater?

Parafoveal reflectance

  • Foveal cones have more short wavelength-absorbing pigment

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What wavelengths are used for retinal imaging? Why?

700 to 900 nm (Near infrared)

  • Not absorbed by retinal structures

  • Less visible to subject → Less photophobia

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Things that will fuck up retinal imaging

  • Accommodation

  • Tear film between blinks

  • Fixational eye movements

  • Patient becomes uncomfortable → Moves around

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Adaptive optics (AO) systems

Compensates for fluctuations in accommodation and tear film changes during retinal imaging

  • Continuously monitors quality of retinal image

  • Adjusts according to changes in accommodation/tear film

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Fixational eye movements

Factor degrading retinal imaging quality

  • Displace image up to 10 microns

  • Solution

    • Short imaging exposure

      • <10 msec

    • Eye tracking recordings

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Confocal scanning laser ophthalmoscope (cSLO)

Problem: Each retinal layer scatters light differently → Image quality degraded

cSLO solution

  • Excludes scattered light from every layer except the one of interest

    • Via a pin-hole that only allows reflected light from the desired layer

<p>Problem: Each retinal layer scatters light differently → Image quality degraded</p><p>cSLO solution</p><ul><li><p>Excludes scattered light from every layer <u>except</u> the one of interest</p><ul><li><p>Via a pin-hole that only allows reflected light from the desired layer</p></li></ul></li></ul><p></p>
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cSLO is used in the diagnosis of…

  • Glaucoma

  • Macular degeneration

  • Retinal disorders

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How exactly does a cSLO work?

  • Horizontal and vertical scanning mirrors move laser over the retina (Raster scan)

    • Uses reflected intensity from each spot to form the image

  • Pinhole used to only focus the reflected light from the plane you want to image at (Image)

    • Confocal = The desired layer is in line with the pinhole

<ul><li><p>Horizontal and vertical <u>scanning mirrors</u> move laser over the retina <sub>(Raster scan)</sub></p><ul><li><p>Uses reflected intensity from each spot to form the image</p></li></ul></li><li><p>Pinhole used to only focus the reflected light from the plane you want to image at <sub>(Image)</sub> </p><ul><li><p>Confocal = The desired layer is in line with the pinhole</p></li></ul></li></ul><p></p>
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Optical sectioning

  • Changing the layer of the retina that us confocal with the cSLO pinhole allows high resolution image of different sections of the optical media

    • Can form a 3D scan based on individual images

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Axial resolution of cSLO is dependent on…

  • Dependent on f-number

    • focal length / D

<ul><li><p>Dependent on f-number</p><ul><li><p>focal length / D</p></li></ul></li></ul><p></p>
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What is numerical aperture?

Math concept relating f-number to cSLO imaging

NA = 1 / (2 * f #)

<p><em>Math concept relating f-number to cSLO imaging</em></p><p>NA = 1 / (2 * f #)</p>
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Equation to determine axial resolution (∆z) of cSLO

<p></p>
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Factors lowering axial resolution

𝛥z= 1.4𝛌/NA2

𝛥z= 5.6𝛌 f/#2

f/# = f / D

  • Smaller pupil

    • ↓ D = ↑ f/# = ↑ ∆z = Lower resolution

  • Longer wavelength

  • Uncorrected aberrations

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Optical coherence tomography (OCT) offers very high…

Axial resolution (∆z)

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OCT is analogous to what type of imaging?

Ultrasound

Ultrasound

  • Measures time for sound to bounce back

  • Axial resolution ~100um

OCT

  • Measures time for light to bounce back

  • Axial resolution ~5-10um

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Two main types of OCT’s

  • Time domain OCT

  • Spectral (Fourier) domain OCT

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Low-coherence interferometry

Refers to interferometer emitting a beam but…

  • Light source is only “coherent” over a short distance before dissociating

<p><strong>Refers to interferometer emitting a beam but…</strong></p><ul><li><p>Light source is only “coherent” over a short distance before dissociating</p></li></ul><p></p>
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How do OCT’s induce short coherence lengths?

Light source of super-luminescent diode (SLD)

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How does an OCT work?

  • OCT shoots short coherence light onto the retina

    • One beam is reflected from the tissue sample

    • One beam reflected off mirror in the OCT

Both beams interfere with each other over a short distance

  • Limitation in distance allows you to pinpoint the depth at which the interference signal is coming from

Therefore axial resolution of the OCT = coherence length of the source

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Time-domain OCT (TD-OCT)

Measures interference as a function of tissue depth

  • Reference and tissue beam shoot out (Normal OCT)

  • Mirror inside OCT moves around measuring

    • Depth of signal

    • Intensity of reflected ‘echoes’

  • Generates an A-scan

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Spectral (Fourier) OCT

  • Stationary reference mirror (Contrast to TD-OCT)

  • Spectrometer separates reflected light by wavelength

  • Resulting interpretation measures depth of scan to form OCT image

    • Faster than TD-OCT

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A,B,C scans

  • A scan → Single axial scan

  • B scan → Series of A scans across the retina, retinal slice

  • C scan → Vertical stack of B-scans in coronal plane

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Equation for axial resolution of OCTs

knowt flashcard image
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Bandwidth

Refers to the range of wavelengths within a light source

  • Lasers → Narrow bandwidth

  • SLDs → Broader bandwidth

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Best combined SD-OCT and cSLO system

Heidelberg engineering cSLO and OCT

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Adaptive optics systems can be applied to…

  • Fundus cameras

  • SLO

  • OCT

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3 main components of adaptive optics systems

  • Wavefront sensor (WFS)

    • Measures wavefront aberrations

  • Wavefront corrector

    • Corrects aberrations with deformable mirror

  • Control computer

    • Controls the WFS and DM