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1PIBM Sept 05 Andy Harvey
Spectral Imaging of the Retina
Andy R.Harvey, Ied Abboud, Alistair Gorman, Andy I.McNaught*
School of Engineering & Physical Sciences,
Heriot Watt University, Edinburgh, UK
*Eye Unit,Cheltenham General Hospital,
Cheltenham, UK
2PIBM Sept 05 Andy Harvey
Outline
• What is spectral imaging?• Spectral retinal imaging
• Why?• Spectral time-sequential spectral imaging
• For flexibility and research
• 2D snapshot• For real-time, high throughput screening
• Conclusions
3PIBM Sept 05 Andy Harvey
Conventional Spectral Imaging
RGB Image Spectrally classified image
Dysplasticcell
Superficialsquamouscell
Intermediatecell
Lymphocyte
PMN
Courtesy CRI
Classificationspectra
4PIBM Sept 05 Andy Harvey
Imaging the eye
Sclera
Cornea
Iris
Lens
Retina
Macula
Vitreous humour
Light
Anterior chamber (full of aqueous humour)
Optic nerve
Posterior chamber
Choroid
Optic disc
5PIBM Sept 05 Andy Harvey
The Role of Spectral Retinal Imaging
• By 2020 there will be 200 million visually-impaired people world wide• Glaucoma, diabetic retinopathy, ARMD• 80% of those cases are preventable or
treatable • Screening and early detection are
crucial • Can spectral imaging offer
enhancements to current screening techniques ?
• Spectral imaging is non-invasive and safe• cf. fluorescein angiogram
• Spectral imaging can enable imaging of • Retinal biochemistry
• Blood oximetry• Diabetic retinopathy, glaucoma
• Lipofuscin etc• Age-related macula degeneration
6PIBM Sept 05 Andy Harvey
Spectral Imaging:Traditional approaches
And Fourier-transform equivalents
N(t)
NxNy
N
NxNy(t)
Time-sequential spectral multiplex
Time-sequential spatial multiplex
• Limitations
• Optically inefficient
• 2D time-varying scenes
• 2D snapshot
• required for:• Retinal
imaging• in vitro, in
vivo imaging
7PIBM Sept 05 Andy Harvey
Spectral Fundus Camera
• Source filtering by LCTF incorporated into COTS fundus camera• 10 nm spectral width• 20 msec random access
• Images captured using a cooled, low-noise CCD camera
8PIBM Sept 05 Andy Harvey
1.00
10.00
100.00
1000.00
10000.00
200 400 600 800 1000
Wavelength (nm)
Abs
orpt
ion
Coe
ffici
ent (
cm-1
)
Absorption Coefficient for HbO2 (cm-1)
Absorption Coefficient for Hb (cm-1)
Isobestic point
Coregistered Spectral Images of a Healthy Retina
800nm
Images translationally and rotationally coregistered
9PIBM Sept 05 Andy Harvey
Spectral angle map of healthy and diabetic retina
• Shading indicates similarity of each pixel spectrum with artery and vein spectra• Qualitative oxymetry
Normal Retina
Diabetic Retina
10PIBM Sept 05 Andy Harvey
Supervised spectral classifiaction
• Implicit calibration based on spectral signatures within the eye• Classification possible
without absolute calibration
• Clear distinction between veins/arteries, on/off optic disc • Spectra depends on
local environment
• Inversion of data to calculate biochemical concentrations (eg oxygenation) requires a model of light propagation and scattering in the retina to remove environmental effects
• Monte Carlo, Kubelka Monk, Transfer equation
11PIBM Sept 05 Andy Harvey
Requirements for a snapshot technique: retinal imaging
• Improved calibration
• Patient patience
• Remove imperfect coregistration
• due to Variations in imaging distortion between images
• Similar issues with other in vivo applications
• Imaging internal epithelial cancers
• Eg gastrointestinal
PC15
12PIBM Sept 05 Andy Harvey
Image Replication Imaging Spectrometer: IRIS
Snapshot image• zero temporal misregistration
• ‘100%’ optical efficiency• World’s only snapshot, 2D
spectral imager (almost !)• Conceptually related to Lyot
filter
Large formatdetector
SpectralDemultiplexor
13PIBM Sept 05 Andy Harvey
Lyot filter: principle of operation
n=1 � l Cos2@pîDDCos2@pîDDCos2@2pîDDCos2@pîDDCos2@2pîDDCos2@4pîDDCos2@pîDDCos2@2pîDDCos2@4pîDDCos2@8pîDD
PolariserWaveplate
14PIBM Sept 05 Andy Harvey
Exploded view of N Wollaston prisms N wave plates
2N spectral images at detector Field
stop
Input polarizer
• Wollaston prism polarisers replicate images• Each Wollaston prism-waveplate pair provides both cos2 and sin2 responses
• All possible products of spectral responses are formed at detector
)(sin
)(cos2
2
)2(sin
)2(cos2
2
)4(sin
)4(cos2
2
IRIS snapshot spectral imager: principle of operation
15PIBM Sept 05 Andy Harvey
Spectral transmission
cos2
sin2
cos2(cos2(2)
sin2 (
cos2 (2)
cos2(sin2(2)
sin2(sin2(2)
cos2(cos2(2)cos2(4) cos2(sin2(2)cos2(4)
cos2(cos2(2)sin2(4) cos2(sin2()sin2(4)
sin2(cos2(2)cos2(4) sin2(sin2(2)cos2(4)
sin2(cos2(2)sin2(4) sin2(sin2()sin2(4)
Wollaston/waveplateassembly
16PIBM Sept 05 Andy Harvey
Spectral responses
• Bands are overlapping bell shapes• Choose cost function to minimise sidelobes
• Small (~5%) reduction in spectral separation• Cut-off filters used to define spectral range
Theoretical system response
0
20
40
60
80
100
450 500 550 600 650 700 750 800 850
Wavelength (nm)
Res
po
nse
(%
)
•8 channel visible-band system
•520nm820m
•3 Quartz retarders
•32 channel, visible-band system
•520nm 720nm
•5 Quartz retarders
17PIBM Sept 05 Andy Harvey
Optical scaling laws
Hamamatsu
ORCA-ER
Inputs:
FoV
Sub image size on CCD
CCD pixel size
Primary lens magnification & F#
Collimating lens back focal distance, focal length & front element diameter
Prism birefringence
Outputs:
Field stop size
Collimating lens rear element diameter
Splitting angles, apertures & depths of prisms
Apertures of retarders, polarisers and filters
Imaging lens focal length & front element diameter
Field stopCollimating
lens
Bandpass
filter
Imaging
lens
Camera
Polariser, retarders & Wollaston prisms
(index matched)Primary lens
18PIBM Sept 05 Andy Harvey
Components & Assembly
• 8 channel system• 520nm to 820nm• 3 Quartz retarders• 3 Calcite Wollaston prisms
19PIBM Sept 05 Andy Harvey
Spectral Retinal Imaging • Difficult imaging conditions render application of traditional HSI
techniques problematic• IRIS enables real-time and snapshot spectral imaging
Canon CR4-45NMCR4-45NM
20PIBM Sept 05 Andy Harvey
Blood oximetry
• Optimal spectral band for retinal oximetry• Vessel thickness ~ optical depth• 570-615 nm• Eight bands approximately equally spaced
0
2
4
6
8
10
12
14
16
18
20
565 575 585 595 605 615 625
Wavelength (nm)
Tra
nsm
issi
on (
%)
40
20
80
21PIBM Sept 05 Andy Harvey
Video sequence recorded with bandpass filtered inspection lamp
22PIBM Sept 05 Andy Harvey
Retinal image recorded with flash illumination
23PIBM Sept 05 Andy Harvey
574581585592595603607613
Coregistered and PCA images
PC1PC2PC1 & PC2
24PIBM Sept 05 Andy Harvey
Summary
• Spectral imaging of the retina shows promise for non-invasive detection of retinal disease• Clinical trials on-going
• LCTF-based, time-sequential spectral filtering enables rapid and flexible 2D spectral retinal imaging• Flexible data acquisition• Pulse and other motion artefacts limit accuracy
• Snapshot spectral imaging in 2D (IRIS) promises high-performance real-time multi-spectral imaging• Ideal for in vivo imaging• No temporal misregistration
• Absolute, quantitative data requires a model of light interaction within the retina
25PIBM Sept 05 Andy Harvey
• Wollaston prism polarisers replicate images• Each Wollaston prism-waveplate pair provides both cos2 and sin2 responses
• All possible products of spectral responses are formed at detector
Exploded view of N Wollaston prisms N wave plates
2N spectral images at detector Field
stop
Input polarizer
IRIS snapshot spectral imager
26PIBM Sept 05 Andy Harvey
Measured & predicted spectral responses
27PIBM Sept 05 Andy Harvey
Absolute total transmission
• Bandpass filter & polariser dominate losses
• Improved system: T>80%
• Theoretical throughput is 2n times higher than for spatial/spectral multiplexed techniques!
0
25
50
Re
sp
on
se
(%
)
Absolute response curves in polarised light
28PIBM Sept 05 Andy Harvey
Application to microscopy:Imaging of multiple fluorophors
• IRIS fitted to conventional epi-fluorescence microscope
• Germinating spores of Neurospora crassa stained with• GFP – nucleii fluoresce at 510 nm• FM4-64 – membranes fluoresce at >580 nm0
25
50
Re
sp
on
se
(%
)
29PIBM Sept 05 Andy Harvey
Principle component decomposition
PC1
PC15
• Artery structure is a pulse artefact
• Very difficult to co-register by image processing means
• Snapshot technique desirable
PC3
30PIBM Sept 05 Andy Harvey
Conclusions
• IRIS is a new spectral imaging technique that enables snapshot spectral imaging in 2D• No rejection of light• No data inversion
• Highest-possible signal-to-noise ratios• Simple logistics
• Inherently compact and robust• Simply fitted to conventional imaging systems
• Birefringent materials exist for applications from 0.2m to 12 m
• Applications• In vivo, in vitro imaging
• Retinal imaging• Microscopy
• Multiple fluorophors• Quantum dots
• Surveillance• Remote sensing• Etc.
31PIBM Sept 05 Andy Harvey
• Optical depth of Hb & HbO2 dominates variation of penetration with
• Tissues vary between highly turbid and transparent• Blue light images retinal surface• Light at ~600 nm enables spectral oximetry within retinal blood vessels
• optical depth of HbO2 > vessel thickness so vessels translucent
• optical depth of Hb < vessel thickness so vessels are opaque
• Light > 640 nm penetrates to coroid
BlueGreenRed
1.00
10.00
100.00
1000.00
10000.00
200 400 600 800 1000
Wavelength (nm)
Abs
orpt
ion
Coe
ffici
ent (
cm-1
)
Absorption Coefficient for HbO2 (cm-1)
Absorption Coefficient for Hb (cm-1)
Isobestic point
Spectral Characteristics of the Retina
32PIBM Sept 05 Andy Harvey
Issues for Spectral Retinal Imaging
• Calibration• Components of interest within a
complex turbid medium• Patient tolerance
• Using current technology, time-sequentialspectral bandpass offers• Optimal SNR• Reduced light intensity at the retina• Agile selection of spectral bands (data efficient)
• Issues• Coregistration• Calibration
± 100 pixels
±2º
• Spectral imaging of static scenes is relatively ‘easy’
• Spectral imaging of the retina encounters
• Imaging through an erratically moving, low-quality f/6 eye-lens system
Solutions: 2D snapshot spectral imaging
33PIBM Sept 05 Andy Harvey
The End
34PIBM Sept 05 Andy Harvey
1D image x path difference
Fixedmirror
Scanning mirror
Detector array
N
NxNy(t)
N
NxNy(t)
FTFT
N(t)
NxNy
N
NxNy(t)
Direct Imaging Spectrometry (Fourier) Transform Imaging SpectrometryT
emp
oral
ly s
can
ned
Sn
apsh
ot/f
ull
y st
arin
g
N(t)
NxNy
FT
N
NxNy
35PIBM Sept 05 Andy Harvey
Why another spectral imaging technique?
• Traditional approaches• Time sequential spectral multiplex
• Monochromatic two-dimensional image in snapshot• Time sequential spatial multiplex
• One-dimensional spectral image in a snapshot• (and Fourier-transform equivalents)
• Problems• Cannot record two-dimensional spectral images of time-varying
scenes• Optically inefficient
• Time-resolved (snapshot) spectral imaging is required for• Dynamic scenes
• In vitro, in vivo imaging and microsocopy• Combustion dynamics, surveillance…
• Irregular motion between scene and imager• In vivo imaging• Ophthalmology• Remote sensing, airborne surveillance, industrial inspection…