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CHAPTER


                  The physics, instruments and

                  modalities of retinal imaging                              3







                                                                    b
                                                        a
                                          a
                                                                                    b
                           Andrew R. Harvey , Guillem Carles , Adrian Bradu , Adrian Podoleanu
                           a School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom
                                b School of Physical Sciences, University of Kent, Canterbury, United Kingdom
                  1  Introduction

                  The vital importance of the human eye has stimulated an enormous effort into imag-
                  ing the retina and other parts of the eye to provide clinical diagnostic information
                  on disease and for fundamental research. In this chapter we discuss how the physics
                  underpinning the formation of images of the retina impacts the salient features im-
                  portant for analysis of retinal images.
                     The fascination of the physicist with the eye dates back, at least, to the first gruesome
                  insertion by Newton, in 1665, of a ‘bodkin’ (needle) behind his eye ball [1]. Over the
                  succeeding three-and-a-half centuries we have developed a deep understanding of im-
                  age formation and vision in the eye. This has included the development of increasingly
                  elaborate imaging systems, originating with the first ophthalmoscopes at the time of von
                  Helmhotz [2] in 1851 and progressing through modern scanning-laser ophthalmoscopes
                  (SLO) for improved contrast and depth sectioning; optical-coherence tomography for
                  imaging the three-dimensional structure of the retina [3]; to emerging techniques such
                  as adaptive optics that enables the imaging of individual photoreceptors [4]. A vast range
                  of imaging techniques are used in ophthalmic research and clinical application. Over
                  the past two decades the digital recording of retinal images has become pervasive—and
                  with it the possibility of automated analysis of images for screening and providing ob-
                  jective metrics to aid diagnosis. The aim of this chapter is to highlight how the physics of
                  image formation within the eye leads to specific characteristics of retinal images. For ex-
                  ample: why is it that images recorded with a SLO appear different from those recorded
                  with a fundus camera? Why is it difficult to record images of individual blood cells and
                  the smallest capillaries? Why do arteries and veins appear so different?
                     The eye has more than a passing resemblance to a camera in terms of function
                  and shares many similar components. Like a modern camera, there is a lens for form-
                  ing an image, which can be varied for optimal focus at a range of distances (referred
                  to as accommodation by clinicians), an iris for adjusting the amount of transmitted
                  light, and an array of opto-electronic photoreceptors transduce the optical image into
                  an electronic signal for transmission and processing. Importantly, when we record

                  Computational Retinal Image Analysis. https://doi.org/10.1016/B978-0-08-102816-2.00003-4  19
                  © 2019 Elsevier Ltd. All rights reserved.
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