Download presentation
Presentation is loading. Please wait.
1
Ophthalmic Optical Instruments I
Telescopes and Microscopes C. I. OPHTMALMOMETER, CHICAGO ILLINOIS ca 1899
2
TELESCOPES
3
Astronomical (Keplerian) Telescope
Image is Inverted objective eyepiece Fe Fo fe fo M = - fe fo Virtual image at 25 cm
4
Astronomical Telescope
objective eyepiece Fe Fo fe fo Virtual image at infinity D
5
Galilean Telescope plus lens fp fp negative lens fp fp’s coincide
final telescope parallel rays
7
Viewing Through a Galilean Telescope
parallel rays emmetropic eye object iImage UPRIGHT OBJECT APPEARS UPRIGHT D GTT 04
8
MICROSCOPES
9
ANGULAR MAGNIFICATION
Apparent size of object depends on angle it subtends at eye.
10
ANGULAR MAGNIFICATION
On average, an object cannot be closer than 25 cm from the eye to be seen clearly. Average distance of most distinct vision
11
cm (cm)
12
BASIC MICROSCOPE magnifier real image magnification
13
MICROSCOPE MAGNIFICATION
25 M = 2 f Im Im 25 M = = M X 1 Ob Ob f total
14
n a a D NA = sin n OBJECTIVES w.d. EXAMPLE a = 14 n = 1.00 (air)
Numerical Aperture (NA) Light gathering ability Resolution a n a NA = sin n EXAMPLE a D = 14 n = 1.00 (air) w.d. NA = 1.00 x sin(14 ) NA = 0.24
15
OBJECTIVES N.A. Examples
16
parallel rays from eyepiece
EYEPIECES (OCULARS) Huygens Ramsden parallel rays from eyepiece Real image Real image converging rays from objective D
17
REAL MICROSCOPE
18
EXPERIMENT 4 Basic Microscope iris diaphragm real image on card onion skin f Produce real image of onion skin on card. Mark distance of real image on base.
19
EXPERIMENT 4--CONTINUED
View real image with magnifier (“eyepiece”) real image plane f Adjust iris diaphragm. How does image change? Im 25 What is the total magnification? = M X Ob f total
20
Slit-lamp Biomicroscope
21
The slit-lamp biomicroscope begins with a microscope….
Eyepiece Objective Specimen
22
….change specimen, objective & eyepiece
….turned on its side ….change specimen, objective & eyepiece Huygens eyepiece objective subject image plane …….fundamental slit-lamp biomicroscope
23
Galilean telescope to change mag
Build in magnification change without changing working distance working distance fobj Galilean telescope to change mag no image in image plane
24
Galilean telescope to change mag
Build in magnification change without changing working distance working distance fobj Galilean telescope to change mag no image in image plane D
25
astronomical telescope
…..add lens to form image in eyepiece image plane astronomical telescope D
26
Porro* prism 2 right-angle prisms 1800 image rotation
reduce length of telescope displace image horizontally Porro -Abbe *Ignazio Porro – Italian optical instrument maker
27
Slit-lamp with folded optical path
28
D
29
binocular slit-lamp viewing system
30
Operating Microscope
31
Operating microscope optics are very similar to those of the slit-lamp.
33
binocular astronomical telescopes Change magnification without changing working distance magnification change: Galilean telescopes prism objective lens
34
Specular Microscope specular == “mirror-like”
Endothelial cells posterior surfaces flat & adjacent to aqueous Difference in index of refraction gives specular reflection Useful in seeing corneal endothelial cells
35
Specular Microscope D halogen lamp condenser slit dipping cone lens M
objective Ramsden eyepiece film or CCD D
36
endothelium { slit image specular reflections and stray light
37
Typical image of endothelium from specular microscope
38
Confocal Principle Red cell in thick sample imaged by lens
Blue cell, nearer to surface, imaged at different point Pinhole in image plane passes all light from blue cell Pinhole blocks most of light from red cell Based on Webb, RH, Rep Prog Phys 59:427
39
Confocal Principle Point source CONFOCAL with blue cell & pinhole selectively illuminates blue cell Confocal point source gives less light to red cell, and most is blocked by pinhole Beam splitter makes confocal microscope epitaxial Based on Webb, RH, Rep Prog Phys 59:427
40
Confocal Optical Systems:
Pinhole allows light from small volume in sample. Other stray light blocked. Confocal point source confines light to small volume in sample. Rejects stray light Allows Z-axis “sectioning”
41
Confocal systems can improve imaging
Standard specular microscope Confocal specular microscope
42
Koester’s confocal microscope
43
M M Koester’s Confocal scanning microscope CCD camera lamp
confocal slit slit rotating mirror Koester’s Confocal scanning microscope objective specimen
45
Other Scanning Methods and Confocal Microscopes
Tandem Scanning Confocal Microscope Scanned (laser) Spot Confocal Microscope Scanned Slit Confocal Microscope
46
Tandem Scanning Confocal Microscope
q r Uses Nipkow disk Paul Nipkow ( ) Studied with Helmholtz Invented disk in 1883 Used for telegraphing pictures Later used in 1st television r = a + bq Sets of holes in plate Holes on Archimedes spirals D
48
Petran Tandem Confocal Scanning Microscope
Very light inefficient Petran Tandem Confocal Scanning Microscope
49
TCSM for imaging cornea
51
X-Y mirror confocal laser scanning
52
Confocal slit scanning
53
3-D reconstruction from confocal images
d fiber from subepithelial plexus Guthoff et al. Cornea 24:608
54
Commercial Confocal Scanning Corneal Microscopes
Heidelberg HRT II*-Rostock attachment Nidek Confoscan Topcon SP-2000p *also scans retina
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.