310 likes | 505 Views
Optical systems: The eye, magnifier, microscope, telescope & binoculars . Hecht 5.7 Monday October 7, 2002. Human Eye, Relaxed. 20 mm. 15 mm. n’ = 1.33. F. H. H’. F’. 3.6 mm. P = 66.7 D. 7.2 mm. Accommodation. Refers to changes undergone by lens to enable imaging of closer objects
E N D
Optical systems:The eye, magnifier, microscope, telescope & binoculars Hecht 5.7 Monday October 7, 2002
Human Eye, Relaxed 20 mm 15 mm n’ = 1.33 F H H’ F’ 3.6 mm P = 66.7 D 7.2 mm
Accommodation • Refers to changes undergone by lens to enable imaging of closer objects • Power of lens must increase • There is a limit to such accommodation however and objects inside one’s “near point” cannot be imaged clearly • Near point of normal eye = 25 cm • Fully accommodated eye P = 70.7 for s = 25 cm, s’ = 2 cm
Myopia: Near Sightedness Eyeball too large ( or power of lens too large)
Myopia – Near Sightedness Far point of the eye is much less than ∞, e.g. lf Must move object closer to eye to obtain a clear image Normal N.P. Myopic F.P. Myopic N.P.
Myopia e.g. lf = 2m How will the near point be affected? 0.5 + 66.7 = 67.2 D is relaxed power of eye – too large! To move far point to ∞, must decrease power to 66.7 Use negative lens with P = -0.5 D
Laser Eye surgery Radial Keratotomy – Introduce radial cuts to the cornea of the elongated, myopic eyeball Usually use the 10.6 µm line of a CO2 laser for almost 100% absorption by the corneal tissue Blurred vision Front view
Laser Eye surgery Radial Keratotomy – Introduce radial cuts to the cornea of the elongated, myopic eyeball Usually use the 10.6 µm line of a CO2 laser for almost 100% absorption by the corneal tissue Distinct vision Front view Flattening
Hyperopia – Far Sightedness Eyeball too small – or lens of eye can’t fully accommodate Image of close objects formed behind retina
Hyperopia – Far Sightedness Suppose near point = 1m Recall that for a near point of 25 cm, we need 70.7D Use a positive lens with 3 D power to correct this person’s vision (e.g. to enable them to read) Usually means they can no longer see distant objects - Need bifocals
Correction lenses for myopia and hyperopia http://users.rcn.com/jkimball.ma.ultranet/BiologyPages/V/Vision.html
Hand magnifier Observation with unaided eye θ
Magnifier To maximize the image, bring object as close to the eye as possible, i.e. bring object to near point s = ln = 25 cm h’ θmax
Hand Magnifier What is the angular magnification of the image for an object at the near point or at ∞? With thin lens H,H’ h” θ’ F so hM’ l f s’ L
Compound Microscope x’ L Fe Fo Fo Fe Recall xx’ = fo2 x x’ ≈ L Wish to have intermediate image (h’) just inside the focus of the eyepiece x = fo2/L s’ ≈ fo + L s = x + fo
Compound Microscope L Fe h h’ Fo Fo Fe h” • Recall: The magnification of an image formed • at the near point is • at infinity
Compound microscope Total magnification (Image at infinity) (Image at near point)
Compound Microscope In most microscopes, L ~ 16 - 17 cm Objective Eyepiece (image at ∞) 10 X, 20 X, 40 X etc fe = 2.5 cm 10X Me = 10 40X fo = 0.4 cm Overall magnification M = 40X10 = 400
Compound Microscope L A.S. Fe Fo Fo Fe EnP ExP Where should the eye be located to view the image? • Optimum viewing – • Place eye near ExP (moving eye away decreases illumination and F.O.V.) • Ensure that exit pupil ~ same size as eye pupil!
Compound Microscope L A.S. Fe Fo Fo Fe EnP ExP Chief Ray Marginal ray
Numerical Aperture Measure of light gathering power N. A. = n sin α Lens Air Oil αg αg’ αo αa Cover Glass ng O
Numerical Aperture If cover glass in air If cover glass immersed in oil (no = 1.516) – between glass and oil there is essentially no refraction since ng = 1.5 Increases the light gathering power by about 1.5 (N.A. roughly analogous to f# of a lens)
Numerical Aperture In optical fibres Cladding n2 Core n1 θc θ no αmax Cladding n2 N.A. = nosinαmax= n1sin θ = n1sin (90o - θc) = n1cos θc This is a measure of the maximum cone of light accepted
Viewing distant objects, e.g. stars star h θ feye Image size on retina h = feyeθ
Telescope Objective Eyepiece fo fe hT=feyeθ’ θ’ θ h’ θ’ h” s’
Telescope Show (magnification of the telescope) (diameter of the exit pupil)
The Hubble Space Telescope 0.3 m secondary mirror 2.4 m primary mirror
Binoculars Two telescopes side-by-side Prisms used to erect images Objective Eyepiece
Binoculars “6 X 30” Angular Magnification (M) Diameter of objective lens, Do (mm) Exit pupil = 5 mm, a good match to the normal pupil diameter For night viewing, a rating of 7 X 50 is better: i.e. ~ 7 mm