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Optical systems: Magnifier, microscope, telescope & binoculars . Hecht 5.7 Wednesday October 9, 2002. 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. s o. h M ’. l. f. s’. L.
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Optical systems:Magnifier, microscope, telescope & binoculars Hecht 5.7 Wednesday October 9, 2002
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