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Cardinal planes and matrix methods

Cardinal planes and matrix methods. Monday September 23, 2002. Principal planes for thick lens ( n 2 =1.5 ) in air. Equi-convex or equi-concave and moderately thick  P 1 = P 2 ≈ P/2. H. H’. H. H’. Principal planes for thick lens ( n 2 =1.5 ) in air.

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Cardinal planes and matrix methods

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  1. Cardinal planes and matrix methods Monday September 23, 2002

  2. Principal planes for thick lens (n2=1.5) in air Equi-convex or equi-concave and moderately thick  P1 = P2≈ P/2 H H’ H H’

  3. Principal planes for thick lens (n2=1.5) in air Plano-convex or plano-concave lens with R2 =   P2= 0 H H’ H H’

  4. Principal planes for thick lens (n=1.5) in air For meniscus lenses, the principal planes move outside the lens R2 = 3R1 (H’ reaches the first surface) H H’ H H’ H H’ H H’ Same for all lenses

  5. Examples: Two thin lenses in air H H’ ƒ1 ƒ2 n = n2 = n’ = 1 Want to replace Hi, Hi’ with H, H’ d h h’ H1 H1’ H2 H2’

  6. Examples: Two thin lenses in air H H’ ƒ1 ƒ2 n = n2 = n’ = 1 F F’ d ƒ’ ƒ s s’

  7. Huygen’s eyepiece In order for a combination of two lenses to be independent of the index of refraction (i.e. free of chromatic aberration) Example, Huygen’s Eyepiece ƒ1=2ƒ2 and d=1.5ƒ2 Determine ƒ, h and h’

  8. Huygen’s eyepiece H1 H’ H2 H h’ = -ƒ2 h=2ƒ2 d=1.5ƒ2

  9. Two separated lenses in air f1’=2f2’ H’ H H’ H F’ F’ F F f’ f’ d = f2’ d = 0.5 f2’

  10. Two separated lenses in air f1’=2f2’ Principal points at  H’ H F’ F f’ d = 3f2’ d = 2f2’ e.g. Astronomical telescope

  11. Two separated lenses in air f1’=2f2’ e.g. Compound microscope H H’ F’ F f’ d = 5f2’

  12. Two separated lenses in air f1’=-2f2’ e.g. Galilean telescope d = -f2’ Principal points at 

  13. Two separated lenses in air f1’=-2f2’ H H’ F F’ f’ e.g. Telephoto lens d = -1.5f2’

  14. Matrices in paraxial Optics Translation (in homogeneous medium)  0 y yo L

  15. Matrix methods in paraxial optics Refraction at a spherical interface  y ’  φ ’ n n’

  16. Matrix methods in paraxial optics Refraction at a spherical interface  y ’  φ ’ n n’

  17. Matrix methods in paraxial optics Lens matrix n nL n’ For the complete system Note order – matrices do not, in general, commute.

  18. Matrix methods in paraxial optics

  19. Matrix properties

  20. Matrices: General Properties For system in air, n=n’=1

  21. System matrix

  22. System matrix: Special Cases (a) D = 0  f = Cyo (independent of o) f yo Input plane is the first focal plane

  23. yf o System matrix: Special Cases (b) A = 0  yf = Bo (independent of yo) Output plane is the second focal plane

  24. yf System matrix: Special Cases (c) B = 0  yf = Ayo yo Input and output plane are conjugate – A = magnification

  25. o f System matrix: Special Cases (d) C = 0  f = Do (independent of yo) Telescopic system – parallel rays in : parallel rays out

  26. Examples: Thin lens Recall that for a thick lens For a thin lens, d=0 

  27. Examples: Thin lens Recall that for a thick lens For a thin lens, d=0  In air, n=n’=1

  28. Imaging with thin lens in air ’ o yo y’ Input plane Output plane s s’

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