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Lecture 22 Wave Optics-3 Chapter 22

Lecture 22 Wave Optics-3 Chapter 22. PHYSICS 270 Dennis Papadopoulos April 2, 2010. Gratings. Phase Arrays. What happens when slit is too large to be considered a point source ? Huygens principle replace wave-front by a continuous series of point sources.

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Lecture 22 Wave Optics-3 Chapter 22

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  1. Lecture 22Wave Optics-3 Chapter 22 PHYSICS 270 Dennis Papadopoulos April 2, 2010

  2. Gratings Phase Arrays

  3. What happens when slit is too large to be considered a point source ? Huygens principle replace wave-front by a continuous series of point sources

  4. When to use ray optics and when wave optics

  5. Actual double slit interference pattern (a<d and a> wavelength) – Convolution of ideal double slit and single slit patterns

  6. Raleigh Criterion • Two objects are resolvable if a>qmin=1.22l/D, namely the angle of the first dark fringe of the diffraction pattern • Objects not resolvable if a<qmin • Objects marginally resolvable if a=qmin

  7. Resolution limit -- Rayleigh’s criteria For circular aperture, slightly different:

  8. The Resolution of Optical Instruments The minimum spot size to which a lens can focus light of wavelength λis where D is the diameter of the circular aperture of the lens, and f is the focal length. In order to resolve two points, their angular separation must be greater than θmin, where is called the angular resolution of the lens. The same criterion applies to the focusing spot of mirrors if D is the diameter of the mirror

  9. Raleigh Criterion • Two objects are resolvable if a>qmin=1.22l/D, namely the angle of the first dark fringe of the diffraction pattern • Objects not resolvable if a<qmin • Objects marginally resolvable if a=qmin

  10. EXAMPLE The Hubble space telescope has a diameter 2.4 meters. It is used to photograph objects 30000 light years away ( 1 light year is 9.46x1015 meters). Assume that it uses red light with 650 nm wavelength. What is the distance between two stars that can be resolved?

  11. The Eye-Angular Magnification- Resolution SECTIONS 24.3-24.4-24.5

  12. Vision • The human eye is roughly spherical, about 2.4 cm in diameter. • The transparent cornea and the lens are the eye’s refractive elements. • The eye is filled with a clear, jellylike fluid called the aqueous humor and the vitreous humor. • The indices of refraction of the aqueous and vitreous humors are 1.34, only slightly different from water. • The lens has an average index of 1.44. • The pupil, a variable-diameter aperture in the iris, automatically opens and closes to control the light intensity. • The f-number varies from roughly f/3 to f/16, very similar to a camera. f-number = f/D f/3 means that f-number is 3

  13. Focusing and Accommodation • The eye focuses by changing the focal length of the lens by using the ciliary muscles to change the curvature of the lens surface. • Tensing the ciliary muscles causes accommodation, which decreases the lens’s radius of curvature and thus decreases its focal length. • The farthest distance at which a relaxed eye can focus is called the eye’s far point (FP). The far point of a normal eye is infinity; that is, the eye can focus on objects extremely far away. • The closest distance at which an eye can focus, using maximum accommodation, is the eye’s near point (NP). Usually 25 cm

  14. Cannot focus any closer than the near point of the eye ~ 25 cm

  15. Angular Magnification Exercise: Compare concepts and scaling of angular vs. lateral magnification

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