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Newton`s Rings - Manchester HEP
Newton`s Rings - Manchester HEP

...  To measure the wavelength of sodium light using the method of Newton's rings.  To gain familiarity with using a Vernier microscope. Introduction In this experiment the physical property of interference of light will be used to determine the wavelength,  , of a light source. The interference frin ...
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Diffraction and Interference

... “see” an atom in visible light? • If the size of object is the same as the wavelength of light, the image will be blurred by diffraction. Smaller objects won’t be seen at all • No optical microscope can be built big enough or designed well enough to overcome this diffraction limit. • Electron micros ...
Diffraction Intensity, resolving power, Xray diffraction
Diffraction Intensity, resolving power, Xray diffraction

... Circular apertures • An aperture of any shape forms a diffraction pattern. • The figures below illustrate diffraction by a circular aperture. The Airy disk is the central bright spot. • The first dark ring occurs at an angle given by sinθ1 = 1.22 λ/D. ...
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Lecture 31 - Purdue Physics

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3.0Mb PDF - David Kleinfeld

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Airy disk



In optics, the Airy disk (or Airy disc) and Airy pattern are descriptions of the best focused spot of light that a perfect lens with a circular aperture can make, limited by the diffraction of light. The Airy disk is of importance in physics, optics, and astronomy.The diffraction pattern resulting from a uniformly-illuminated circular aperture has a bright region in the center, known as the Airy disk which together with the series of concentric bright rings around is called the Airy pattern. Both are named after George Biddell Airy. The disk and rings phenomenon had been known prior to Airy; John Herschel described the appearance of a bright star seen through a telescope under high magnification for an 1828 article on light for the Encyclopedia Metropolitana:...the star is then seen (in favourable circumstances of tranquil atmosphere, uniform temperature, &c.) as a perfectly round, well-defined planetary disc, surrounded by two, three, or more alternately dark and bright rings, which, if examined attentively, are seen to be slightly coloured at their borders. They succeed each other nearly at equal intervals round the central disc....However, Airy wrote the first full theoretical treatment explaining the phenomenon (his 1835 ""On the Diffraction of an Object-glass with Circular Aperture"").Mathematically, the diffraction pattern is characterized by the wavelength of light illuminating the circular aperture, and the aperture's size. The appearance of the diffraction pattern is additionally characterized by the sensitivity of the eye or other detector used to observe the pattern.The most important application of this concept is in cameras and telescopes. Owing to diffraction, the smallest point to which a lens or mirror can focus a beam of light is the size of the Airy disk. Even if one were able to make a perfect lens, there is still a limit to the resolution of an image created by this lens. An optical system in which the resolution is no longer limited by imperfections in the lenses but only by diffraction is said to be diffraction limited.
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