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diffraction |
Also found in: Encyclopedia, Wikipedia, Hutchinson | 0.04 sec. |
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diffraction /dif·frac·tion/ (dĭ-frak´shun) the bending or breaking up of a ray of light into its component parts.
diffraction [difrak′shən] Etymology: L, dis, opposite of, frangere, to break the bending and scattering of wavelengths of light or other radiation as the radiation passes around obstacles or through narrow slits. X-ray diffraction is used in the study of the internal structure of cells. See also refraction. diffraction the bending or breaking up of a ray of light into its component parts. x-ray diffraction
a method used to determine the three-dimensional structure of the single object, e.g. protein molecule, that composes the crystal. Based on recording and analyzing the diffraction pattern of an x-ray beam passing through a crystalline structure, either organic or inorganic. diffraction Deviation of the direction of propagation of a beam of light, which occurs when the light passes the edge of an obstacle such as a diaphragm, the pupil of the eye or a spectacle frame. There are two consequences of this phenomenon. First, the image of a point source cannot be a point image but a diffraction pattern. This pattern depends upon the shape and size of the diaphragm as well as the wavelength of light. Second, a system of close, parallel and equidistant grooves, slits or lines ruled on a polished surface can produce a light spectrum by diffraction. This is called a diffraction grating. See Airy's disc; diffraction fringes; Maurice's theory. How to thank TFD for its existence? Tell a friend about us, add a link to this page, add the site to iGoogle, or visit webmaster's page for free fun content. |
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| For sharp tips, the electromagnetic coupling was confined to a lateral range of a few nanometers, a factor of 100 better than the diffraction limit of conventional optics. What enables the new microscope to both beat the diffraction limit and reduce distortion from its oblong spot, he explains, is a one-two combination of laser pulses. Even at its calmest, however, the atmosphere blurs star images to a diameter at least 10 times greater than a large telescope's natural diffraction limit. |
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