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Diffraction-limited The ability to produce optical images with angular separations as small as the instrument's theoretical limit. A telescope with this capability is said to be diffraction limited.
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A diffraction grating consists of a set of many evenly spaced slits, in which the slit separation is very small.
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Diffraction Limited Electromagnetic waves diffract around the edges of opaque objects or on passing through or reflecting off a finite aperture, like a dish, lens or mirror.
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Diffraction of seismic waves provided the first clear-cut evidence for a lunar crust, mantle, and core analogous to those of the earth. The lunar crust is about 45 mi (70 km) thick, making the moon a rigid solid to a greater depth than the earth.
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diffraction The ability that waves have to bend around corners. The diffraction of light establishes its nature as a wave.
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diffractionthe spreading out of light as it passes the edge of an obstacle E ...
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Diffraction of light through the eye lashes Floaters Haidinger's brush Monocular diplopia (or polyplopia) from reflections at bound aries between the various ocular media Phosphenes from stimulation other than by light (e.g.
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DIFFRACTIONDiffraction is the ability of a wave to bend around corners. The diffraction of light established its wave nature.
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Diffraction Fringe Blurred fringe surrounding and image caused by wave properties of light. because of this no image detail smaller than the fringe can be seen Dirty Snowball Theory ...
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diffraction -- a disturbance of light (or other electromagnetic waves) as it passes through an opening or around an obstacle. Diffraction limits the ability to distinguish fine details in images.
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diffraction grating - (n.) A very closely ruled series of lines that, through their diffraction of light, provide a spectrum of radiation that falls on it. disk - (n.) ...
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Diffraction(a) A property which distinguishes wave-like motions. When a wave is incident upon a barrier which is broken by a narrow slit (of comparable size to the wavelength), then the slit will act as a new isotopic source of secondary waves.
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Diffraction grating A flat optical surface, transparent or reflecting, ruled with many parallel grooves at precisely spaced distances.
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diffraction ~: a dial invented in 1999 by M. Catamo & C. Lucarini. It has no gnomon, but the dial plate consists of a circular diffraction pattern, which forms a bright, ...
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Diffraction observed with incident parallel light. In Fraunhofer diffraction the wavefronts are parallel. Although a special case of Fresnel diffraction, it is far more important in most practical cases.
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diffraction The process by which the direction of radiation is changed so that it spreads into the geometric shadow region of an opaque or refractive object that lies in a radiation field. Diffraction is an optical edge effect.
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(2-fiber optics) The regions, far from source, where the diffraction pattern is substantially the same as that at infinity.
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When light is passed through a prism or a diffraction grating to produce a spectrum, the type of spectrum you will see depends on what kind of object is producing the light: is it a thick or thin gas, is it hot or cool, is it a gas or a solid?
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The actual calculation follows a similar course to that by which Huygens's conception of the resolution of a wave into components corresponding to the various parts of the wave-front is usually verified (see Diffraction Of Light).
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The photon displays clearly wave-like phenomena such as diffraction and interference on the length scale of its wavelength.
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The central spot in the diffraction pattern of the image of a star at the focus of a telescope, named after George Airy. It is surrounded by several fine diffraction rings like the rings around the bull's-eye of a target.
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The chemical analysis and physical study of inaccessible heavenly bodies were made possible by the invention in 1814 of the diffraction- grating spectroscope by the German physicist Joseph von Fraunhofer and his subsequent discovery of the spectral ...
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The small black circle in the center of the spot diagrams represent the diffraction limit for a 9.8" aperture. It is the same size as the airy disc seen using a high power eyepiece.
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Diffraction, the ability of light to bend around a sharp edge, certainly gave credence to the idea that light was a form of wave motion.
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A Compact Disc (CD) or Digital Versitile Disk (DVD) offers an example of a spectroscopic diffraction grating.
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diffraction effects from partially closing the mirror covers of the 1.5-m telescope. (A Digitized Sky Survey image of Alpha Centauri may become available at the Nearby Stars Database, or see one at Astronomy Picture of the Day.) ...
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diffraction The bending of light around an opaque physical edge that demonstrates the wave nature of light. dome In astronomy, the building that houses a telescope.
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Note the bright spikes going off in four directions from the bright star. These are called diffraction spikes and, if you see them, the object is a star even if it has been classified as a galaxy.
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For instance, the scattering of X-rays as they pass through a metal foil is easy to understand using a particle model, while the diffraction patterns produced when light is passed through narrow slits are easier to understand in terms of overlapping ...
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Fraunhofer's work with the spectra and also with diffraction gratings was seminal in the science of spectroscopy.
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The whole apparatus for doing this job is called a spectroscope (if you look through it), or a spectrograph (if the spectrum is recorded photographically or by some means other than the eye). All modern spectrographs use diffraction gratings; ...
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Joseph Fraunhofer (1787-1826) was a German physicist who first studied the Sun's (these dark lines are now called Fraunhofer lines). His work with the spectra and also with diffraction gratings was seminal in the science of spectroscopy.
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get good enough for them to demonstrate that a half-meter shaving mirror will blow eighteen centimeters of optical perfection clean out of the water, and if they start talking about faint galaxies you can always change the subject to diffraction ...
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The model was derived by fitting a helix of G-actin structures according to low- resolution fiber diffraction data from the filament. Several models of the filament have been proposed since.
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When the CCD camera sees a very bright star, some of the star's light spills over into neighboring pixels, making the pointlike star look like an extended light source. You can recognize a bright star by diffraction spikes - bright crosses centered ...
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See also: Light, Time, Wavelength, Second, Telescope
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