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Gratings, diffraction Rowland

The relationships in Figure 4-11 are strongly reminiscent of those that exist for ordinary light diffracted from a concave Rowland grating.24 To understand this process, it is best to look first at the reflection of light from a concave mirror. [Pg.121]

Rowland circle spect A circle drawn tangent to the face of a concave diffraction grating at its midpoint, having a diameter equal to the radius of curvature of a grating surface the slit and camera for the grating should lie on this circle. ro.lsnd, s3r-k3l ... [Pg.329]

Rowland ghost spect A false spectral line produced by a diffraction grating, arising from periodic errors in groove position. ro,l3nd, gost ... [Pg.329]

Many modern spectroscopes employ the diffraction grating instead of the prism. In the concave grating spectroscope, developed by Rowland, the collimating lens and telescope or camera objective are unnecessary because of the focusing effect of the grating itself. See Fig, 2,... [Pg.1531]

Rowland ghosts spurious intensity maximum spurred from periodic errors in the spacing of the ruled grooves in a diffraction grating. [Pg.163]

Diffraction gratings were studied by many scientists in the nineteenth century. By the end of the century gratings were improved markedly thanks to Rowland s studies. In the Rowland spectrograph the slit, grating, and camera were all in the same circle (Rowlands circle). [Pg.1]

Fraunhofer usually is credited with the discovery of the diffraction grating. His grating was made of parallel wires wound back and forth between the threads of two long screws. Rowland and Michelson improved on the grating and found it to be an excellent device to use as a replacement for the prism to produce spectra. It was found especially useful in the ultraviolet and infrared regions of the spectrum, where prisms encounter transparency problems. [Pg.60]

Concave diffraction gratings were first introduced The concave diffraction grating is an optical element in spectrometric practice by Henry Rowland in 1883. combining two functions (1) reflecting and focusing Based on Fermat s principle, Rowland was able to... [Pg.4462]

In the history of physics the diffraction grating stands out as one of the most important instruments. It seems to have been invented by the American astronomer David Ritten-house in about 1785 and rediscovered some years later by Joseph von Fraunhofer. Great progress in the manufacture of ruled gratings was due to Harry A. Rowland, who in 1882 built a machine for ruling gratings with an uncorrected periodic error much less than 1/300,000. [Pg.241]


See other pages where Gratings, diffraction Rowland is mentioned: [Pg.292]    [Pg.775]    [Pg.127]    [Pg.279]    [Pg.120]    [Pg.53]    [Pg.292]    [Pg.229]    [Pg.289]    [Pg.292]    [Pg.426]    [Pg.472]    [Pg.206]    [Pg.223]    [Pg.4463]    [Pg.4463]    [Pg.529]    [Pg.4]    [Pg.127]    [Pg.279]   
See also in sourсe #XX -- [ Pg.65 ]




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