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spectroheliograph

  (spĕk'trō-hē'lē-ə-grăf') pronunciation
n.

An instrument used to make spectroheliograms.

spectroheliographic spec'tro·he'li·o·graph'ic adj.
spectroheliography spec'tro·he'li·og'ra·phy (-ŏg'rə-fē) n.
 
 
Sci-Tech Encyclopedia: Spectroheliograph

A spectrographic instrument that produces mono-chromatic images of the Sun. In a simple form of the instrument, an image of the Sun from a solar telescope is focused on a plane containing the entrance slit of the spectroheliograph (see illustration). The light passing through the slit is collimated by a concave mirror that is tilted such that the light is incident on a plane diffraction grating. Part of the dispersed light from the grating is focused by a second concave mirror, identical to the first mirror, at an exit slit identical to the entrance slit. By symmetry of the optical system, the portion of the solar disk imaged on the entrance slit is reimaged in the plane of the exit slit with the same image scale but in dispersed wavelength. The light imaged along the exit slit then corresponds to the portion of the solar image falling on the entrance slit, but in the light of only a narrow region of the spectrum, as determined by the spectrographic dispersion. The particular wavelength sampled is set by the grating angle. By uniform transverse motion of the instrument such that the entrance slit is scanned across the solar image, the light passing through the exit slit maps out a corresponding monochromatic image of the Sun, which can be recorded photographically with a stationary camera or digitally by sequential readout of a linear array that moves with the exit slit. See also Astronomical spectroscopy; Diffraction grating; Sun.

Optical configuration of a simple spectroheliograph.
Optical configuration of a simple spectroheliograph.


 
Columbia Encyclopedia: spectroheliograph,
device for photographing the surface of the sun in a single wavelength of light, usually one corresponding to a chief element contained in the sun, e.g., hydrogen or calcium; the resulting photograph is called a spectroheliogram. The spectroheliograph was invented in 1890 independently by G. Hale and by H. Deslandres and modernized (1932) by R. R. McMath to take motion pictures. In operation, the instrument is preset by means of a prism or grating and a narrow slit that passes only one wavelength of light to a photographic plate or digital detector; the image of the sun is then moved slowly or stepwise across the entrance slit until the entire disk of the sun has been photographed. See spectrum.


 
Wikipedia: spectroheliograph

The spectroheliograph is an instrument used in astronomy. It captures a photographic image of the Sun at a single wavelength of light, a monochromatic image. The wavelength is usually chosen to coincide with a spectral wavelength of one of the chemical elements present in the Sun.

It was developed independently by George Ellery Hale and Henri-Alexandre Deslandres in 1890 and further refined in 1932 by Robert R. McMath to take motion pictures.

The instrument comprises a prism or diffraction grating, together with a narrow slit that passes a single wavelength (a monochromator). The light is focused onto a photographic medium and the slit is moved across the disk of the Sun to form a complete image.

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Dictionary. The American Heritage® Dictionary of the English Language, Fourth Edition Copyright © 2007, 2000 by Houghton Mifflin Company. Updated in 2007. Published by Houghton Mifflin Company. All rights reserved.  Read more
Sci-Tech Encyclopedia. McGraw-Hill Encyclopedia of Science and Technology. Copyright © 2005 by The McGraw-Hill Companies, Inc. All rights reserved.  Read more
Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2003, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/  Read more
Wikipedia. This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Spectroheliograph" Read more

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