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- W840751432 abstract "The purposes of spectroscopy in astronomy are to measure the radiation flux of the spectroscopic emission or absorption line and to measure the dynamical parameters of the line profile. In order to use an appropriate instrument for the scientific purpose, we need to understand the characteristics of various spectrometers, e.g., a prism spectrometer, a grating spectrometer, and a Fabry-Perot spectrometer (FPS), which are being used in ultra-violet, optical, and infrared bands. The FabryPerot spectrometer is not very popular compared to the grating spectrometer, because of its complex and tricky operations. The Fabry-Perot spectrometer, however, can get a two-dimensional image at one exposure, so we can study radiation mechanisms and dynamical properties of extended sources, e.g., clusters, nebula, and galaxies." @default.
- W840751432 created "2016-06-24" @default.
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- W840751432 date "2000-01-01" @default.
- W840751432 modified "2023-09-28" @default.
- W840751432 title "FABRY-PEROT SPECTROMETER IN ASTRONOMY" @default.
- W840751432 hasPublicationYear "2000" @default.
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