| 翻訳と辞書 |
| Integral field spectrograph ： ウィキペディア英語版 |
Integral field spectrograph
An integral field spectrograph or a spectrograph equipped with an integral field unit (IFU) is an optical instrument combining spectrographic and imaging capabilities, used to obtain spatially resolved spectra in astronomy and other fields of research such as bio-medical science and earth observation (or remote sensing).
== Rationale ==
Integral field spectroscopy (IFS) has become an important sub-discipline of astronomy with the proliferation of large aperture, high-resolution telescopes where there is a need to study the spectra of extended objects as a function of position, or of clusters of many discrete stars or point sources in a small field. Such spectroscopic investigations have previously been carried out with long-slit spectrographs in which the spectrum is dispersed perpendicular to the slit, and spatial resolution is obtained in the dimension along the slit. Then by stepping the position of the slit, the spectrum of points in the imaged field can be obtained, but the process is comparatively slow, and wasteful of potentially restricted telescope time. Integral field spectrographs are used to speed up such observations by simultaneously obtaining spectra in a two-dimensional field. As the spatial resolution of telescopes in space (and also of ground-based instruments using adaptive optics) has rapidly improved in recent years, the need for such multiplexed instruments has become more and more pressing.
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
■ウィキペディアで「Integral field spectrograph」の詳細全文を読む
スポンサード リンク
| 翻訳と辞書 : 翻訳のためのインターネットリソース |
Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.
|
|