地面FTS和红外阵列光谱学

Fourier Transform Spectroscopy Pub Date : 1900-01-01 DOI:10.1364/fts.1997.fwc.1

K. Hinkle

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引用次数: 0

摘要

1978年，基特峰国家天文台在4米望远镜上引入了最大路径差为1.8米的FTS，作为夜间天文学的设施仪器。这台仪器在记录了数以万计的光谱后，于1995年退役。Hall等人(1979)描述了这种FTS。请注意，虽然4米FTS功能相似，但它与基特峰麦克马斯-皮尔斯太阳望远镜上的FTS不同。麦克马斯-皮尔斯FTS (Brault 1978, 1985)继续广泛用于太阳能和实验室工作。

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Ground Based FTS and Infrared Array Spectroscopy

In 1978 Kitt Peak National Observatory introduced a FTS of 1.8 m maximum path difference as a facility instrument for night-time astronomy at the 4 meter telescope. This instrument was decommissioned in 1995, after having recorded tens of thousands of spectra. This FTS is described by Hall et al. (1979). Note that the 4 meter FTS while similar in function is not the same instrument as the FTS at the Kitt Peak McMath-Pierce solar telescope. The McMath-Pierce FTS (Brault 1978, 1985) continues to be used extensively for both solar and laboratory work.

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Fourier Transform Spectroscopy

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