PNL/KPNO大地频谱计划

G. Stokes, J. Brault, L. Testerman
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引用次数: 0

摘要

在一年多的时间里,我们利用基特峰国家天文台麦克马斯太阳望远镜的傅立叶变换光谱仪(FTS)获得了地球大气在1.0-2.5μm区域的月度光谱。目前,光谱是在1到10个气团范围内获得的。单个光谱覆盖了整个1.0 ~ 2.5μm区域,分辨率为9.5 mK。除10个气团光谱外,其余气团光谱的信噪比均大于1000。
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The PNL/KPNO Telluric Spectrum Program
For more than a year we have obtained monthly spectra of the earth s atmosphere in the 1.0-2.5μm region using the Fourier Transform Spectrometer (FTS) at the McMath Solar Telescope of Kitt Peak National Observatory. At the present time the spectra are obtained over a range of airmasses ranging between 1 and 10 airmasses. The individual spectra cover the entire 1.0-2.5μm region in a single observation with a resolution of 9.5 mK. The signal-to-noise ratios are generally greater than 1000 for all but the 10 airmass spectra.
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