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Fourier Transform Blackbody Spectroscopy: Towards Thermodynamic Temperature Measurement

机译:傅立叶变换黑体光谱:朝热力学温度测量

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The concept of basing a temperature scale on a wavelength standard was introduced by Gebbie almost 30 years ago, in a proposal to use Fourier-transform spectroscopy to measure the emission from blackbody sources operated at a series of different temperatures. At the National Research Council of Canada, we have embarked on a project to investigate the feasibility of this idea. Experimental and theoretical results will be shown describing an interpolation technique for obtaining temperature information for intermediate settings of the source, when the highest and lowest spectra are assumed fixed and known. The ratio technique which combines spectra three at a time is then considered as a candidate for determining a self-consistent solution which can calculate the temperatures of all of the data, thus eliminating the requirement for the two calibration points. Work with real and simulated data is presented to explore some of the difficulties faced when attempting to determine absolute thermodynamic temperature in this way.
机译:Gebbie差不多30年前引入了基于波长标准对波长标准的温度级的概念,在使用傅立叶变换光谱法测量在一系列不同温度下操作的黑体来源的发射。在加拿大国家研究委员会,我们已经开始了一个项目来调查这个想法的可行性。将示出实验和理论结果,描述用于获得源的中间设置的温度信息的插值技术,当假定最高和最低光谱和已知的频谱时。然后将Spectra三次组合的比率技术被认为是用于确定可以计算所有数据的温度的自我一致解的候选,从而消除了两个校准点的要求。使用真实和模拟数据的工作,以探讨尝试以这种方式确定绝对热力学温度时面临的一些困难。

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