实验曲线反褶积的一种实用方法

A. Jones, D. L. Misell
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引用次数: 34

摘要

本文给出了实验光谱失真后的一般校正方法,其中F(x)为观测光谱,F(x)为真实剖面,S(x)为狭缝函数或本征展宽函数。该方法应用于实际中遇到的三种主要缝函数类型,即指数分布、高斯分布和柯西分布。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A practical method for the deconvolution of experimental curves
A general method is given for the correction of experimental spectra when they have been distorted according to the convolution integral described, where F(x) is the observed spectrum, f(x) is the true profile and S(x) is the slit function or intrinsic broadening function. The method is applied to the three main types of slit functions which are encountered in practice, namely the exponential, Gaussian and Cauchy distributions.
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