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Transverse coherence properties of X-ray beams in third-generation synchrotron radiation sources

机译:第三代X射​​线束的横向相干特性   同步辐射源

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摘要

This article describes a complete theory of spatial coherence for undulatorradiation sources. Current estimations of coherence properties often assumethat undulator sources are quasi-homogeneous, like thermal sources, and rely onthe application of the van Cittert-Zernike theorem for calculating the degreeof transverse coherence. Such assumption is not adequate when treating thirdgeneration light sources, because the vertical(geometrical) emittance of theelectron beam is comparable or even much smaller than the radiation wavelengthin a very wide spectral interval that spans over four orders of magnitude (from0.1 Angstrom up to 10^3 Angstrom). Sometimes, the so-called Gaussian-Schellmodel, that is widely used in statistical optics in the description ofpartially-coherent sources, is applied as an alternative to thequasi-homogeneous model. However, as we will demonstrate, this model fails toproperly describe coherent properties of X-ray beams from non-homogeneousundulator sources. As a result, a more rigorous analysis is required. Wepropose a technique, based on statistical optics and Fourier optics, toexplicitly calculate the cross-spectral density of an undulator source in themost general case, at any position after the undulator. Our theory, that makesconsistent use of dimensionless analysis, allows relatively easy treatment andphysical understanding of many asymptotes of the parameter space, together withtheir region of applicability. Particular emphasis is given to the asymptoticsituation when the horizontal emittance is much larger than the radiationwavelength, and the vertical emittance is arbitrary. This case is practicallyrelevant for third generation synchrotron radiation sources.
机译:本文介绍了波动辐射源空间相干性的完整理论。当前对相干特性的估计通常假定波动源与热源一样是准均质的,并且依赖于van Cittert-Zernike定理的应用来计算横向相干度。当处理第三代光源时,这种假设是不充分的,因为在跨越四个数量级(从0.1埃到最大)的非常宽的光谱间隔中,电子束的垂直(几何)发射率与辐射波长相当,甚至比辐射波长小得多。 10 ^ 3埃)。有时,所谓的高斯-谢尔模型(Gaussian-Schellmodel)在准相干源的描述中广泛用于统计光学中,被用作准均一模型的替代方法。但是,正如我们将要证明的那样,该模型无法正确描述来自非均匀波源的X射线束的相干特性。结果,需要更严格的分析。我们提出一种基于统计光学和傅立叶光学的技术,在最一般的情况下,在波动器之后的任何位置,明确计算波动源的交叉谱密度。我们一贯使用无量纲分析的理论允许对参数空间的许多渐近线及其适用范围进行相对轻松的处理和物理理解。当水平发射率远大于辐射波长,而垂直发射率是任意的时,则特别强调渐近状态。这种情况实际上与第三代同步加速器辐射源有关。

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