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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment >Transverse coherence properties of X-ray beams in third-generation synchrotron radiation sources
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Transverse coherence properties of X-ray beams in third-generation synchrotron radiation sources

机译:第三代同步加速器辐射源中X射线束的横向相干特性

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This article describes a complete theory of spatial coherence for undulator radiation sources. Current estimations of coherence properties often assume that undulator sources are quasi-homogeneous, like thermal sources, and rely on the application of the van Cittert-Zernike theorem for calculating the degree of transverse coherence. Such assumption is not adequate when treating third generation light sources, because the vertical (geometrical) emittance of the electron beam is comparable or even much smaller than the radiation wavelength in a very wide spectral interval that spans over four orders of magnitude (from 0.1 up to 10~3 A). Sometimes, the so-called Gaussian-Schell model, that is widely used in statistical optics in the description of partially coherent sources, is applied as an alternative to the quasi-homogeneous model. However, as we will demonstrate, this model fails to properly describe coherent properties of X-ray beams from non-homogeneous undulator sources. As a result, a more rigorous analysis is required. We propose a technique, based on statistical optics and Fourier optics, to explicitly calculate the cross-spectral density of an undulator source in the most general case, at any position after the undulator. Our theory, that makes consistent use of dimensionless analysis, allows relatively easy treatment and physical understanding of many asymptotes of the parameter space, together with their region of applicability. Particular emphasis is given to the asymptotic situation when the horizontal emittance is much larger than the radiation wavelength, and the vertical emittance is arbitrary. This case is practically relevant for third generation synchrotron radiation sources.
机译:本文介绍了波动波辐射源空间相干性的完整理论。当前对相干性的估计通常假设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。在处理第三代光源时,这种假设是不充分的,因为在跨越四个数量级(从0.1向上)的非常宽的光谱区间中,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。至10〜3 A)。有时,所谓的高斯-谢尔模型(Gaussian-Schell model)在准相干模型的描述中被广泛使用于统计光学中,用于描述部分相干光源。但是,正如我们将要演示的那样,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上,显式计算波动器源的交叉谱密度。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区域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时,则特别要注意渐近情况。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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