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Cauchois and Senemaud Tables of wavelengths of X-ray emission lines and absorption edges

机译:X射线发射线和吸收边的波长的Cauchois和Senemaud表

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We present the Cauchois and Senemaud Tables of X-ray emission lines and absorption edges. They are written both in French and English. They were published in 1978 by Pergamon Press and are insufficiently known. However they are of large interest because of their completeness. They comprise the energies of all the K, L, M, N and O emission lines of natural elements from lithium up to uranium as well as the energies of satellite emissions and absorption discontinuities. The more intense lines of radio-elements up to fermium (Z = 100) are also given. The Tables range from the hard X-rays (122 keV, 0.01 nm) to the extreme ultra-violet (12 eV, 102 nm). For each transition, thewavelength (A and uX) and energy (eV and Ry) are given and references are indicated. The transitions are grouped by increasing wavelength (decreasing photon energy) and also by element and spectral series.We present, as an example, the use of the Tables to identify the emissions of the molybdenum L spectrum.Wedecided to scan the Cauchois and S′en′emaud Tables and make them available for the scientific community. They are now available at the Website of our laboratory, http://www.lcpmr.upmc.fr/.
机译:我们介绍了X射线发射线和吸收边的Cauchois和Senemaud表。它们以法语和英语编写。它们是由Pergamon Press于1978年出版的,鲜为人知。但是,由于它们的完整性,它们引起了极大的兴趣。它们包括从锂到铀的自然元素的所有K,L,M,N和O发射谱线的能量,以及卫星发射和吸收不连续的能量。还给出了直至fer(Z = 100)的更强的无线电元素线。这些表的范围从硬X射线(122 keV,0.01 nm)到极端紫外线(12 eV,102 nm)。对于每个跃迁,给出了波长(A和uX)和能量(eV和Ry)并指出了参考。这些跃迁按波长增加(光子能量减少)以及元素和光谱系列进行分组。我们以表格为例说明钼L光谱的发射,决定扫描Cauchois和S'编入表格并提供给科学界使用。现在可以在我们实验室的网站http://www.lcpmr.upmc.fr/上找到它们。

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