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Titlebook: Vth International Congress on X-Ray Optics and Microanalysis / V. Internationaler Kongre? für R?ntge; Tübingen, September G. M?llenstedt,K

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樓主: GALL
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發(fā)表于 2025-3-23 13:34:30 | 只看該作者
12#
發(fā)表于 2025-3-23 16:28:47 | 只看該作者
Untersuchung zur ASR (Anomalous Surface Reflection) von R?ntgenstrahlen mit einer Mikrofokus-R?ntgentierte R?ntgenstrahlung das aus dem sichtbaren Spektralgebiet bekannte Reflexionsgesetz . erfüllt. Ist das erste Medium Luft, dann ist im Wellenl?ngengebiet der R?ntgenstrahlen der Brechungsindex des zweiten Mediums stets kleiner als 1, und es kann bei hinreichend schwacher Absorption des zweiten Me
13#
發(fā)表于 2025-3-23 19:32:36 | 只看該作者
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發(fā)表于 2025-3-24 01:21:47 | 只看該作者
Application of X-Ray Optical Methods in Solar Astronomyious theoretical work on solar X-rays by G. . of Tübingen University and by experimental work of the microminiaturisation group of the Institute of Applied Physics who could provide Fresnel-Microzoneplates [1] for soft X-ray optics.
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發(fā)表于 2025-3-24 02:44:31 | 只看該作者
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發(fā)表于 2025-3-24 07:35:59 | 只看該作者
Principles and Limitations of Electron Probe Microanalysis] that each element in the periodic table is characterised by a relatively simple X-ray spectrum. The basic experimental arrangement is outlined in Fig. 1. An electron beam (.) of moderate energy (5–40 kV) is directed on to the sample (.) to be investigated, in vacuo, and the X-rays (.) emitted from
17#
發(fā)表于 2025-3-24 14:40:37 | 只看該作者
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發(fā)表于 2025-3-24 15:53:39 | 只看該作者
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發(fā)表于 2025-3-24 22:23:01 | 只看該作者
A Study of the Deadtime Correction in Electron Probe Microanalysiserrors in the measured relative X-ray intensity ratio, ., which often are of the same magnitude as the precision in the determination of .; even greater errors will result when analyzing dilute alloys while using pure element standards ., . and . [1] developed a simple method of determining the dead
20#
發(fā)表于 2025-3-25 00:06:53 | 只看該作者
The Measurement of Total Mass per Unit Area and Elemental Weight-Fractions along Line Scans in Thin servations of characteristic line intensities with simultaneous observations of the bremsstrahlung. The bremsstrahlung counting rate also provides a means to subtract background instantaneously from a characteristic peak, with no need for background measurements off the Bragg angle, thus permitting
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