Kα Satellite Lines

خطوط Kα التابعة

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ID: 269883
1936
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Abstract
With a two-crystal vacuum spectrometer, ionization curves of the $K{\ensuremath{\alpha}}_{3, 4}$ group of x-ray satellite lines have been recorded for elements S(16) to Ge(32). In the $K{\ensuremath{\alpha}}_{3, 4}$ satellite group are found five component lines for $16\ensuremath{\le}Z\ensuremath{\le}28$ and four components for $29\ensuremath{\le}Z\ensuremath{\le}32$. The wave-length position, relative intensity, and line width at half-maximum intensity of each satellite component has been measured. The widths and shapes of the $K{\ensuremath{\alpha}}_{1, 2}$ lines were determined and a brief discussion of these data is given.
باستخدام مطياف تفريغ ثنائي البلورة، سُجِّلت منحنيات التأين لمجموعة خطوط الساتل للأشعة السينية $K{\ensuremath{\alpha}}_{3, 4}$ للعناصر من S(16) إلى Ge(32). ووُجد في مجموعة ساتل $K{\ensuremath{\alpha}}_{3, 4}$ خمسة خطوط مكوِّنة في النطاق $16\ensuremath{\le}Z\ensuremath{\le}28$ وأربعة مكوِّنات في النطاق $29\ensuremath{\le}Z\ensuremath{\le}32$. كما قِيس موضع الطول الموجي، والشدة النسبية، وعرض الخط عند نصف الشدة القصوى لكل مكوِّن من مكوِّنات الساتل. وحُدِّدت عروض وأشكال خطوط $K{\ensuremath{\alpha}}_{1, 2}$، وقُدِّمت مناقشة موجزة لهذه البيانات.
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parratt1936physicalkα Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Lyman G. Parratt
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Journal physical review
Year 1936
DOI
doi:10.1103/PhysRev.50.1
URL
https://doi.org/10.1103%2FPhysRev.50.1
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