Автор |
U D Misra |
Автор |
L M Watson |
Дата выпуска |
1987-10-01 |
dc.description |
Magnesium Kα<sub>3,4</sub> satellite spectra along with the Kα<sub>1,2</sub> diagram line and the Kα' satellite line from magnesium, its oxide, halides, sulphate, acetate and binary alloys with silver, cadmium, indium, tin and antimony have been recorded in direct excitation using a Johann-type crystal spectrometer with a MoS<sub>2</sub> crystal (2d = 12.30 Å). It is found that the chemical environment surrounding the emitting atoms affects the satellite intensity ratio (IKα<sub>4</sub>/IKα<sub>3</sub>) strongly. No obvious trend between the electronegativity differences of the compounds and the intensity ratios of the Kα<sub>4</sub>/Kα<sub>3</sub> satellites is evident. No linear relationship between the satellite intensity ratios (IKα<sub>4</sub>/IKα<sub>3</sub>) and the magnesium content in the alloy is observed as reported by Baun and Fischer for the aluminium system. The origin of the Kα<sub>3</sub> and Kα<sub>4</sub> satellites is discussed. |
Формат |
application.pdf |
Издатель |
Institute of Physics Publishing |
Название |
Kα X-rays from magnesium, some of its compounds and alloys |
Тип |
paper |
DOI |
10.1088/0031-8949/36/4/010 |
Electronic ISSN |
1402-4896 |
Print ISSN |
0031-8949 |
Журнал |
Physica Scripta |
Том |
36 |
Первая страница |
673 |
Последняя страница |
675 |
Аффилиация |
U D Misra; Department of Metallurgy, University of Strathclyde, Glasgow G1 1XN, Scotland, UK |
Аффилиация |
L M Watson; Department of Metallurgy, University of Strathclyde, Glasgow G1 1XN, Scotland, UK |
Выпуск |
4 |