Stark broadening parameters for ion lines of copper
Fundamental atomic parameters are required in many spheres of modern physics and engineering. Particularly, atomic data for spectral lines are widely used in astrophysics, plasma physics and technology, laser engineering. But in many cases there is appreciable lack of such data. Especially, it is re...
Збережено в:
| Дата: | 2003 |
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| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
2003
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| Назва видання: | Вопросы атомной науки и техники |
| Теми: | |
| Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/110608 |
| Теги: |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Stark broadening parameters for ion lines of copper / A.K. Lobko, S.A. Trubchaninov, A.V. Tsarenko // Вопросы атомной науки и техники. — 2003. — № 1. — С. 165-168. — Бібліогр.: 6 назв. — англ. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Резюме: | Fundamental atomic parameters are required in many spheres of modern physics and engineering. Particularly, atomic data for spectral lines are widely used in astrophysics, plasma physics and technology, laser engineering. But in many cases there is appreciable lack of such data. Especially, it is refer to ions of heavy elements. Apparently experiment is the only possible source of reliable data in this situation. During last years a number of experiments were carried out with quasi-steady-state plasma accelerator QSPA Kh-50. This scientific activity was related to the physics of plasma accelerating, development of diagnostic techniques of dense plasma, modeling experiments, and applied problem. This work represents the first attempt to apply plasma-target interaction investigations for solving the problems of the atomic physics, particularly determination of fundamental constants – Stark widths and shifts. Experimental data on Stark broadening parameters for some CuII and CuIII spectral lines in the range of 220nm-600nm are offered. |
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