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The fine structure spectra from very highly stripped ions of the medium and high-Z elements have important applications in plasma diagnostics and the atomic structure calculations. Therefore, on the SG-II laser facility, the X-ray emission spectra from highly stripped plasma of Molybdenum (Mo) are observed by focusing an Nd-glass frequency-tripled (0.35 m) laser beam onto the surface of the Mo target. The fine structure spectra of Mo ions in a range of 0.320.58 nm are measured by a high-resolution elliptically bent crystal spectrometer. Some of resonance transitions and inner-shell transitions of the type 42 and 32 in the C-like, O-like, F-like and Ne-like iso-electronic sequence and the lines from H-like and He-like Mo ions are identified and classified. In addition, the full widths at half maximum (FWHM) of wavelengths are also analyzed. Wavelengths are measured within an uncertainty of 0.0005 nm. A comparison shows that they are in good agreement with computational results of Hartree-Fock-Relativistic (HFR) method. This work is very helpful for enriching the spectra of Mo ions.
[1] Keane C J, Hammel B A, Osterheld A L, Kania D R 1994 Phys. Rev. 72 3029
[2] Yang G H, Zhang J Y, Zhang B H, Zhou Y Q, Li J 2000 Acta Phys. Sin. 49 2389 (in Chinese) [杨国洪, 张继彦, 张保汉, 周裕清, 李军 2000 49 2389]
[3] Skobelev I Y, Faenov A Y, Dyakin V M, Fiedorowicz H, Bartnik A, Szczurek M 1997 Phys. Rev. E 55 3773
[4] Fang Q Y, Yan J 2006 it The Theory of Atomic Structure, Collisions and Spectra (Beijing: National Defence Industry Press) pp402-422 (in Chinese) [方泉玉, 颜君 2006 原子结构、碰撞与光谱理论 (北京: 国防工业出版社) 第402—422页]
[5] Marrs R E, Levine M A, Knapp D A, Henderson J R 1988 Phys. Rev. Lett. 60 1715
[6] Goldstein W H, Walling R S, Bailey J, Chen M H, Fortner R F, Klapisch M, Phillips T, Stewart R E 1987 Phys. Rev. Lett. 58 2300
[7] Keane C J, Hammel B A, Osterheld A L, Kania D R 1994 Phys. Rev. Lett. 72 3029
[8] Bauche-Arnoult C, Bauche J, Klapisch M 1985 Phys. Rev. A 31 2248
[9] Kelly R L 1982 ORNL 5922
[10] Wang R R, Chen W M, Wang W, Dong J Q, Xiao S L 2010 Chin. Phys. B 19 075202
[11] Wang R R, Chen W M, Mao C S, Dong J Q, Fu S Z 2009 Chin. Opt. Lett. 7 156
[12] Zhu T, Zhang J Y, Zhang B H, Yang C W, Yang G H, Yang J M, Li J J 2007 At. Mol. Phys. 24 513 (in Chinese) [朱托, 张继彦, 张保汉, 杨朝文, 杨国洪, 杨家敏, 李军 2007 原子与分子 24 513]
[13] Zhou Y Q, Zhang B H, Lei A L 1995 Phys. Lett. A 204 379
[14] Gao Q, Wu Z Q, Zhang C F, Li Z H, Xu R K, Zu X T 2012 Acta Phys. Sin. 61 015201 (in Chinese) [高启, 吴泽, 张传飞, 李正宏, 徐荣昆, 祖小涛 2012 61 015201]
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[1] Keane C J, Hammel B A, Osterheld A L, Kania D R 1994 Phys. Rev. 72 3029
[2] Yang G H, Zhang J Y, Zhang B H, Zhou Y Q, Li J 2000 Acta Phys. Sin. 49 2389 (in Chinese) [杨国洪, 张继彦, 张保汉, 周裕清, 李军 2000 49 2389]
[3] Skobelev I Y, Faenov A Y, Dyakin V M, Fiedorowicz H, Bartnik A, Szczurek M 1997 Phys. Rev. E 55 3773
[4] Fang Q Y, Yan J 2006 it The Theory of Atomic Structure, Collisions and Spectra (Beijing: National Defence Industry Press) pp402-422 (in Chinese) [方泉玉, 颜君 2006 原子结构、碰撞与光谱理论 (北京: 国防工业出版社) 第402—422页]
[5] Marrs R E, Levine M A, Knapp D A, Henderson J R 1988 Phys. Rev. Lett. 60 1715
[6] Goldstein W H, Walling R S, Bailey J, Chen M H, Fortner R F, Klapisch M, Phillips T, Stewart R E 1987 Phys. Rev. Lett. 58 2300
[7] Keane C J, Hammel B A, Osterheld A L, Kania D R 1994 Phys. Rev. Lett. 72 3029
[8] Bauche-Arnoult C, Bauche J, Klapisch M 1985 Phys. Rev. A 31 2248
[9] Kelly R L 1982 ORNL 5922
[10] Wang R R, Chen W M, Wang W, Dong J Q, Xiao S L 2010 Chin. Phys. B 19 075202
[11] Wang R R, Chen W M, Mao C S, Dong J Q, Fu S Z 2009 Chin. Opt. Lett. 7 156
[12] Zhu T, Zhang J Y, Zhang B H, Yang C W, Yang G H, Yang J M, Li J J 2007 At. Mol. Phys. 24 513 (in Chinese) [朱托, 张继彦, 张保汉, 杨朝文, 杨国洪, 杨家敏, 李军 2007 原子与分子 24 513]
[13] Zhou Y Q, Zhang B H, Lei A L 1995 Phys. Lett. A 204 379
[14] Gao Q, Wu Z Q, Zhang C F, Li Z H, Xu R K, Zu X T 2012 Acta Phys. Sin. 61 015201 (in Chinese) [高启, 吴泽, 张传飞, 李正宏, 徐荣昆, 祖小涛 2012 61 015201]
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