Branching Ratios of Cerium with the Kitt Peak 1m FTS

S. Bisson, B. Comaskey, J. Conway, C. Haynam, J. Stockdale, E. Worden
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引用次数: 0

Abstract

The emission spectrum of cerium was recorded on the 1m Fourier transform spectrometer (FTS) at the National Solar Observatory, Kitt Peak, AZ., using a 140Ce electrodeless discharge lamp (EDL) as a source. The frequency range 4,000 to 27,600 cm-1 was covered in two runs while maintaining the EDL parameters as constant as possible. Large UV diodes were used as detectors for the 9,100 to 27,600 cm-1 range and In/Sb detectors were used for the 4,000 to 14,300 cm-1 range. The instrument was intensity calibrated for both ranges using standard lamp scans. A multiplication factor obtained from the overlap region was applied to bring the two regions to the same intensity scale.
基特峰1米傅立叶变换下铈的分支比
使用140Ce无极放电灯(EDL)作为光源,在美国亚利桑那州基特峰国家太阳天文台的1m傅里叶变换光谱仪(FTS)上记录了铈的发射光谱。两次入井可以覆盖4000 ~ 27600 cm-1的频率范围,同时尽可能保持EDL参数不变。在9,100至27,600 cm-1范围内使用大型UV二极管作为探测器,在4,000至14,300 cm-1范围内使用In/Sb探测器。仪器使用标准灯扫描对两个范围进行强度校准。利用从重叠区域得到的乘法因子使两个区域达到相同的强度尺度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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