基特峰1米傅立叶变换下铈的分支比

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

摘要

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。
Branching Ratios of Cerium with the Kitt Peak 1m FTS
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.
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