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首页> 外文期刊>The Astrophysical journal >FOURIER TRANSFORM EMISSION SPECTRA OF THE (000)-(000) BAND OF THE λ4051.6 BAND OF C_3
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FOURIER TRANSFORM EMISSION SPECTRA OF THE (000)-(000) BAND OF THE λ4051.6 BAND OF C_3

机译:C_3的λ4051.6能带的(000)-(000)能带的傅里叶变换发射光谱

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The (000)-(000) band of the 4051.6 A group (A ~1∏_u - X-tilde ~1Σ_g~+) of C_3 was recorded in emission with a Bruker IFS 120HR Fourier transform (FT) spectrometer at the University of Waterloo. The band was excited by a microwave discharge in isopropanol (less than a few mtorr) diluted in helium (2 torr). Our new FT data provide more reliable and accurately calibrated transition wavenumbers than those from the grating spectra given by Gausset and co-workers. Analysis of our new spectrum combined with the data by McCall and coworkers confirmed that the lower J levels in the A state were strongly perturbed, as reported by Gausset and coworkers. The unidentified lines observed by McCall and coworkers could be attributed to extra transitions to an unknown perturbing state.
机译:4051.6A组(A〜1∏_u-X-tilde〜1Σ_g〜+)C_3的(000)-(000)谱带是用美国University of University的布鲁克IFS 120HR傅立叶变换(FT)光谱仪记录的。滑铁卢。微波通过在氦气(2托)中稀释的异丙醇(小于几毫托)中的微波放电来激发。与Gausset及其同事提供的光栅光谱相比,我们的新FT数据可提供更可靠,更准确地校准的跃迁波数。根据Gausset及其同事的报告,对我们新光谱的分析与McCall及其同事的数据相结合,证实了A状态下较低的J值受到强烈干扰。麦考尔及其同事观察到的不确定的线可能归因于向未知扰动状态的额外过渡。

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