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首页> 外文期刊>Journal of Quantitative Spectroscopy & Radiative Transfer >Spectral line decomposition and frequency shifts in AlHe alpha group emission from laser-produced plasma
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Spectral line decomposition and frequency shifts in AlHe alpha group emission from laser-produced plasma

机译:激光产生等离子体的AlHeα基团发射的谱线分解和频移

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Precise spectroscopic observations of K-shell emission from highly stripped Al ions immersed in dense, constrained-flow laser-produced plasma is reported. By using a vertical dispersion Johann spectrometer, the time-integrated spectra of the Al He alpha group were measured with a high spectral and spatial resolution. The complex spectral profiles modified by the satellite formation, line broadening and frequency shifts were decomposed into individual pseudo-Voigt components by using a code GASPED based on a problem-dependent genetic algorithm. The method uses eight operators tailored to the problem of spectral decomposition and variable-size genomes to fit the data with a varying number of spectral lines. The spectra fitting was based on anticipatory theoretical knowledge of the satellite structure simulated by the multilevel collisional-radiative code MARIA and on an assumption of the aggregate plasma-induced shift of the parent lines and their satellites. The analysis of the spectral profiles revealed systematic red shifts of the resonance and the intercombination lines. Their magnitude is commensurate with predictions of the atomic data and spectral line shape codes combined with the 1D hydrodynamic modeling of the plasma conditions and independent electron density measurements. The results obtained corroborate the feasibility of an accurate decomposition of the spectral profiles encompassing optically thick and thin lines overlapped by a strong satellite emission. (C) 2005 Elsevier Ltd. All rights reserved.
机译:据报道,从高剥离铝离子浸入致密的约束流激光产生的等离子体中,K壳发射出了精确的光谱观察结果。通过使用垂直色散约翰光谱仪,以高光谱和空间分辨率测量了Al He alpha基团的时间积分光谱。通过使用基于问题的遗传算法的代码GASPED,将由卫星编队,线展宽和频移修改的复杂频谱轮廓分解为单个的伪Voigt分量。该方法使用了针对光谱分解和可变大小的基因组的八个运算符,以使数据适应不同数量的光谱线。光谱拟合基于多级碰撞辐射代码MARIA模拟的卫星结构的预期理论知识,并假设母线及其卫星发生了总的等离子体诱发的位移。光谱分布图的分析揭示了共振线和相互结合线的系统性红移。它们的大小与原子数据和光谱线形状代码的预测相结合,并与等离子体条件的一维流体动力学建模和独立的电子密度测量相结合。获得的结果证实了准确分解包括由强卫星发射重叠的光学粗细线的光谱轮廓的可行性。 (C)2005 Elsevier Ltd.保留所有权利。

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