期刊文献+
共找到7篇文章
< 1 >
每页显示 20 50 100
Non-LTE恒星大气模型完全线性化原理
1
作者 赵定烽 陈子栋 《甘肃科学学报》 2000年第2期28-34,共7页
通过对 Non- LTE的平面平行状恒星大气结构的数值模型完全线性化方法工作原理的介绍 ,阐述了恒星大气理论的工作原理和一般方法 。
关键词 恒星 non-ltE大气数值模型 完全线性化 大气结构
下载PDF
恒星大气中Li的non-LTE效应研究进展
2
作者 张晓宇 施建荣 赵刚 《天文学进展》 CSCD 北大核心 2008年第1期15-26,共12页
Li元素是性质非常活跃且易发生核反应的轻核元素。其精确的丰度可以检验宇宙大爆炸学说。Li元素在宇宙早期化学演化、元素核合成理论和恒星的结构与演化研究中都有着非常重要的地位。近几年来,人们逐渐认识到在局部热动平衡(LTE)的假设... Li元素是性质非常活跃且易发生核反应的轻核元素。其精确的丰度可以检验宇宙大爆炸学说。Li元素在宇宙早期化学演化、元素核合成理论和恒星的结构与演化研究中都有着非常重要的地位。近几年来,人们逐渐认识到在局部热动平衡(LTE)的假设下不能准确得到Li丰度,特别在冷的矮星中非局部热动平衡(non-LTE)效应的影响不容忽视。随着理论的发展,人们对原子参数有了更深入的了解,对non-LTE效应的研究也更趋成熟。确定元素丰度时考虑non-LTE影响已成为主要趋势。该文分析了影响Li元素non-LTE效应的各种机制,介绍了确定Li元素non-LTE效应的重要参数及Li原子模型的发展历程,最后对Li在各类恒星中的non-LTE效应进行了综合分析。 展开更多
关键词 non-ltE效应 Li原子数据 谱线形成 Li丰度
下载PDF
处理Non-LTE谱线覆盖效应的有效方法——近似A算子法
3
作者 吴关钱 《天文研究与技术》 CSCD 1990年第2期44-50,共7页
本文在分析完全线性化方法不能很好地处理Non-LTE谱线覆盖效应的基础上,介绍了一种由Werner(1986年)引进的能有效的处理Non-LTE谱线覆盖效应的计算Non-LTE恒星大气模型的方法——近似A算子法。并对这种方法的优缺点和可能的应用作了分... 本文在分析完全线性化方法不能很好地处理Non-LTE谱线覆盖效应的基础上,介绍了一种由Werner(1986年)引进的能有效的处理Non-LTE谱线覆盖效应的计算Non-LTE恒星大气模型的方法——近似A算子法。并对这种方法的优缺点和可能的应用作了分析和讨论。 展开更多
关键词 谱线覆盖 non-ltE 子法 恒星大气 近似解 线性化方法 近似算子 Werner 光学深度 非线性方程组
下载PDF
两种日珥光谱分析方法的比较
4
作者 张其洲 方成 《南京大学学报(自然科学版)》 CAS CSCD 1990年第4期588-595,共8页
本文将完全线性化方法同非局部热动平衡计算方法进行了比较,考察了用完全线性化方法确定光谱参数的可靠性,并研究了光谱分析中经常用的“共空间发射”等假设的合理性。本文研究结果表明,用完全线性化方法可以唯一确定谱线多普勒宽度,线... 本文将完全线性化方法同非局部热动平衡计算方法进行了比较,考察了用完全线性化方法确定光谱参数的可靠性,并研究了光谱分析中经常用的“共空间发射”等假设的合理性。本文研究结果表明,用完全线性化方法可以唯一确定谱线多普勒宽度,线心光学厚度和源函数线性变化系数,其中多普勒宽度和源函数线性变化系数反映了日珥中H_a和CaⅡH. K线线翼附近所对应形成区的物理状况。H_a线同C_aⅡ H. K线是共空间发射的,从共空间发射求出的温度反映了日珥中上述区域的运动温度。本文结果还表明,一般来说,日珥中CaⅢ粒子数大于CaⅡ粒子数,从CaⅡ H、K线求氢原子密度必须考虑两次电离钙的贡献。 展开更多
关键词 太阳 日珥 光谱分析 non-ltE
下载PDF
Parameterization of the Non-Local Thermodynamic Equilibrium Source Function with Chemical Production by an Equivalent Two-Level Model
5
作者 Xun ZHUThe Johns Hopkins University Applied Physics Laboratory, MD 20723-6099, USA 《Advances in Atmospheric Sciences》 SCIE CAS CSCD 2003年第4期487-495,共9页
The classic two-level or equivalent two-level model that includes only the statistical equilibrium of radiative and thermal processes of excitation and quenching between two vibrational energy levels is extended by ad... The classic two-level or equivalent two-level model that includes only the statistical equilibrium of radiative and thermal processes of excitation and quenching between two vibrational energy levels is extended by adding chemical production to the rate equations. The modifications to the non-local thermodynamic equilibrium source function and cooling rate are parameterized by &#981;<SUB>c</SUB>, which characterizes the ratio of chemical production to collisional quenching. For applications of broadband emission of O<SUB>3</SUB> at 9.6 &#956;m, the non-LTE effect of chemical production on the cooling rate and limb emission is proportional to the ratio of O to O<SUB>3</SUB>. For a typical [O]/[O<SUB>3</SUB>], the maximum enhancements of limb radiance and cooling rate are about 15%–30% and 0.03–0.05 K day<SUP>&#8722;1</SUP>, respectively, both occurring near the mesopause regions. This suggests that the broadband limb radiance above &#8764;80 km is sensitive to O<SUB>3</SUB> density but not sensitive to the direct cooling rate along the line-of-sight, which makes O<SUB>3</SUB> retrieval feasible but the direct cooling rate retrieval difficult by using the O<SUB>3</SUB> 9.6 &#956;m band limb emission. 展开更多
关键词 non-ltE radiative transfer ozone cooling ozone retrieval space weather
下载PDF
Opacity calculations for Non-Local-Thermodynamic-Equilibrium plasmas
6
作者 逄锦桥 WU Ze-qing +1 位作者 YAN Jun HAN Guo-xing 《原子与分子物理学报》 CAS CSCD 北大核心 2004年第B04期169-171,共3页
In this paper, we presented a method to calculate the spectral-resolved opacity for Non-Local-Thermodynamic-Equilibrium (non-LTE) plasmas. By solving the rate equations, we get the population. In the rate equations, c... In this paper, we presented a method to calculate the spectral-resolved opacity for Non-Local-Thermodynamic-Equilibrium (non-LTE) plasmas. By solving the rate equations, we get the population. In the rate equations, configuration-averaged rate coefficients are used and the cross sections are calculated based on the first-perturbation theory. Using the detailed configuration accounting with the term structures treated by the unresolved transition array model, we calculated the spectral-resolved opacity of Al plasmas. The results are compared with those of other theoretical models. From the comparison, we can see that the present results fit well with other models for low-Z plasmas. For high-Z plasmas, we will give detailed discussion in the future. 展开更多
关键词 OPACITY Non-local-thermodynamic-equilibrium (non-ltE) Unresolved-transition-array(UTA)
下载PDF
Investigation on non-LTE radiation emitted from a laser-irradiated Au disk
7
作者 GU Peijun PEI Wenbing FENG Tinggui WU Changshu 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2005年第3期345-360,共16页
The spectral character of X-ray emitted from laser-irradiated gold disk is studied by using the one-dimensional non-LTE multigroup radiation transport hydrodynamics code RDMG. The applicability of the “three-temperat... The spectral character of X-ray emitted from laser-irradiated gold disk is studied by using the one-dimensional non-LTE multigroup radiation transport hydrodynamics code RDMG. The applicability of the “three-temperature” model in which the radiation is described with thermal conduction approximation is checked. The simulation results show that the X-ray emitted from the laser-produced gold plasma is in non-LTE, and that the atom model has significant effect on the structure of X-ray spectrum. However, the plasma states, laser absorption efficiency and X-ray conversion efficiency, which are calculated with the “three-temperature” model, are almost the same as those with non-LTE multigroup radiation transport model. This fact indicates that the “three-temperature” model can be used to study plasma states and the energy distributions produced by a laser-irradiated high-Z target. This is meaningful to the 2-D or 3-D simulation. 展开更多
关键词 laser-irradiated Au target the state of plasma X-ray non-ltE radiation ATOM model.
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部