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利用l能级分裂的屏蔽氢模型(SHML)，计算了不同混合比例的Au-Gd混合物在温度为250eV、密度为1g•cm–3的Rosseland平均不透明度。计算值与实验值和理论值吻合得较好。     

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利用SHML模型计算了密度为ρ=1g·cm-3、温度为150eV、200eV、250eV、300eV、400eV的Sn等离子体的随光子能量变化的辐射不透明度及Rosseland平均不透明度.分析了不透明度随光子能量变化曲线的吸收峰值(不透明度峰值)与能级跃迁的对应关系.还将Sn的Rosseland平均不透明度与DCA/UTA及STA模型计算结果作了比较,吻合较好.     

Rosseland Mean Opacity of a High—Z Mixture Palsma

An eight-beam 0.351-μm laser with pulse duration of about 1.0ns and energy of 260J per beam was injcted into a cylindrical cavity to generate intense x-ray radiation on the Shengguang Ⅱ high power laser facility.A mixture foil of gold and gadolinium and a gold foil were attached on portion of a diagnostic hole in the mid-plane of the cavity and ablated by the intense x-ray radiation.The propagating time of the radiation heat wave in the mixture and the pure gold foil were measured with soft-x-ray spectrometer and by adopting space-and time resolved measurement technolgoy,respectively,The results shows that the mixrue of gold and gadolinium has higher Rosseland mean opacity than the gold sample in our experiment.     

Pt等离子体不透明度的理论计算

利用考虑l能级分裂的屏蔽氢离子模型SHML,计算了重核等离子体Pt在密度温度分别为时束缚—束缚、束缚—自由、自由—自由的吸收系数,并由此计算了Pt等离子体随光子能量变化的辐射不透明度.SHML模型计算的辐射不透明度好于SHM模型的计算结果这是肯定无疑的.     

Ne、Ar、Kr、Xe等离子体Planck和Rosseland平均不透明度的近似计算

根据平均原子模型和类氢光吸收系数，近似地计算了Ne、Ar、Kr、Xe等惰性元素高温、高密度等离子体的Planck和Rosseland不透明度。在计算线谱吸收过程中，采用了唯象方法处理线谱演化成谱带时的加宽效应及谱带重叠效应。将不透明度数据拟合成温度和密度的幂函数形式，它能够用于辐射体的数值拟合。     

用STA模型计算Au等离子体的不透明度

 在局部热动平衡条件下,用STA（超组态跃迁阵）模型探索研究和计算Au等离子体在一定温度和密度下的跃迁阵的参数,并用来计算冲击压缩下等离子体的辐射不透明度。     

高温稠密金等离子体辐射不透明度的多极效应

使用平均原子模型研究了电四极及更高阶跃迁对高温稠密金等离子体辐射不透明度的贡献.计算并讨论了在不同温度密度条件下,电四极,电八极,电十六极跃迁对束缚-束缚跃迁的影响.计算了密度为96.405 g/cm3时,不同温度条件下,电四极,电八极跃迁对Rosseland平均不透明度的贡献.考虑了电四极、电八极跃迁后金等离子体不透明度的相对改变最大分别为4.67%和1.5%,并和其它文献的理论结果进行了比较.     

SHML模型计算Sn等离子体的平均离化度

The screened hydrogen-ion model with l splitting is proposed to calculate the average ionization stage (AIS) of Sn plasma in the temperature of 100～2000eV and density of 0.001～10g•cm^-3. The relationships of AIS with density and temperature are given, and the “flat-roof” phenomenon is discussed.     

高密度氩等离子体电子密度的计算

用屏蔽氢离子模型计算了冲击压缩产生的温度T～2.0eV、密度ρ～0.01g/cm3～0.49g/cm3范围内氩等离子体的电子密度,探讨了不同温度、密度范围内的高密度氩等离子体中粒子之间相互作用对电子密度的影响.     

Calculation of the radiative opacity of laser-produced plasmas using a relativistic-screened hydrogenic model

In this work, we use a relativistic-screened hydrogenic model to compute the radiative opacity of laser-produced plasmas. The model is based on a set of screening charges which allow one to easily calculate atomic properties of isolated ions. These screened charges have been fitted to a fourth-order polynomial depending on the nuclear charge Z for ground and single excited states of ions belonging to the isoelectronic sequences comprised between He-like to U-like. In the opacity model used, ionic populations are obtained by solving the Saha equation including degeneracy corrections. Bound-bound transitions are determined using a Voigt profile for line shape, which includes natural, collisional, Doppler and UTA widths. Bound-free and free-free opacities are evaluated using the Kramer cross-sections with appropriate corrections. Scattering processes are computed through the use of the Thomson formula with corrections. The results are compared with other screened hydrogenic models and more sophisticated self-consistent codes.     

Multipole effects to the opacity of hot dense gold plasma

The contributions of the multipole transitions to the opacity of hot dense gold plasma are taken into account by using an average-atom model. The influences of the E2, E3 and E4 transitions on the Rosseland opacity are studied, respectively. Comparisons with Miao’s calculation have been made. It shows that using the Taylor series to account for the multipole transitions is no longer valid since ik · r is not much smaller than the unit when the photon energy goes very high.     

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利用分裂的屏蔽氢不透明度模型计算了Ar、Kr、Xe惰性元素混合物随光子能量变化的不透明度以及Rosseland平均不透明度。研究了温度为100～250eV,密度为0.5～2g·cm-3范围内惰性元素混合物的Rosseland平均不透明度与混合物质、混合比例、温度和密度的密切关系。结果显示,Ar-Xe混合以及Xe-Kr混合后的Rosseland平均不透明度比它们为纯元素时有较大的增加;而Ar-Kr混合后的Rosseland平均不透明度则比纯Kr低。通过对比纯惰性元素随光子能量变化的不透明度峰、谷值,分析了造成混合后不透明度增加或降低的原因,同时给出了获得惰性元素混合物平均不透明度为最大时的混合比例。     

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利用试验势法和平均半径-屏蔽电荷迭代法研究基于解析势的相对论和非相对论屏蔽类氢模型。通过对屏蔽电荷的计算和比较,证实平均半径-屏蔽电荷迭代法无论在效率上还是计算精度上优于试验势法。与More和Faussurier屏蔽类氢模型比较,在电子电离能、离子总能量和电子跃迁能量的计算结果精度方面,基于解析势的相对论性屏蔽类氢模型占有优势。