短脉冲驱动下膨胀冷却等离子体中软X射线激光研究

在解析求解等离子体流体力学方程组的基础上，数值求解了以ＭｇＸＩ为主体的等离子体能级占据数速率方程，进而给出了短脉冲驱动下膨胀冷却等离子体中ＭｇＸＩｌｓ３ｄ－ｌｓ４ｆ激光跃迁增益系数的时空分布，讨论了泵浦激光脉冲宽度对增益的影响。 关键词：     

水窗波段附近激光等离子体X光辐射产生的途径

讨论了利用激光等离子体产生水窗波段Ｘ光辐射的可能途径。靶材，即原子序数的选取是决定产生这一波段辐射的基本因素，利用激光等离子体的平衡态和非平衡态特性都可在水窗波段产生亮度Ｘ光辐射，提出利用黑体辐射来实现水窗波段Ｘ光显微成像研究的方案。     

等离子体波导中的复合X射线激光

短脉冲强激光和气体靶相互作用可产生等离子体波导。利用自相似模型，得到了等离子体波导中等离子体参数的时空演化。利用自编制的程序，以类Ｈｅ氮为例，研究了在这种等离子体波导中，产生复合机制Ｘ射线激光的过程。研究表明，在等离子体波导中有可能产生复合机制Ｘ射线激光，从而有可能利用等离子波导获得大ＧＬ值的复合机制Ｘ射线激光     

线状等离子体测量中的晶体谱仪及其在X射线激光实验中的应用

本文讨论了两种适用于Ｘ射线激光实验的聚焦型弯晶谱仪和针孔晶体谱仪。给出了弯晶谱仪的设计参数，以及针孔晶体谱仪在实验中摄得的线状Ｍｇ和ＣａＦ２等离子体空间分辨谱；分析了晶体谱仪在Ｘ射线激光实验中的应用。     

利用人工神经网络进行激光等离子体诊断

利用前馈神经网络对激光等离子体打靶实验中所得的Ｘ光光谱数据进行处理，可以方便地球出等离子体的电子温度和电子密度等参数。在对网络的训练时采用误差信号反向传输算法，训练后的神经网络能够有效地对Ｘ光光谱数据进行处理，文中给出了用此法算出的Ｍｇ等离子体电子温度和电子密度的空间分布轮廓，与用传统方法所得的结果完全吻合。     

用网格衰减膜相对标定SIOFM─5FW软X光底片

点聚焦激光等离子体发出的Ｘ射线经晶体色散形成均匀的单色Ｘ射线源，在此基础上，用单层网格作为衰减膜，得到未经衰减和经过衰减的Ｘ射线谱，对无保护膜ＳＩＯＦＭ５ＦＷ软Ｘ光底片作了试验性的相对标定，得到了０．９１ｎｍ波长的特性曲线     

用网格衰减膜相对标定SIOFM—5FW软X光底片

点降焦激光等离子体发出的Ｘ射线经晶体色散形成均匀的单色Ｘ射线源，在此基础上，用单层网格作为衰减膜，得到未经衰减和经过衰减的Ｘ射线谱，对无保护膜的ＳＩＯＦ－Ｍ５ＦＷ软Ｘ光底片作了试验性的相对标定，得到了０．９１ｎｍ波长的特性曲线。     

等离子体波导的复合X射线激光

短脉冲强激光和气体革相互作用可产生等离子体波导。利用自相似模型，得到了等离子体波导中等离子体参数的时人演化。利用自编制的程序，以类Ｈｅ氮为例，研究了在这种等离子体波导中，产生复合机制Ｘ射线激光的过程。     

吸气式激光推进中激光能量沉积过程的数值模拟

 结合辐射输运方程,在流体力学方程组的能量方程中加入包括空气吸收的激光能量以及高温气体向周围辐射损失的能量源项,转化为辐射流体力学方程组,建立了用于模拟吸气式激光推进中能量沉积过程的物理力学模型和计算方法。该辐射流体力学计算程序可以很好地模拟激光能量沉积过程中空气对激光能量的吸收、等离子体对激光的屏蔽作用以及激光维持的爆轰波的传播规律,计算得到激光能量的沉积效率约为57%,激光维持的爆轰波的传播速度与同等条件下的理论和实验结果吻合得较好。     

MgF2晶体的激光损伤与加固研究

报道了ＭｇＦ２晶体１．０６μｍ激光损伤阈值和损伤形貌。研究了用ＣＯ２、ＸｅＣｌ和Ｃｕ蒸气三种不同的激光对ＭｇＦ２进行激光预辐照加固和酸腐蚀加固。结果表明，Ｃｕ蒸气激光加固效果最佳，蕨是酸腐蚀和ＸｅＣｌ激光预辐照，并对加固机理进行了分析。     

强激光天体物理学研究——在强激光实验室中模拟某些天体物理过程(Ⅰ)

用激光等离子体相互作用对天体物理过程进行模拟研究已成为当前世界物理和天文学家深感兴趣的重要前沿领域 .文章比较了强激光作用下产生的等离子体与天体物理条件下的等离子体之间在内部物理过程的相似性 ,论述了由前者模拟后者的物理依据 ,即相似性原则和定标规律 .在此基础上 ,回顾和评述了当前已经在高离化态光谱学、类天体等离子体状态方程和辐射不透明度以及流体动力学不稳定性等方面开展的强激光天体物理学的研究 ,这些研究对于理解超新星、白矮星、中子星以及巨行星、褐矮星等领域的天体物理过程起到了极大的作用 ,并正在成为联系天体物理理论模拟和观测的中间桥梁     

Picosecond x-ray laser interferometry of dense plasmas

We present the first results from picosecond interferometry of dense laser-produced plasmas using a soft x-ray laser. The picosecond duration and short wavelength of the 14.7 nm Ni-like Pd laser mitigates effects associated with motion blurring and refraction through millimeter-scale plasmas. This enables direct measurement of the electron-density profile to within 10 microm of the target surface. A series of high-quality two-dimensional (2D) density measurements provide unambiguous characterization of the time evolution in a fast-evolving plasma suitable for validation of existing 1D and 2D hydrodynamic codes.     

强激光天体物理学研究

用激光等离子体相互作用对天体物理过程进行模拟研究已成为当前世界物理和天文学家深感兴趣的重要前沿领域.文章比较了强激光作用下产生的等离子体与天体物理条件下的等离子体之间在内部物理过程的相似性,论述了由前者模拟后者的物理依据,即相似性原则和定标规律.在此基础上,回顾和评述了当前已经在高离化态光谱学、类天体等离子体状态方程和辐射不透明度以及流体动力学不稳定性等方面开展的强激光天体物理学的研究,这些研究对于理解超新星、白矮星、中子星以及巨行星、褐矮星等领域的天体物理过程起到了极大的作用,并正在成为联系天体物理理论模拟和观测的中间桥梁.     

Spectroscopic studies of plasmas produced from thin foils by fast risetime nanosecond laser pulses

Studies of emission spectra in the region 20–250 ? from plasmas produced from thin foils of various materials 6?Z?26 by fast risetime nanosecond laser pulses are reported. Ionization and recombination occuring in these plasmas as deduced from the identification of the spectral lines and their intensities is discussed. Estimates of the plasma temperature are made. The results are compared with the predictions of a computer code based on a thermal wave model for the initial burn through the foil and subsequent hydrodynamic expansion of the plasma.     

Nonlinear dynamics of surface dust vortex and dust zonal flow systems

We present analytical and simulation studies of highly resolved dust fluid flows involving nonlinearly coupled incompressible surface dust vortex modes (SDVMs) and dust zonal flows (DZFs) in nonuniform unmagnetized dusty plasmas. For this purpose, we use the hydrodynamic equations for the dust fluid and Boltzmann distributed electrons and ions and obtain a set of equations that exhibit nonlinear couplings between the SDVMs and DZFs. The nonlinear equations are then used to investigate the parametric excitation of DZFs by the Reynolds stresses of the SDVMs. Large scale SDVMs emerge through nonlinear interactions with DZFs, and they suppress the dust particle transport across the density gradient. In contrast, DZFs possess short scale vortices with a higher turbulent transport. The relevance of our investigation into the role of coherent structures in a nonuniform dusty plasma is discussed.     

MgXI等离子体软X射线自发辐射放大增益的数值模拟

本文采用碰撞辐射模型,考虑MgX,MgXII,MgXIII的基态及MgXI主量子数n≤6到光谱项层次的21个能级,假定等离子体电子温度按高斯函数随时间下降,用初始温度下定态能级占据数速率方程的解作初值,求解瞬态能级占据数速率方程,根据各能级粒子数的时间分布分析了MgXI1s3p—1s4d,1s3d—1s4f跃迁的自发辐射放大增益系数的时间特性。     

有质动力和静电分离场对激光等离子体流体力学状态的影响

利用建立在欧拉坐标系上的一维电子_离子双流双温流体力学程序, 模拟了超短脉冲强激光 (1×1015W/cm2, 150fs)与线性密度梯度等离子体相互作用的流体力学过程. 模拟结果显示，入射激光与临界密度面的反射光叠加，在临界密度以下区域形成局域驻波， 产生的强有质动力在低密区驱动电子形成周期性密度结构——Bragg光栅，激光的反射被增 强. 临界密度处有质动力将等离子体分成向内和向外运动的两部分. 由于离子所受的有质动 力和热压强的梯度力远小于电子，体系产生了强静电分离场，离子的运动主要由该静电分离 场决定. 对双流双温模型和单流双温模型的模拟结果进行了比较. 当有质动力和热压强梯度 力较大时，两种模型对等离子体流体力学状态的描述有明显差异，单流双温模型无法描述此 时的流体力学状态. 关键词： 有质动力 密度调制 双流双温流体力学模型 单流模型     

Laser-Generated Plasmas as X-Ray Sources in the keV-Range

This report will give an introduction to the X-line emission processes in laser-generated plasmas according to a plasma physical point of view. After a short discussion of the experimental results using laser pulses in the range of ? 10 J and irreadiances of 1 to 100 MW/cm² and of first conclusions about the temperature scaling and the dependence of the emission concerning the atomic number of the target material some models of laser-generated plasmas are analysed. The simple hot-spot model neglects any hydrodynamics and only solves for the rate equations. We discuss the underlying collisional-radiative model and evaluate the numerical results of a more complete model for the spatial and temporal plasma evolution including the hydrodynamics. The applications of such plasmas as small, strong, short sources of X-rays in the keV range is discussed with regard to the lithographic replication of sub-μm structures and to the EXAFS spectroscopy. Laser-generated plasmas are compared with conventional X-ray tubes (with rotating anode) and with synchrotrons. The question of amplified spontaneous emission in the XUV range (superradicant X-ray sources) is only shortly touched upon. In conclusion some comments are given to the recoil momentum effects of the ablating plasma on the target are given (rocket model).     

Few-cycle relativistic solitons in plasmas

A set of exact one-dimensional solutions to coupled nonlinear equations describing the propagation of a relativistic ultrashort circularly polarized laser pulse in a cold collisionless and bounded plasma where electrons have an initial velocity in the laser propagating direction is presented. The solutions investigated here are in the form of quickly moving envelop solitons at a propagation velocity comparable to the light speed. The features of solitons in both underdense and overdense plasmas with electrons having different given initial velocities in the laser propagating direction are described. It is found that the amplitude of solitons is larger and soliton width shorter in plasmas where electrons have a larger initial velocity. In overdense plasmas, soliton duration is shorter, the amplitude higher than that in underdense plasmas where electrons have the same initial velocity.