热电子,双离子成分对离子漂移回旋不稳定性的影响

分析了热电子、温离子成分对离子漂移回旋不稳定性的影响，给出了临界稳定热电子成分值α与温离子成分值班出子温度比和离子抗磁漂移速度的关系；讨论了热电子、温、冷离子成分对不稳定性各谐频分支的影响；分析了热电子成分稳定作用的物理机制。     

电子-离子碰撞对超热电子影响的PIC模拟计算

超热电子-离子的产生和输运在传统的ICF方案和“快点火”方案中都是很重要的问题.讨论了电子-离子碰撞对参量不稳定性产生超热电子的过程和超热电子输运过程的影响.指出电子-离子弱碰撞项的加入增强了碰撞吸收,提高了热电子温度,降低了静电波破裂时的场能.这些改变了超热电子的总能量和分布,使之更集中于静电波的相速;电子-离子碰撞的存在还增强了自洽电场,阻碍了超热电子的输运,同样也是超热电子能量下降的原因之一.同时,为确保计算结果的可靠,讨论了初条件对PIC模拟计算的影响,指出空间位置随机热启动容易引入非物理因素,对 关键词：     

啁啾展宽激光脉冲的有限带宽效应对参量不稳定性及超热电子的抑制

 若驱动激光的相干时间小于不稳定性增长时间,则有可能直接控制参量不稳定性。研究了有限带宽的啁啾展宽脉冲对等离子体冕区参量不稳定性及超热电子的抑制效果,给出解析分析及用PIC程序数值模拟结果,考察了电子－离子碰撞对超热电子的影响。     

热电子与热离子共存时的电荷裸露效应

本文采用简晰的平板模型，在局域近似下讨论了热电子，热离子共存时它们对低频交换模的影响，分析了两种热成分电荷裸露效应的相互作用。     

啁啾展宽激光脉冲的有限带宽效应对参量不稳定性及超热电子的抑制

若驱动激光的相干时间小于不稳定性增长时间,则有可能直接控制参量不稳定性。研究了有限带宽的啁啾展宽脉冲对等离子体晚区参量不稳定性及超热电子的抑制效果,给出解析分析及用ＰＩＣ程序数值模拟结果,考察了电子一离子磁拦对超热电子的影响。     

极高β等离子体中由电子温度各向异性引起的不稳定性

用数值方法研究了电子速度分布为双麦克斯韦分布的极高β等离子体的动力学不稳定性,考虑了离子热效应、离子漂移运动、少量超热电子及其漂移运动对不稳定性的影响。     

BTCF上离子引起的束流不稳定性研究

对所设计的北京τ-粲工厂(BTCF)高亮度对撞模式下电子环中的离子引起的束流不稳定性做了研究.计算了不同束团填充空隙下的离子俘获比,然后用自编的模拟程序对BTCF上快束流–离子不稳定性做了模拟跟踪,得到的快束流–离子不稳定性的增长时间和理论解析计算值基本一致.     

热电子等离子体无碰撞漂移波的稳定性

本文采用Vlasov方程,分析了热电子等离子体中低频交换模和漂移波的性质,讨论了热电子成分的稳定作用。稳定交换模要求热电子成分约为10％,稳定漂移波要求热电子成分约为30%。文中还讨论了离子有限Larmor半径、等离子体密度梯度和温度、磁场曲率、扰动波长等参数对稳定性的影响。同MHD近似下强碰撞漂移波的结果相比较,热电子对无碰撞漂移波有更好的稳定作用。 关键词：     

热电子等离子体低频不稳定性的非线性理论

本文分析了热电子等离子体中低频漂移不稳定性和交换不稳定性的非线性性质,导出了扰动幅度随时间变化的非线性耦合方程,得到了等离子体密度扰动的饱和幅度,讨论了热电子成分对饱和幅度的影响。漂移波引起的等离子体密度扰动相对幅度约20％,交换模引起的等离子体密度相对扰动幅度约5％。当热电子成分达到线性稳定条件所要求的阈值时,漂移波和交换模的饱和幅度降为零。 关键词：     

温离子对动力迥旋损失锥不稳定性的作用

本文详细研究了温离子对动力论迴旋损失锥(DCLC)不稳定性的作用,并与温离子抑制流体近似下DCLC模的理论进行了比较,发现由于(1)磁漂移共振耗散可以激发负能的DCLC波;(2)另一种新的正能波可以因共振获得能量而增长;因此当流体近似DCLC模被少量温离子所抑制的同时,动力论DCLC模仍然是不稳定的。所以要抑制动力论DCLC不稳定性需要注入更多的温离子,本文给出了定量的结果。 关键词：     

Energy dispersive X-ray spectroscopy for ECR plasma diagnostics

Electron-ion bremsstrahlung spectra down to 4 keV emitted from plasmas of the 7.25 GHz electron cyclotron resonance (ECR) ion source of the Forschungszentrum Rossendorf and of the 14.5 GHz ECR ion source of the Technische Universität (TU) Dresden were de-convoluted using a newly developed integration method. In the approximation of isotropy in velocity space this method yields the exact electron energy distribution function. The high energetic electrons are clearly separated into two Boltzmann distributed populations. Their densities and temperatures could be estimated. Higher frequencies of the microwave can increase the hot and warm electron densities by orders of magnitude. First results are obtained for the behaviour of this populations belonging to the mixture (argon — oxygen). Gas mixing increases the densities of these populations. The influence of the electron energy distribution function on X-ray line intensities is discussed.     

Stability of two-dimensional ion acoustic solitons

A modified KdV equation for two-dimensional ion acoustic soliton has been derived for warm (adiabatic) ions and hot isothermal electrons in a collision free plasma. Its solution is found to be stable against transverse perturbations.     

Effect of finite ion temperature on modulational instability of ion-acoustic waves

A nonlinear Schrödinger equation for ion-acoustic waves in a collision free plasma, consisting of warm ions and hot isothermal electrons is derived using the KBM method. It is found that for finite ion temperature these waves are modulationally unstable only in a range of wave numbers. As the ratio of ion to electron temperature increases, the range of the unstable region decreases and shifts towards small wave numbers.     

Fluid Model of a Sheath Formed in Front of an Electron Emitting Electrode Immersed in a Plasma with Two Electron Temperatures

The formation of a sheath in front of a negatively biased electrode (collector) that emits electrons is studied by a one‐dimensional fluid model. Electron and ion emission coefficients are introduced in the model. It is assumed that the electrode is immersed in a plasma that contains energetic electrons. The electron velocity distribution function is assumed to be a sum of two Maxwellian distributions with two different temperatures, while the ions and the emitted electrons are assumed to be monoenergetic. The condition for zero electric field at the collector is derived. Using this equation the dependence of electron and ion critical emission coefficients on various parameters ‐ like the ratio between the hot and cool electron density, the ratio between hot and cool electron temperature and the initial velocity of secondary electrons ‐ is calculated for a floating collector. A modification of the Bohm criterion due to the presence of hot and emitted electrons is also given. The transition between space charge limited and temperature limited electron emission for a current‐carrying collector is also analyzed. The critical potential, where this transition occurs, is calculated as a function of several parameters like the Richardson emission current, the ratio between the hot and cool electron density, the ratio between hot and cool electron temperature and the initial velocity of secondary electrons. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Dust-acoustic solitary waves in an adiabatic hot dusty plasma

An adiabatic hot dusty plasma (containing non-inertial adiabatic electron and ion fluids, and negatively charged inertial adiabatic dust fluid) is considered. The basic properties of arbitrary amplitude dust-acoustic (DA) solitary waves, which exist in such an adiabatic hot dusty plasma, are explicitly examined by the pseudo-potential approach. To compare the basic properties (critical Mach number, amplitude and width) of the DA solitary waves observed in a dusty plasma containing adiabatic electron, ion and dust fluids with those observed in a dusty plasma containing isothermal electron and ion fluids and adiabatic dust fluid, it has been found that the adiabatic effect of inertia-less electron and ion fluids has significantly modified the basic properties of the DA solitary waves, and that on the basic properties of the DA solitary waves, the adiabatic effect of electron and ion fluids is much more significant than that of the dust fluid.     

弱相对论等离子体横向扰动下的离子声孤波

在低阶近似下，得到了描述无磁场相对论热离子等离子体的KP(Kadomtsev-Petviashvilli) 方程.研究表明，相对论热离子等离子中的非线性离子声孤波在高阶横向拢动下是稳定的， 且在相对论热离子等离子体中仅存在压缩型孤波. 关键词： 离子等离子体 孤波 声波 约化摄动法     

Ionization dynamics of dense matter generated by intense ultrashort X‐ray pulses

We investigate a pump‐probe X‐ray Thomson scattering (XRTS) experiment that might be carried out at a free electron laser facility to study warm‐to‐hot states of dense matter. Ultrashort and intense X‐ray pulses with different energies (1,560–1,830 eV) heat a 1 µm thick Al target isochorically and create homogeneous and uncompressed warm‐to‐hot states of dense matter. A second pulse with variable delay probes this heated state via XRTS. The X‐ray laser–target interaction is modelled within radiation‐hydrodynamic simulations applying the HELIOS‐CR code. The HELIOS‐CR results qualitatively agree with Monte‐Carlo simulations, where the laser pulse absorption is simulated based on a uniform random sequence of events. The electron feature in the simultaneously observed X‐ray scattering spectrum is a function of the degree of ionization and the target temperature. Therefore, the temporal evolution of the plasmon peak measures the ionization dynamics on ultra‐short time scales. The XRTS spectrum is calculated based on the Chihara formula utilizing the Born‐Mermin approximation for the free electron dynamic structure factor. The proposed experiment will reveal important details of the ionization dynamics on ultra‐short time scales as well as of the relaxation on ps time scales.     

New interior solution describing relativistic fluid sphere

Nonlinear low-frequency electrostatic waves in a magnetized, three-component plasma consisting of hot electrons, hot positrons and warm ions have been investigated. The electrons and positrons are assumed to have Boltzmann density distributions while the motion of the ions are governed by fluid equations. The system is closed with the Poisson equation. This set of equations is numerically solved for the electric field. The effects of the driving electric field, ion temperature, positron density, ion drift, Mach number and propagation angle are investigated. It is shown that depending on the driving electric field, ion temperature, positron density, ion drift, Mach number and propagation angle, the numerical solutions exhibit waveforms that are sinusoidal, sawtooth and spiky. The introduction of the Poisson equation increased the Mach number required to generate the waveforms but the driving electric field E ₀ was reduced. The results are compared with satellite observations.     

Ion sound wave excitation in a plasma under a Langmuir turbulence regime

Ion sound wave excitation in a warm non-relativistic (W_b ≤ 400 eV) electron beam unmagnetized plasma system is studied experimentally. The spectrum of these waves shows two peaks at frequencies of 70 and 230 kHz respectively. The origin of these waves is connected with modulational instability and cavity collapse. We show that the energy of bulk accelerated electrons can explain the measured value of kr_De for high-frequency sound waves. The energy of ion sound waves is not high enough to have an influence on the Langmuir turbulence dynamics.