Physical mechanism of the vertical electric field generation over active tectonic faults

The concept of the Global Electric Circuit (GEC) provides an explanation of the existence of a vertical atmospheric electric field and coupling between the ground and ionosphere. Presently, ionospheric physics pays more attention to electric fields and coupling processes in the polar and auroral regions, whereas in other areas the potential difference between the ground and ionosphere usually is not taken into account. Regional processes exist, however, that are able to significantly affect the GEC parameters and through modification of the ionospheric potential to create plasma density irregularities of different scales within the ionosphere. One such source of ionosphere modification is air ionization in the vicinity of active tectonic faults, which takes place due to increased radon emanation. This paper considers the process of local modification of the GEC and corresponding ionospheric variability due to tectonic activity.     

弹道快速解法-样条边值法

本文提出了一种弹道计算的新方法，样条边值法，它具有精度高，收敛快的优点。     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.     

高超声速边界层的转捩及预测

首先描述了边界层转捩的基本过程及研究内容。在此基础上,指出了高超声速边界层不同于不可压缩边界层的流动不稳定性特性,并介绍了边界层的转捩机理与感受性特征;给出了高超声速三维边界层中预测转捩的常用方法,并着重介绍了多用于工程实际的e N方法以及对e N方法的理性改进,同时列举了在高超声速三维边界层中应用e N方法实现转捩预测的多个实例。最后,分析并总结了高超声速边界层转捩预测所存在的困难及需要解决的问题。     

高超声速边界层转捩机理及应用的若干进展回顾

高超声速边界层转捩对飞行器的热传递、表面摩阻和流动分离等有重要影响,尤其是再入飞行器和吸气式巡航飞行器。然而,人们对边界层转捩机理中的很多问题认识还不清楚,或存在争议。本文从扰动波演化的角度回顾了高超声速边界层感受性、线性稳定性和非线性作用的国内若干研究进展,并以基于谐波共振的人工转捩技术为例示范了这些机理认识在转捩控制上的应用。扰动的产生和发展是认识边界层转捩机理的核心。通过研究扰动波来认识边界层转捩机理,开展应用创新研究对提升飞行器性能具有重要意义。     

超声速平板边界层旁路转捩直接数值模拟

采用具有七阶精度的有限差分格式和基于Euler方程组的特征边界条件,通过直接数值模拟研究了由固定相位周期性吹吸扰动诱导的、Ma∞=2.25、Re∞=2.5×107/m(635 000/inch)空间发展平板边界层的旁路转捩过程,并建立了相应的直接数值模拟数据库。数值结果表明:扰动相位的随机性并不是转捩发生的必要条件,固定相位周期性吹吸扰动即可诱发边界层的转捩;当采用固定相位时,随着吹吸频率的增加,转捩位置向下游移动;当扰动频率足够大时,周期性吹吸无法诱导出边界层的转捩。随后,在所得数据库中提取了速度及热力学变量的平均值,与已有的数据库和理论分析吻合良好;速度脉动均方根与公认的不可压缩平板边界层实验基本吻合;热力学变量脉动均方根和雷诺应力与已有数据库的统计结果及实验数据具有相同的分布特征。对比发现,不同转捩的诱导因素对平均转捩位置和热力学变量均方根、雷诺应力等高阶统计量的影响较大。     

(高)超声速流动试验技术及研究进展

近年来,与高速飞行器相关的(高)超声速流动受到了极大的关注。这类流动所具有的非定常性、强梯度和可压缩性对试验方法和风洞设计技术提出了挑战。超声速纳米示踪平面激光散射(NPLS)技术是由作者所在团队研发的非接触光学测试技术。它能够以较高的空间分辨率来揭示超声速三维流场的一个瞬态剖面的时间解析的流动结构。介绍了NPLS技术以及基于NPLS开发的密度场测量、雷诺应力测量和气动光学波前测量等方法,并回顾了这些技术在超声速边界层、超声速混合层、超声速压缩拐角、激波/边界层相互作用和光学头罩绕流等流动中的应用,清晰地再现了边界层、混合层、激波等典型流场结构及其时空演化特性。另外,为了模拟和研究高空大气条件下边界层自然转捩和超声速混合层的转捩特性,介绍了高超声速静风洞、超-超混合层风洞的设计技术以及层流化喷管的设计方法。     

The Low-Latitude Boundary Layer at the Flanks of the Magnetopause

This is a brief overview on what we know and do not know about the low-latitude boundary layer (LLBL) at the flanks of the magnetotail. On the basis of recent observations, simulations and theories we conclude that reconnection is the dominant process in generating the LLBL and its structure probably even under northward IMF conditions. Part of the LLBL always seems to be on open field lines. Possibly the LLBL possesses a double structure with its outer part open and inner part closed. Anomalous diffusive processes cannot sustain the LLBL but provide sufficient diffusivity for reconnection. Strong diffusion is only expected in narrow localized regions and can make the transition to superdiffusion. Kelvin-Helmholtz instability (KHI) is favoured for northward IMF, producing vortices at the tail flanks. Its contribution to efficient mass transport still remains questionable. Coupling of the LLBL to the ionosphere can strongly affect the internal structure of the LLBL, causing turbulent eddies and detachments of plasma blobs as also field-aligned currents and electron heating. The structure and dynamics of the LLBL are affected by field-aligned electric potentials that decouple the LLBL from the ionosphere. Non-ideal coupling simulations suggest that the dusk flank is decoupled, favouring KHI, while the dawn flank is dominated by currents and turbulence.     

用特征根构造变系数线性最佳控制

本文研究单输入n阶常系数线性系统满足二次型指标(积分区间有限,终点给定为(o,…o)) 的最佳控制。所得结果使用户无需解Riccati方程,也不要用数值法解出两点边值问题,仅由这个两点边值问题的特征根即可构造变系数线性最佳控制。这个结果既适于低价(n=1,2,3)时用来写出变系数线性最佳控制的一般表达式(17)—(19),也适于高阶时用计算机计算,其程序已用FORTRAN-Ⅳ在AD三TAMAX-186机上实现。     

平板湍流摩阻系数的显式表达式

 湍流摩阻系数的计算是工程技术中经常遇到的问题。计算时所依据的公式多为半经验半理论的结果,如Karman公式,Van Driest公式和Prandtl公式等。这些公式是以隐函数给出的,给计算带来不便。但是不难发现,这类公式经过适当的变换,可以化为统一形式的超越代数方程,这种方程没有有限形式的解析解,本文给出了一种近似解析解。根据这种方法除了导出上述公式的显式表达式外,还对White公式作了修正。当然解超越代数方程最根本的方法是迭代法,本文对此也作了简单讨论。