Reconstruction of space weather physical parameters on 400-year scale

The main goal of this paper is to get physically informative comprehensive data about dynamics of the solar magnetic field, geomagnetic field, and interplanetary magnetic field over large time scales. The total sunspot magnetic flux, aa and IDV indices of geomagnetic activity, the IMF strength, the dipole-octopole index of the large-scale magnetic field of the Sun, and the open magnetic flux are reconstructed for 400 years. The reconstruction of the π index of the large-scale polar magnetic field of the Sun is performed for 150 years.     

Alfven modes of solar coronal magnetic arches: Excitation of ballooning instability and modulation of flare emission

The effect of Alfven-type oscillations in a coronal magnetic arch on modulation of the gyrosynchrotron radiation and development of the ballooning instability in the arch is considered. On the basis of the energy method and the method of normal modes, the expressions are obtained for increments of ballooning instability at its swinging by natural oscillations of the arch. The conclusion is drawn that bending oscillations, which do not actually compress the plasma and, therefore, represent the Alfven-type modes, unlike the radial oscillations, are capable, under solar corona conditions, to effectively swing ballooning instability and, as a consequence, play a part of a trigger for solar flares. The ballooning instability of coronal arches is shown to be capable of causing formation of helmet-shaped structures in the lower solar corona. On the basis of calculations of the intensity modulation depth and the degree of circular polarization of non-thermal gyrosynchrotron radiation, under the assumption of excited Alfven oscillations of a coronal arch, the conclusion is drawn, that microwave observations at a frequency of > 10 GHz can be used for studying the conditions of excitation and propagation of Alfven modes in flare loops. The consequences of obtained results are discussed using the flare on April 15, 2002 as an example.     

An analysis of low-frequency component in microacceleration measurements made onboard the <Emphasis Type="Italic">Foton M-2</Emphasis> satellite

The low-frequency component is investigated in the data of measurements performed onboard the Foton M-2 satellite with the three-component accelerometer TAS-3. Investigations consisted in comparison of this component with its calculated analog found from a reconstruction of the satellite’s attitude motion. The influence of the Earth’s magnetic field on the accelerometer readings is discovered by way of spectral analysis of the functions representing the results of determining the low-frequency microacceleration by two methods. After making correction for this influence, the results obtained by these two methods coincided within a root-mean-square error of less than 10^?6 m/s².     

Turbulent fluctuations of plasma and magnetic field parameters in the magnetosheath and the low-latitude boundary layer formation: Multisatellite observations on March 2, 1996

The results of simultaneous analysis of plasma and magnetic field characteristics measured on the INTERBALL/Tail Probe, WIND and Geotail satellites on March 2, 1996, are presented. During these observations the INTERBALL/Tail Probe crossed the low-latitude boundary layer, and the WIND and Geotail satellites measured the solar wind’s and magnetosheath’s parameters, respectively. The plasma and magnetic field characteristics in these regions have been compared. The data of the Corall, Electron, and MIF instruments on the INTERBALL/Tail Probe satellite are analyzed. Fluctuations of the magnetic field components and plasma velocity in the solar wind and magnetosheath, measured onboard the WIND and Geotail satellites, are compared. The causes resulting in appearance of plasma jet flows in the low-latitude boundary layer are analyzed. The amplitude of magnetic field fluctuations in the magnetosheath for a studied magnetosphere boundary crossing is shown to exceed the magnetic field value below the magnetopause near the cusp. The possibility of local violation of pressure balance on the magnetopause is discussed, as well as penetration of magnetosheath plasma into the magnetosphere, as a result of magnetic field and plasma flux fluctuations in the magnetosheath.     

基于谱方法的寻的导弹零效脱靶量性能分析

在寻的导弹的设计过程中,制导导弹的性能通常用脱靶量来度量。目前,对寻的制导     

烧蚀条件下氮化硼材料表面的产物分析

建立了氮化硼材料基于热化学平衡条件下的烧蚀模型,并进行了数值模拟分析.结果表明:在烧蚀的过程中氮化硼材料表面形成的主要产物为BO、B2O、B2O2及B2O3;当压力升高时,有利于B2O2及B2O3的产生,不利于BO,B2O的产生,而无因次的质量损失率呈降低的趋势.     

A method for representing the thermodynamic and thermophysical functions in simulation of powerplant processes

A method for representing thermodynamic and thermophysical functions is presented; the functions make it possible to simulate thermal and gasodynamic processes in powerplants that use different individual substances or their mixtures as a working fluid. The method also involves consideration of real gas properties.     

颗粒两相流自由剪切层大涡模拟

采用大涡模拟(LES)方法数值仿真了可压缩流自由剪切层内颗粒两相流流场结构.气相控制方程采用二维盒式滤波法滤除小于网格尺度的小涡以得到LES控制方程,而流场中小涡对大涡的影响采用K-ωSST湍流模型模拟.在Lagrange坐标系下用颗粒轨道模型仿真颗粒运动,用双线性插值方法实现Euler坐标系到肌Lagrange坐标系的转换,并考虑了颗粒速度和温度的改变对气相流场的反作用.分析了仿真结果中气相自由剪切层的涡结构特性,不同St数颗粒在流场中的运动特性,颗粒对流场的反作用效果,得到了合理的结论.     

长寿命航天器机构的加速寿命试验方法

介绍了加速寿命试验的概念、类型和基本特征;综述了长寿命航天器机构加速寿命试验方法的研究现状;分析了固体润滑和油润滑长寿命航天器机构准加速寿命试验方法的特点;针对目前长寿命航天器机构准加速寿命试验中存在的问题,提出了解决这些问题的思路。     

一种软件化激光引信的实现方法

测距精度是衡量激光引信性能的重要指标之一。以往模拟信号波形处理中常采用前沿阈值法来检测处理波形。但是当激光回波波形因各种因素发生随机起伏和畸变时,这种方法就会出现较大的误差,严重地影响测距精度。设计了一种基于DSP硬件平台的软件化激光引信实现方案,给出了模块化后的硬件电路结构图以及各个功能模块的作用和相互之间的关系。研究了用数字波形处理技术提取测距基准的波形质心算法。通过计算机模拟比较了前沿阈值法和波形质心算法的性能,仿真结果显示波形质心算法具有较低的虚警概率、漏警概率和较高的测距精度。