捷联惯性测量装置陀螺仪零次项误差温度补偿方法

为满足捷联惯性测量装置快速启动的要求,研究了陀螺仪零次项误差随温度变化的规律,建立了陀螺仪零次项误差随温度变化的模型,提出了一种可以使用软件对温度带来的误差实时进行补偿的方法,并通过试验验证了温度模型的准确性和补偿方法的有效性。     

极弱信号环境下GPS位同步和载波跟踪技术

为解决环路未锁定、无法找出正确的导航数据位跳变点时极弱全球定位系统(GPS)信号跟踪问题,通过分析信号跟踪模型和相关器1 ms采样数据特性,将最优路径动态规划算法应用于GPS位同步,并提出基于平方根无迹卡尔曼滤波(SRUKF)和位同步结合的载波联合跟踪算法。建立了适合位同步的SRUKF载波环参数估计模型,针对位同步的实现条件和无相位频率先验信息的情况,将位同步模块提前,研究设计了环路未锁定时串行和并行两种弱信号跟踪方案。位同步跟踪完成后环路采用单独的SRUKF工作方式。实验结果证实该文提出的算法具有较高的数据位边缘检测概率(EDR)和参数估计性能,而无须关心环路是否处于锁定状态,能够对载噪比低至22 dB/Hz的弱信号实现跟踪。     

行波机理对低散射目标支架雷达散射截面的影响研究

针对雷达低散射支架,文中首先采用天线机理分析行波对雷达散射截面(RCS)的贡献,并且使用等效相速度的概念求出双弧线外形目标支架在远区的辐射场,最后分析得出低散射支架行波辐射特性,并讨论行波对目标支架RCS的影响。     

空间目标姿态角估计与RCS反射图生成

介绍了一种空间目标姿态角估计方法,并在此基础上生成了RCS反射图.该方法主要是在直角坐标系中对目标的运动特征用二次项进行描述,并用最小二乘估计求解二次方程,从而根据运动方程估计出目标的姿态角.实测数据验证结果表明,该方法能够有效地估计出空间目标的姿态角变化情况,并可反映出目标RCS随其姿态变化的规律.     

极化扭转技术在毫米波天线中的应用

本文简述了极化扭转反射器的工作原理，将极化扭转技术应用到毫米波天线中去的几个主要应考虑的因素；探讨了在倒置卡塞格伦天线中主、副反射面上栅条的成型技术；在经过优化设计基础上对加工而成的毫米波天线进行了测试，给出实测结果并对结果进行了分析。     

测试理论在紧缩场天线测试中的新应用

文章以中国空间技术研究院紧缩场测试系统的组成和特点为例,分析介绍了紧缩场测试误差的来源、测试设备必要的升级改造和测试软件的更新应用。通过将测试理论知识应用于测试工程实际,可有效去除由于测试场非理想因素引入的各类测试误差,获得更接近天线实际性能的测试结果;同时有效分析处理测试数据,简化实际测试工作,提高测试效率。     

Ion dynamics associated with Alfven wave in the near-Earth magnetotail: Two-dimensional global hybrid simulation

Ion dynamics in the near-Earth magnetotail region is examined during periods of fast Earthward flow with a two-dimensional (2-D) global-scale hybrid simulation. The simulation shows that shear Alfven waves are generated at x ∼ −10R_E, where the strong earthward flow is arrested by the dipole field, and propagate along field lines from the equator to both southern and northern polar ionosphere. Non-gyrotropic ion velocity distributions occur where the large-amplitude Alfven waves are dominant. The simulation indicates that the Alfven waves are generated by interaction of the fast earthward flow with the stationary near-Earth plasma. Beam ions are found to be pitch-angle scattered and trapped in the wave field, leading to the non-gyrotropic ion distributions in the high-latitude plasma sheet boundary. In addition, significant particle heating and acceleration are found to occur behind the dipolarization front due to the effect of wave turbulence.     

Improvement in the GERB short wave flux estimations over snow covered surfaces

Because space-borne radiometers do not measure the Earth’s outgoing fluxes directly, angular distribution models (ADMs) are required to relate actual radiance measurement to flux at given solar angle, satellite-viewing geometries, surface, and atmospheric conditions. The conversion of one footprint broad-band radiance into the corresponding flux requires therefore one to first characterize each footprint in terms of surface type and cloud cover properties to properly select the adequate ADM.

A snow (and sea-ice) retrieval technique based on spectral measurements from the Spinning Enhanced Visible and Infrared Imager (SEVIRI) on board Meteosat 8 is presented. It has been developed to improve the scene identification and thus the ADM selection in the near-real time processing of the Geostationary Earth Radiation Budget (GERB) data at the Royal Meteorological Institute of Belgium. The improvement in the GERB short wave flux estimations over snow covered scene types resulting from angular conversion using dedicated snow ADMs (e.g., empirical snow ADMs and/or pre-computed theoretical snow ADM) instead of empirical snow-free ADMs is discussed.     

面对面倾斜度误差的解析评定

简要地叙述了面对面倾斜度误差的最小二乘评定和最小条件评定法,并分别建立了评定面对面倾斜度误差的数学模型。文中的评定原理可扩展到其他倾斜度误差的评定。     

RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium

The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral distribution of natural plasma waves, and monitor dust and gas activities around the nucleus. The MIP instrumentation consists of an electronics board for signal processing in the 7 kHz to 3.5 MHz range and a sensor unit of two receiving and two transmitting electrodes mounted on a 1-m long bar. In addition, the Langmuir probe of the RPC/LAP instrument that is at about 4 m from the MIP sensor can be used as a transmitter (in place of the MIP ones) and MIP as a receiver in order to have access to the density and temperature of plasmas at higher Debye lengths than those for which the MIP is originally designed.