多基线组合求解深空航天器载波相位模糊方法

针对深空航天器高精度定位需求,提出多基线组合求解载波相位模糊方法,获得比群时延更精确的相时延,极大地提高无线电干涉测量精度。首先建立多基线组合求解载波相位模糊的数学模型,推导该方法对长短基线组合的约束条件。然后利用美国甚长基线阵(VLBA)对本文方法进行仿真校验,结果表明航天器定位精度可以达到纳弧度量级。最后结合我国已有干涉测量网,分析在我国未来深空探测任务中采用多基线组合测量载波相时延的可行性,给出满足方法约束的站址选择建议,可为我国深空导航无线电干涉测量技术的发展和深空测控网的完善提供参考。     

一种用于深空导航定位的新型DOR信标

甚长基线干涉测量(VLBI)是深空探测器导航定位的重要手段之一,深空探测器的VLBI观测通常采用差分单程测距(DOR)信标和双差单程测距(Delta-DOR)测量体制,精确地测量深空探测器相对于河外射电源的角距.相位杂散是影响Delta-DOR测量精度的主要误差源之一,针对这项误差研究了一种基于伪随机噪声调制方式的新型...     

单模式LIPS-200离子推力器的寿命及可靠性定量评估

针对离子推力器产品工作寿命及可靠性定量评估的难题,结合单工作模式LIPS-200离子推力器产品成熟度提升需求,通过寿命主要影响因素耦合分析,应用试验数据、数值模型和数理统计方法,提出了单工作模式离子推力器寿命及可靠性定量评估的可行技术途径:通过分析模型、验证试验和数值模型之间的不断迭代实现各失效模式对应磨损模型的精细化...     

Overview of atmospheric ionizing radiation (AIR) research: SST-present.

The Supersonic Transport (SST) program, proposed in 1961, first raised concern for the exposure of pregnant occupants by solar energetic particles (SEP), and neutrons were suspected to have a main role in particle propagation deep into the atmosphere. An eight-year flight program confirmed the role of SEP as a significant hazard and of the neutrons as contributing over half of the galactic cosmic ray exposures, with the largest contribution from neutrons above 10 MeV. The FAA Advisory Committee on the Radiobiological Aspects of the SST provided operational requirements. The more recent lowering of ICRP-recommended exposure limits (1990) with the classification of aircrew as "radiation workers" renewed interest in GCR background exposures at commercial flight altitudes and stimulated epidemiological studies in Europe, Japan, Canada and the USA. The proposed development of a High Speed Civil Transport (HSCT) required validation of the role of high-energy neutrons, and this resulted in ER-2 flights at solar minimum (June 1997) and studies on effects of aircraft materials on interior exposures. Recent evaluation of health outcomes of DOE nuclear workers resulted in legislation for health compensation in year 2000 and recent European aircrew epidemiological studies of health outcomes bring renewed interest in aircraft radiation exposures. As improved radiation models become available, it is imperative that a corresponding epidemiological program of US aircrew be implemented.     

机会数字阵雷达概念与应用技术分析

机会数字阵雷达是以平台隐身性设计为核心,以数字阵列雷达为基础,兼具多功能、多模式的"一体化"新概念雷达系统.本文在对国外有关概念雏形描述理解基础之上,对其定义和涵义进行了深入透析,详细论述了"机会"一词的几层涵义.分析了机会数字阵雷达不同于传统相控阵雷达的技术特性和应用潜力,以及机会数字阵雷达所面临的技术难题,如3-D空间单元"机会性"分布优化选取和波束综合,信号传输与同步以及多自由度的系统资源优化管理等问题,并给出了初步的解决方案和仿真结果.     

Polarization pattern of low and mid-frequency magnetic pulsations in the polar cap: A comprehensive analysis at Terra Nova Bay (Antarctica)

The polarization pattern of ULF pulsations (f ≈ 1–100 mHz) at Terra Nova Bay (Antarctica, CGM λ ∼ 80°) has been determined for the entire 2003, soon after the solar maximum. A comparison with the results of previous investigations, conducted at the same station close to the solar minimum (1994–96), allows to focus common elements and major differences among different frequency bands which persist through the entire solar cycle. Basically, between f ∼ 1.5 and 5 mHz, the day can be divided into four sectors with alternate polarizations. The local time and latitudinal dependence of the observed pattern can be tentatively interpreted in terms of a latitude of resonant field lines reaching λ ∼ 80° in the noon sector; on the other hand, resonance effects of lower latitude field lines can be clearly identified also far from the noon meridian when the station moves into the deep polar cap. Moreover, in the morning sector the resonance region would extend to lower latitudes than in the evening sector. The proposed profile of the resonant region can interpret also the results obtained at other cusp/auroral stations and appears consistent with that one inferred in the northern hemisphere at smaller latitudes. The resonance region progressively shifts toward lower latitude with increasing frequency; correspondingly, the four-sector pattern progressively disappears at TNB. Above f ∼ 20 mHz, the experimental observations might suggest an additional contribution from Sunward propagating waves, possibly via the magnetotail lobes.     

An Investigation of the Mechanical Properties of Some Martian Regolith Simulants with Respect to the Surface Properties at the InSight Mission Landing Site

In support of the InSight mission in which two instruments (the SEIS seismometer and the \(\mbox{HP}^{3}\) heat flow probe) will interact directly with the regolith on the surface of Mars, a series of mechanical tests were conducted on three different regolith simulants to better understand the observations of the physical and mechanical parameters that will be derived from InSight. The mechanical data obtained were also compared to data on terrestrial sands. The density of the regolith strongly influences its mechanical properties, as determined from the data on terrestrial sands. The elastoplastic compression volume changes were investigated through oedometer tests that also provided estimates of possible changes in density with depth. The results of direct shear tests provided values of friction angles that were compared with that of a terrestrial sand, and an extrapolation to lower density provided a friction angle compatible with that estimated from previous observations on the surface of Mars. The importance of the contracting/dilating shear volume changes of sands on the dynamic penetration of the mole was determined, with penetration facilitated by the \(\sim1.3~\mbox{Mg/m}^{3}\) density estimated at the landing site. Seismic velocities, measured by means of piezoelectric bender elements in triaxial specimens submitted to various isotropic confining stresses, show the importance of the confining stress, with lesser influence of density changes under compression. A power law relation of velocity as a function of confining stress with an exponent of 0.3 was identified from the tests, allowing an estimate of the surface seismic velocity of 150 m/s. The effect on the seismic velocity of a 10% proportion of rock in the regolith was also studied. These data will be compared with in situ data measured by InSight after landing.     

基于稀疏随机阵列配置的CS-MIMO雷达感知矩阵构造

压缩感知(CS)理论中的感知矩阵在观测数据获取和信号重建过程中起关键性作用。目前,大部分研究通过引入高斯随机矩阵作为测量矩阵实现压缩观测,这类测量矩阵对硬件要求很高,工程实现困难。提出了一种基于稀疏随机阵列配置的压缩感知-多输入多输出(CS-MIMO)雷达中的感知矩阵构造方法,当MIMO雷达阵元配置为满足某种概率分布的稀疏随机阵列时,发射与接收导引矢量的Kronecker积能够起到压缩测量的作用。从理论上分析了所构造的感知矩阵的归一化互相关系数、Gram矩阵以及阵列方向图之间的内在联系,并证明了当随机阵元位置满足均匀分布时所构造的感知矩阵满足压缩感知重构条件。在这种稀疏随机阵列配置方式下,既可以避免额外引入随机测量矩阵,又能减少所需的阵元个数,从而大大降低CS-MIMO雷达系统复杂度。仿真实验表明,该方法具有较低的感知矩阵归一化互相关系数,与满阵CS-MIMO雷达相比能够在减少阵元个数的同时获得良好的重构性能,且使重构所需运算量大大降低。     

基于幅频特性曲线簇公共点的智能弹簧减振系统参数设计

研究了无阻尼智能弹簧减振系统的一种参数设计方法.采用等效线性化方法将系统中的干摩擦阻尼等效成黏性阻尼,建立系统的数学模型,推导出无量纲化的振动微分方程,得到系统频响特性的解析解.对系统幅频特性进行了数值分析,结果发现:幅频特性曲线簇通过一个公共点,该公共点随质量比的增大向左偏移,随刚度比的增大向右偏移;系统存在一个最优控制参数值,使系统幅频特性曲线峰值最小,其随质量比的增大而减小,但不受刚度比的影响.根据公共点的性质,得到幅频特性曲线簇公共点对应的频率比、最优控制参数和最小振幅的计算公式.确定系统参数的选用原则与范围,并利用公共点提出智能弹簧减振系统参数设计的方法和步骤.      

Modelling of cometary nuclei: Planetary missions preparation

The planning of planetary missions requires the knowledge as much as possible accurate of the target. This knowledge, which cannot be obtained only by ground based observations, can be supported by theoretical modeling. This is particularly true in the case of Rosetta, a cornerstone ESA mission that will be launched in January 2003, and of its target, the comet 46P/Wirtanen. In this paper we show how, using a nucleus thermal evolution model, it is possible to foresee the temperature of the nucleus surface and the activity level along the orbit and define the range of possible values for these properties. Activity level close to the aphelion depends on the presence of CO. Surface temperatures depend on the physical properties attributed to the dust: temperatures reached by a crust mainly composed by silicatic grains differ from the temperatures reached by a crust mainly composed by organic grains.