行星际空间环境对探测器可靠性影响分析

空间环境是影响航天器可靠性的重要因素。与地球轨道航天器相比,行星际探测任务可能会遭受更加恶劣的空间环境,例如极端温度环境,辐射环境,腐蚀性大气环境、宇宙尘等,再加上行星际任务寿命长,采用先进的器件和材料,空间环境对行星际探测器的可靠性构成严重的威胁,直接关系到探测目标能否实现。因此考虑空间环境对行星际探测器的影响,开展相关的预先研究无论是对于制定行星际空间探测计划,还是搭载仪器的设计都具有非常重要的意义。文章分析了极端温度、辐射环境和行星表面综合环境对探测器的影响,并对开展相关研究提出了建议。     

星载合成孔径雷达模糊特性研究

在分析星载合成孔径雷达模糊信号来源的同时，论述了分辨率，测绘带宽，模糊度，脉冲重复频率之间的相互制约关系，并提出了在总体设计中如何选择脉冲重复频率以减少模糊的方法，最后给出了计算方位模糊比和距离模糊比的实用算法及仿真结果。     

多因素组合下发射载体出管速度偏差预估方法

运用极限偏差、合成标准差、统计分析、蒙特卡洛仿真等多种预估方法,对发射载体出管速度偏差进行对比分析。分析结果表明,极限偏差法工程应用成熟,但预估结果偏于保守,适用于影响因素尚未认知完全的工程型号;对于影响因素比较明确的系统,运用统计分析法、合成标准差法得到的发射载体出管速度预估值一致性好,方法简单,且具有较高的准确性;蒙特卡洛法计算过程复杂,可通过大量仿真计算获取出管速度的分布特性,得到对应不同指标的分布概率,相比其他几种方法,计算结果更加科学、合理。工程型号应用时,可根据实际需要组合使用上述方法进行发射载体出管速度偏差预估分析。     

聚束式SAR中卷积反投影算法的快速实现

对应用于聚束式合成孔径雷达 (SAR) 成像中的卷积反投影 (CBP) 算法进行了详细研究,提出了一种基于傅里叶变换的快速实现方法,使得CBP算法的计算量得到明显降低.在传统的CBP算法中,反投影过程中的重采样通过插值实现,因而所需的插值数量巨大,导致运算效率低下.研究了图像像素之间隐含的相对位置关系之后,本文采用一系列快速傅里叶变换 (FFT)来实现反投影过程中的重采样,避免了运算量巨大的插值过程,故提高了运算效率.仿真结果证明了新算法的可行性和有效性.相比于传统的CBP算法,新算法可以提高大约85%的运算效率.由于FFT适用于并行处理,新方法在实时处理SAR系统中有一定的应用价值.     

Numerical investigation on flow field characteristics of dual synthetic cold/hot jets using POD and DMD methods

In order to improve the control ability of synthetic jets in compressible boundary layer, a novel control method based on dual synthetic cold/hot jets coupled control of velocity profile and temperature profile was proposed. As fundamental investigations on the effects of synthetic jet temperature on the jet behavior and flow field characteristics were essentially necessary, preliminary numerical simulations were conducted to study the influence of temperature (200 K and 400 K) on the flow field characteristics of synthetic jets using Large Eddy Simulations (LES) model. Time-averaged flow fields showed that different temperatures led to variable behavior of two strands of jets. For dual synthetic cold jets, a potential-core arose apparently with its height ranging from 0.01 to 0.03 m, while for dual synthetic hot jets, two strands of jets emerged downstream. The modal decomposition of instantaneous flow fields had been done using both Proper Orthogonal Decomposition (POD) and Dynamic Mode Decomposition (DMD). Various modes showed different characteristics of the flow fields. As the POD method focuses on the energy of flow while the DMD method focuses on the frequency, the first two modes had many similarities, but the third and fourth modes demonstrated completely different vortex structures. The current researches play a role of preliminary investigations for further and comprehensive exploration of novel flow control measures in global velocity field.     

一种基于COTS的SAR分布式目标模拟方法

针对目前合成孔径雷达(SAR)目标模拟器通常只能模拟点目标，且通用化程度和实时性较低的问题，提出了一种基于商用现成品或技术(COTS)的SAR分布式目标模拟方法。利用NI PXI平台构建了一个基于电磁仿真的SAR分布式目标模拟器，由电磁仿真软件模拟获取目标散射特性，并通过高速网口输入硬件设备进行采样及卷积操作得到仿真SAR回波数字信号，经数模转换模块完成对SAR数字信号的调制并输出模拟回波，可以直接用于SAR系统的数据验证。模拟器采用数字式一体化硬件设备，由NI PXIe-5646R和PXIe-5840进行信号的接收和发送，PXIe-7902作为系统核心进行高速实时数据运算。系统以现场可编程门阵列(FPGA)为核心，通过LabVIEW RT (Real Time)和FPGA模块直接进行访问，能实时、高速地采集和处理数据。经过测试，该目标模拟器可以生成分布式目标的射频回波信号，环路验证结果证明了本文提出方法的有效性。另外，本文提出的方法适用于多种雷达信号的模拟，通过设置不同的信号体制或接收外部信号输入，可以实现灵活的SAR目标模拟。     

氨合成-水热改性法制备氢氧化镁阻燃剂

为了解决氢氧化镁和聚合物之间的不相容问题, 对氨合成法-水热改性处理2步法制备高分散氢氧化镁阻燃剂进行了研究,分析了常温合成温度、水热改性温度和水热改性时间对制备大晶型、低比表面积氢氧化镁阻燃剂的影响.结果表明,经过水热改性处理改变了氢氧化镁晶体的生长习性,生成了形貌规则、粒径分布均匀、分散性良好的氢氧化镁六方片状颗粒.另外通过提高氯化镁浓度和氨水过量1倍,探讨了常温合成反应的转化率,认为应该在反应原料等当量下寻求提高转化率的可行方法.     

Loop Models from SOHO Observations

The Coronal Diagnostic Spectrometer (CDS) on SOHO is a grazing/normal incidence spectrograph, aimed to produce stigmatic spectra of selected regions of the solar surface in six spectral windows of the extreme ultraviolet from 150 Å to 785 Å (Harrison et al. 1995). In the present work, CDS, EIT, MDI and Yohkoh observations of active region lops have been analyzed. These observations are part of JOP 54. CDS monochromatic images from lines at different temperatures have been co-aligned with EIT and MDI images, and loop structures have been clearly identified using Fe XVI emission lines. Density sensitive lines and lines from adjacent stages of ionization of Fe ions have been used to measure electron density and temperature along the loop length; these measurements have been used to determine the electron pressure along the loop and test the constant pressure assumption commonly used in loop modeling. The observations have been compared with a static, isobaric loop model (Landini and Monsignori Fossi 1975) assuming a temperature-constant heating function in the energy balance equation. Good agreement is found for the temperature distribution along the loop at the coronal level. The model pressure is somewhat higher than obtained from density sensitive line ratios.     

机动目标的逆合成孔径雷达成像

 逆合成孔径雷达(ISAR)和合成孔径雷达 (SAR)都是利用目标 (场景)与雷达的相对运动,提高横向分辨率,实现对目标 (场景 )的成像。SAR的运动方是雷达平台,可控制作平稳飞行,且用仪器测校其偏离误差;ISAR的运动方通常是非合作目标,运动不受控制,且难以精确测量。当目标作机动飞行时,以目标作固定基准,雷达等效地在空间形成流形复杂的逆合成孔径 (阵列 ),对这种情况下成像的问题进行了系统的研究。     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .