红外型空空导弹智能制导律研究

本文论述了红外型空空导弹应用智能控制的理论基础及结构特点，以多级智能控制的框架和机理设计出以比例导引为主、智能控制为辅的变指令智能制导律，并编制计算机软件以数字仿真的形式验证变指令智能制导规律的有效性和可行性     

红外多光谱扫描仪主体设计

文中简要介绍了中巴合作地球资源卫星(CBERS)红外多光谱扫描仪主体(简称扫描仪主体)的组成和工作原理。     

天体对卫星红外地球敏感器干扰的研究

我国在轨运行的卫星多次因红外地平仪受天体的干扰而出现姿态异常的情况．本文介绍了各种红外地平仪工作原理，分析了它们受干扰的原因，给出了精确预报的方法，并在此基础上提出了相应的抗干扰措施，有些已成功运用到在轨运行的卫星上。     

Radiative and hybrid cooling of infrared space telescopes

The designs of cold space telescopes, cryogenic and radiatively cooled, are similar in most elements and both benefit from orbits distant from the Earth. In particular such orbits allow the anti-sunward side of radiatively-cooled spacecraft to be used to provide large cooling radiators for the individual radiation shields. Designs incorporating these features have predictedT _tel near 20 K. The attainability of such temperatures is supported by limited practical experience (IRAS, COBE). Supplementary cooling systems (cryogens, mechanical coolers) can be advantageously combined with radiative cooling in hybrid designs to provide robustness against deterioration and yet lower temperatures for detectors, instruments, and even the whole telescope. The possibility of such major additional gains is illustrated by the Very Cold Telescope option under study forEdison, which should offerT _tel5 K for a little extra mechanical cooling capacity.     

直升机红外抑制器两种进气方式下的实验研究

利用地面模拟试验件通过实验比较分析了两种进气方式对红外抑制器性能的影响。为了模拟直升机前飞和悬停两种状态,在模型上端开口,分别引入旋翼下洗气流和前端进气,对比分析了这两种状态下模型壁面温度和红外辐射强度的大小。结果表明:引入速度为18 m/s的旋翼下洗气流使得模型壁面内外两侧均受到冷却气膜的保护,从而使壁面温度降低了36%;同时再引入流量为0.2 kg/s的前端进气,可使红外抑制器模型在3~5μm和8~14μm的红外辐射强度分别降低为原来的11%和28%。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

小突片对热射流红外辐射的影响研究

实验研究了收敛喷管在高温（约913K）、高速（超临界）流动状态下，加装小突片后对热排气的红外辐射抑制特性，并探讨了小突片安装片数、后倾角度、堵塞比等因素对红外辐射抑制特性的影响。结果表明，小突片对热排气的红外辐射具有明显的抑制作用，与不装小突片的相比，不仅使热排气的核心区长度大为缩短，而且使热排气的总体红外辐射信号大幅度下降（在实验范围内，最大可下降约73％）。     

红外隐身材料的现状与展望

综述了国内外红外隐身材料的发展历程，重点介绍了构成红外隐身材料的填料、树脂的研究现状以及近年来开始重点研究的红外兼容型多频谱隐身材料，并且指出了红外隐身材料的发展方向。     

调频连续波SAR成像算法研究

机载遥感微波成像雷达在地球观测特别是在城市应用中起着非常重要的作用,现在人们对体积小、重量轻、成本效益高、分辨率高的成像雷达越来越关注。调频连续波(FM-CW)技术和SAR相结合的调频连续波合成孔径雷达应运而生。论文详细分析了FM-CW SAR的成像过程,提出了去除相位残余的算法,并给出仿真结果。通过仿真可以看出,调频连续波合成孔径雷达具有较好的空间分辨力。     

先进的超声可视化成像检测技术及其应用

通过先进的可视化成像检测技术可以准确地获取材料及其结构内部缺陷大小、位置以及三维分布特征。在众多的可视化成像无损检测方法中,超声成像检测方法是一种已经在复合材料、焊接等领域得到广泛应用的可视化成像检测技术,通过超声B-、C-、T-扫描以及三维投影成像,可以揭示材料及其结构中缺陷和微结构的三维量化分布。本文介绍了基于超声成像检测方法的典型检测应用及结果。