基于8098单片机的飞行指引系统综合测试装置

介绍一种基于8098单片机的飞行指引系统综合测试装置，给出了飞行指引系统综合测试装置的用途。主要硬件组成和软件设计方法。     

直升机旋翼试验台数据采集系统的改进与设计

本文详细介绍了直升机旋翼试验台数据采集系统的功能，硬件配置以及软件设计方法。     

二元外压式进气道斜板和唇口参数选择的风洞试验研究

在几何不可调的二元外压式斜板进气道的设计中，选择合理的斜板和唇口几何能数是最重要的问题之一。本文对一个设计马赫数为１．８的这类进气道的斜板和唇口参数进行了风洞试验研究。用缩尺模型风洞试验，对比分析了不同斜板角和不同外侧唇口内唇角，唇缘半径对进气道内流特性的影响，结果表明，对确定的进气道布局，斜板角小的变化对进气道超音速内流总压恢复系数，稳态出口流场周向畸变指数及喘振裕度的影响很大，唇口参数小的改变     

起落架落震试验的数字模拟方法

 <正> 在计算飞机起飞、着陆和滑行等地面运动的静、动态载荷时,除了需要飞机结构和气动参数外,起落架减震器的性能参数更占有重要地位。而这些性能参数中尤以决定油液阻尼力的流最系数为重要。长期以来,国内主要靠查手册、凭经验确定这个系数,如果能较准确地确定流量系数,对载荷计算是很有意义的事。     

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.     

卫星故障诊断的最优奇偶向量法

 提供一种卫星故障诊断方法以提高 GPS导航的完整性。该方法利用最优奇偶向量来检测和诊断卫星故障以提高卫星故障诊断的准确性。仿真结果显示,在故障幅值较小的情况下最优奇偶向量方法相比广义似然比方法可以提高故障的正确检测率和正确诊断率。该方法还可以缩短检测斜坡型故障的时间,从而提高了系统的可靠性。     

电磁兼容技术

介绍了电磁兼容技术的产生及其发展现状 ,重点介绍了当前的电磁兼容预测技术以及工程实现电磁兼容的主要方法。探讨了电磁兼容领域面临的问题以及当前的主要研究方向。     

直升机燃油系统地面模拟试验中试验台转角与油面角的关系

为了在直升机燃油系统地面模拟试验中准确地模拟油面角，本文介绍了试验台转角与油面角的关系，并给出了转换结果，同时，提出了一种用油箱内增压来模拟过载的设想，使在模拟试验时，油泵供油更趋真实，通过简化计算，给出了确定气压力的方法和判断依据。     

直升机尾桨故障及其试飞研究

介绍了直升机尾桨故障类型及其处理方法和试飞方法。探讨了发动机功率、空速、飞行高度等因素对尾故障试飞的影响。在实际试飞的基础上，给出了正确处理尾桨故障的基本方法，为直升机飞行员在飞行时遇到类似故障后的处理及有关研究人员提供了重要的参考。     

数字化机载环控地面检测系统的研究

通过采用两片PIC18F448及其外围器件实现了机载环控地面检测系统的数字化设计。通过I^2C总线实现两片单片机之间的数据传输与协调，并利用其CAN接口模块实现多套检测系统的网络化和远程控制操作。