螺旋弹簧局部振动频率分析与控制

本文首先讨论了单螺旋弹簧局部振动的固有频率的计算方法，在此基础上进一步建立了串联、并联弹簧局部振动的分析模型，并探讨了弹簧局部振动频率的控制方法。     

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.     

考虑飞行强度影响的飞机使用寿命综合评定方法

介绍了针对军用飞机普遍存在的使用寿命指标(飞行小时数、日历寿命)严重不匹配的问题,在现有技术和理论基础上利用腐蚀影响系数m(t),引入飞行强度参量SUS建立了军用飞机使用寿命综合评定方法。算例分析表明,随着飞行强度的提高,腐蚀疲劳寿命NC成线性增加,并得到了协调飞机使用寿命指标的最佳飞行强度SUSbest,为合理制定飞行计划,充分发挥军用飞机的使用功效提供了理论基础。     

正弦波模型化测量方法及应用

本文对应用较多的几种正弦波模型化测量方法进行了综述，它们是曲线拟合法、直方图统计分析法、FFT法和拍频法。较详细地介绍了这几种测量方法的典型用途以及特点，通过比较几种方法的优缺点，讨论了它们应用中的局限性。     

MATLAB电力系统模块中频谱分析的实现

给出了利用电力系统模块(PSB)工具箱对仿真波形进行频谱分析的一种新方法.该方法以MATLAB提供的PSBFFT_SCOPE函数为基础,对其输入变量加以改造,克服了其不能应用于变步长算法模型频谱分析的缺陷,拓宽了在PSB工具箱中进行频谱分析的范围.实际仿真结果表明,该方法分析正确,使用简捷,在实际仿真过程中是切实可行的.     

低频电动振动台的关键技术

简要介绍了低频电动振动台校准系统的结构和工作原理，分析了其存在非线性的原因。针对这些因素提出了在整个系统特别是对其核心——低频电动振动台的研制设计过程中应采取的措施、改进的方法和关键技术。     

冷等离子体处理对碳纤维缝编织物/环氧复合材料界面性能的影响

采用冷等离子体对碳纤维缝编织物进行表面处理 ,并采用XRD对处理前后的碳纤维表面结构进行了分析 ,研究了冷等离子体处理对浸润性以及碳纤维缝编织物 /环氧复合材料的层间剪切强度的影响。实验结果表明 ,冷等离子体处理提高了碳纤维表面活性、浸润性 ,从而改善了碳纤维缝编织物 /环氧复合材料的界面粘结性能 ,进而改善了复合材料的界面性能。     

带减振器的光纤陀螺惯导系统有限元仿真建模方法

以某光纤陀螺捷联惯导系统的IMU单元为研究对象,利用有限元分析软件包Patran/Nastran建立了含减振器的IMU系统有限元模型。重点介绍了有限元模型中减振器的等效处理方法,比较了模型的随机振动响应计算结果和样机振动试验的实测结果,两者的误差在3.2%以内,证明了有限元建模过程中所使用的减振器等效处理方法的合理性。     

高超声速再入体烧蚀流场计算分析

从化学非平衡NS方程或其简化形式(粘性激波层方程、PNS方程)出发,求解高超声速再入体的绕流和底部尾流流场。首先讨论了碳基材料烧蚀壁面条件的确定方法,计算了包含和不包含碳-碳烧蚀产物的再入体半球的化学反应绕流流场,并和文献结果进行了对比。在此基础上,计算了两个高度条件下,包含和不包含碳-酚醛烧蚀产物的再入小钝锥的绕流和尾流流场,分析了烧蚀产物对流场电子数密度、温度等流动参数的影响。     

TES系统中的频率变换及有关参数的设置

在中国民航电话地球站（ＴＥＳ）系统中，远端站所用的室外单元（ＯＤＵ）有两种：ＥＦＤＡＴＡ型和ＨＮＳ的Ｖ２型，这两类站在有关频率参数设置上是不同的，这涉及到系统内的频率变换方法。结合这两类站有关参数的设置，详细分析了ＴＥＳ系统的频率变换过程及特点。