微束等离子焊接钛合金薄板保护规律的研究

 通过试验认为微束等离子焊接钛合金薄板的保护问题,关键在于控制施焊时焊缝处于700℃以上的加热范围,和700℃到400℃的冷却时间。并论证了以氧的污染层厚度作为钛合金焊接污染程度判据的合理性。本文采用电子探针法对氧污染层厚度进行了测定,求出污染方程。从而。使微束等离子焊接钛合金薄板的污染问题,可通过调整焊接规范进行控制。     

超视距舰空导弹爬升段弹道设计

针对超视距舰空导弹中制导的爬升段,采取两段程序圆弧相结合的方法设计弹道,给出了导弹爬升段的高度与倾角指令,并对于在圆弧间及弧与高空平飞段两转接点处出现的抖动现象,通过改变转接基准并做必需的导引指令修正,有效地解决了抖动问题。最后的仿真结果验证了所设计导引律的可行性和对于消除抖动问题所做措施的有效性。     

超声速叶型前缘几何形状对叶栅气动性能的影响

应用NURBS技术构造超声速叶型,采用两个控制参数调整叶栅前缘椭圆弧的几何形状,来探索不同的前缘构型对超声速叶型气动性能的影响效应;通过对比分析调整每个参数所得的一系列叶栅的流场计算结果,发现椭圆弧的形状控制因子对超声速叶栅的前缘激波和气流流动状况具有一定的改善效果,同时在保证叶栅气动弦长基本不变的情况下,存在某个椭圆弧形状控制因子和方向控制因子的匹配能够使叶栅的气动性能达到最佳.     

模型烧蚀对尾迹电子特性影响的计算和实验研究

 基于气动物理研究的需要，针对高焓风洞的来流特点，采用计算和实验相结合的方法研究聚丙烯烧蚀对尾迹电子密度的影响。结果表明：计算结果可以有效模拟实验状态，电子密度的模拟精度有很大提高，误差在一个量级内；聚丙烯烧蚀可以降低尾迹的电子密度，但幅度不大，在2倍左右，其与选择模型材料的催化特性降低幅度相当；对电弧风洞的成功改进和非稀薄流静电探针诊断技术的应用，是尾迹电子密度测试的前提保障。     

吸气模式激光推进空气等离子体光谱

利用实验室自行研制的紫外预电离CO2激光器进行了激光等离子体实验,实验采用底面直径均为60mm,焦距分别为5 mm和10 mm的两种抛物面光船。介绍了激光等离子体光谱和明显的特征谱线,以及激光等离子体温度估计模型;分析了两种光船对激光等离子体的影响。实验表明:相同底面直径10 mm焦距光船产生的等离子体信号峰值和持续时间均略大于5 mm焦距光船;10 mm焦距光船产生的等离子体温度明显高于5 mm的,最大温度产生时间比5 mm光船要晚一些。     

用于激光推进的球隙火花开关放电特性的研究

在自行研制的高压球隙火花开关上,研究短间隙下(6 mm)不同工作气压、不同冷却气体速度对开关工作电压范围、延迟时间和抖动时间的影响及规律。结果表明:提高气压能扩大工作电压范围,增加开关的时延;吹气能够降低开关的时延,但增加开关的抖动时间。在本实验条件下,将开关工作气压从1×105Pa提高到2×105Pa,工作电压范围扩大了50%以上,但开关的时延增加了20 ns,抖动增加了10 ns;有气体冷却时开关的延迟时间比起无吹气时要小几十个纳秒。     

01420铝锂合金的搅拌摩擦焊接

对2 mm厚的01420铝锂合金薄板实现了搅拌摩擦焊接(FSW),分析焊接接头的微观组织形态,研究焊接工艺参数对搅拌摩擦焊接接头成型和接头性能的影响,并与氩弧焊接接头性能相比较.结果表明,当工艺参数选取得当时,焊缝成型较好,表面光洁,焊接接头的强度可达到母材强度的77%,接头的弯曲角可达到180°,均高于氩弧焊接接头.     

等离子体表面技术的研究与应用

概述了离子注入、离子束沉积、等离子喷涂、离子镀、等离子体增强化学气相沉积、等离子体化学热处理和双层辉光离子渗金属等等离子体表面技术的基本原理和最新进展,并给出了部分典型实例。     

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.     

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。