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。     

新型阻燃Ti40合金TIG焊焊接性能研究

研究新型阻燃钛合金Ti40合金的TIG(tungest inert gas)焊焊接性能,采用金相、SEM等方法分析Ti40合金焊缝及热影响区的组织变化.结果表明,Ti40合金钨极氩弧焊焊缝室温、高温拉伸性能良好,冲击性能较低.焊接之后的热处理制度对组织有一定的改善.经500℃×100h热暴露后,晶界粗化,为连续α相.     

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.     

时效处理对T-250钢电子束焊接接头组织及性能的影响

采用金相显微镜、透射电镜观察了焊后不同时效状态下T— 2 5 0马氏体时效钢电子束焊缝的微观组织 ,测试了不同时效状态下焊接接头的室温强度、夏比缺口冲击韧性、显微硬度 ,并用扫描电镜分析了拉伸断口形貌。结果表明 :随时效温度的升高 ,焊缝区枝晶间逆转奥氏体析出量增加 ,焊缝缺口冲击韧性增大 ,断口韧窝增大 ;但由于 5 0 0℃× 4h时效处理后焊缝马氏体孪晶较多而使其拉伸强度和缺口冲击韧性降低。经 4 80℃× 4h时效处理后 ,焊接接头强度具有最佳强韧性配合     

大厚度铝合金飞行器结构的焊接

介绍了采用熔化极脉冲氦弧焊工艺焊接大厚度铝合金燃料箱的优越性。     

接触焊机理的探索

探讨了接触焊的机理，提出了以电位差选择电极材料的原则，以及焊接处的接触电阻和母材内阻在焊接中有一定作用，而且焊接处的总热能是各种能量产生的热量之和，焊接的总热量也应包括通电加热产生的热量和断电后（锻压时）产生的热量。     

GH4169高温合金惯性摩擦焊接头动态再结晶过程

当温度、应变、应变速率达到一定条件时 ,GH4 16 9镍基高温合金在惯性摩擦焊接过程中易发生动态再结晶。本文研究结果表明 ,由于GH4 16 9合金惯性摩擦焊接时间很短 ,动态再结晶进行得相当充分 ,而动态回复不足 ,在动态再结晶的过程中还可以看到有些结晶过程还处于形核阶段 ,这是惯性摩擦焊接头产生细晶乃至超细晶的根本原因     

Ti-24A1-17 Nb合金的激光焊接

研究了Ti-24Al-17Nb合金的激光焊接及其接头的力学性能.研究结果表明,连续激光氦气双面保护可以获得保护效果可靠、无缺陷、成型良好的焊接接头.焊接热输入增大不利于接头的纵向弯曲塑性,而接头的横向拉伸强度与母材基本相同,塑性可以接近母材的塑性,达到14%～17%.     

粉末高温合金FGH96惯性摩擦焊接头常温力学性能分析

第二代粉末高温合金FGH96是采用损伤容限设计思想研制的新型粉末高温合金,是当前750℃工作条件下满足高推比、高燃效发动机使用要求的涡轮盘、环形件和其他热端部件的理想材料.结合FGH96惯性摩擦焊接头的组织特征和强化相γ′数量分析接头的显微硬度和常温拉伸性能.结果表明,FGH96惯性摩擦焊接头具有良好的常温力学性能.     

一类特殊的改进捕错译码

捕错译码是传码率满足Ｒ＜１／ｔ的循环码译码最简单的方式，其中ｔ是所能纠错误数的最大值，Ｒ是传码率。这类码传码率低，纠错少。嵩钟雄运用覆盖多项式的概念得出了传码率不满足Ｒ＜１／ｔ的二进制循环码的改进捕措译码方法。本文找到了嵩钟雄译码器的一个子类－－一类特殊的改进捕错译码器。作者的译码器同捕错译码器一样易于硬件实现，并且能够用于传码率不满足Ｒ＜１／ｔ的情况。对于纠错码，作者找到了适合于这一译码器的码判