利用栅网控制空间等离子体环境效应模拟中的等离子体参数

通常采用ECR等离子体源产生的等离子体的温度和密度都比较大，通过附加适当目数的栅网，并在栅网上加一定的偏置电位来对等离子体参数，尤其是温度，密度进行调整，满足空间等离子体环境模拟要求，本文利用14目，25目的栅网，对已有的地面实验室空间等离子体环境进行了改进，得到了更加接近空间等离子体参数的一个地面模拟环境。     

微波等离子推力器真空实验研究

微波等离子推力器(MPT)具有寿命长、效率高和比冲高的特点，具有广泛的应用前景。通过对MPT真空实验系统，以及中(-lkW)、低(-l00W)功率MPT结构的介绍，重点论述了MPT在真空环境下的启动和稳定工作特性，并对实验结果进行了分析和讨论，给出了MPT初步性能参数。实验结果表明，在30W-lkW功率范围内，MPT真空环境下启动可靠，工作稳定；氦气(He)的比冲远高于氩气(Ar)的比冲。     

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。     

铜基高温钎料中钴作用机制的研究

探讨了Cu-Zn-Mn-Co钎料中钴的变质剂作用机理,为高温钎料的研制提供了实验基础研究。     

混粉电火花加工表面的研究

分析了混粉电火花加工工件表面的组成成分,探讨了混粉电火花加工获得低的表面粗糙度的机理。     

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。     

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。     

热处理对大气等离子喷涂纳米结构YSZ热障涂层晶粒长大的影响

采用大气等离子喷涂制备了纳米结构氧化钇稳定的氧化锆热障涂层。运用SEM ,TEM和XRD等方法研究了涂层和原料粉末的微观结构和相组成。结果表明 ,喷涂过程中平均晶粒大小由4 0nm变为 6 7nm ,涂层主要由亚稳四方相组成。涂层热处理结果显示 ,90 0℃以下晶粒长大速度缓慢 ,然而 1 0 0 0℃以上晶粒长大速度迅速增加 ,而且出现较多的单斜相