一种紧固孔细节原始疲劳质量评定方法

 给出了一种由等幅载荷试验的断口金相数据反推得到的当量初始裂纹尺寸额定值（EIFSR）表征的紧固孔原始疲劳质量评定方法。并据此建立了原始疲劳质量符合性检查的EIF-SR判据和寿命判据。最后用上述判据对紧固孔细节进行了原始疲劳质量评定和符合性检查。     

提高企业标准化人员素质刍议

以企业市场竞争能力与标准化工作的关系为切入点，论述了在市场经济条件下，如何提高企业标准化人员的素质问题。     

企业自我评价方法的层次模型

通过分析比较ISO9000:2000标准和质量奖模型,对应马斯洛的需求层次提出了企业自我评价方法的层次模型,揭示了ISO9000标准和质量奖模型作为企业自我评价方法的层次逻辑关系,即两者互相补充,一方面以ISO9000标准为基础,通过PDCA循环反映企业运作的变化和改进;另一方面,在ISO9000标准的基础上通过质量奖准则,找出企业优势,在此基础上,继续改进.     

高校教师教学质量评价体系及方法初探

教学质量是高校的生命线。但由于在考核制度中片面强调科研的重要性，缺乏科学的教学质量评价体系和方法。很多高校教师对教学投入的主动性和积极性不高，教学质量的监控已经是高校管理中一个很棘手的难题，教学质量的下滑已成为人们普遍关心的问题。根据当前高校教师教学质量评价体系和方法的现状，提出了高校教师教学质量评价体系的全面性和综合性，教学质量评价方法的多维性和动态性的观点。     

空乘专业大学生的人格特征与职业素质分析

采用16PF和UPI量表对176名空乘专业大学生进行测评,发现有中度以上心理障碍的人数占8．40％;焦虑值偏高的人数占20．45％;适应性和成长性偏低的人数占33．50％。该群体的职业素质不能适应现代民航空服职业发展的要求。其主要问题是：缺乏认真负责的精神、意志水平不高、对社会信任不足、感情用事、自律不足、依赖性强、缺乏独立工作和应变能力。对该专业大学生加强责任意识、培养合作精神、树立人生目标的职业素质教育显得尤为重要。     

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.     

铝-锂合金的真空熔炼

 在ZG-25型中频感应真空炉中进行了铝-锂合金的熔炼与铸锭。真空度为66Pa。考察了普通石墨坩埚、氧化铝坩埚,以及氧化锌涂料、氮化硼涂料与铝-锂熔体的反应。抄到了在真空下控制铝-锂熔体中锂含量的方法。在不使用钛-硼细化剂的条件下,铸锭呈细小等轴晶组织,其成分均匀,夹杂物极少。真空熔炼可使合金中的氢、钾,钠等杂质含量显著地降低。     

质量师系统与型号研制RMSS方案论证

阐述了型号质量师系统参与型号研制方案论证的必要性,着重探讨了型号质量师参与型号可靠性、维修性、安全性和保障性(RMSS)方案工作的内容和要求,以及做好方案论证工作,对建立型号研制RMSS监控的指导意义。     

关于发展学生党员质量保证体系建设的思考

建立发展学生党员质量保证体系,有利于科学规范发展学生党员的操作程序、加强学生党员管理和提高党员队伍整体素质。     

彩色三维激光快速成型技术的研究

目前逆向工程采用线结构激光和一个彩色面阵CCD摄像机构成三维彩色扫描系统,彩色CCD摄像机分两次对被测物体成像,首先摄取物体的彩色图片,然后加用滤光片再摄取激光光平面上的三维信息.最后将两次获取的信息重叠,便可得到三维彩色信息.提出了激光光平面方程式三维测量方法,建立了相应的数学模型.研制成一套适用于彩色逆向工程流程,并进行了实验研究,给出了实验结果.