基于SPSS因子分析的舰载机航材保障风险因素分析

为做好舰载机航材保障风险管理工作,必须对其可能存在的风险因素进行深入、细致的分析,查找出其关键风险因素并研究风险因素之间的关系。因此,文章在依据舰载机航材保障风险因素初步识别结果的基础上,通过调查问卷的方式,归纳总结出21个舰载机航材保障风险因素,并利用SPSS统计软件和因子分析法对调查问卷的结果进行分析和计算,最终提炼出具有代表性的7个公共因子,从而完成了舰载机航材保障关键风险因素的确定和分类。     

炭纤维壳体封头设计的几个问题

讨论了炭纤维壳体封头低压破坏的原因及3种破坏模式,即靠近赤道附近部位的封头发生断裂,极孔部位在环向应力作用下断裂和封头沿接头肩部外缘被剪(弯)断;得到了3种破坏模式的强度校核公式.给出了防止封头破坏宜采取的有效措施,对开孔很大的后封头,宜采取补强措施;给出了补强层厚度和补强范围的确定方法.     

动态扭矩遥感测试系统校准方法研究

介绍了一种动态扭矩遥感测试系统的工作原理及其应用,提出了针对该类动态扭矩测试系统的校准原理,并介绍了具体的校准方法.     

对银行信贷风险形成因素的分析

银行信贷风险是重要的金融风险，笔者对银行信贷风险形成机理和因素作了较详细地分析。     

平均电流型功率因子校正电路的研究

研究一种新的功率因子校正器件ＵＣ３８５４的基本原理，技术特点，着重讨论功率因子校正电路物工作原理及设计要点，并给出一个２ｋＷ样机的验证结果。     

基于DDA的强度折减法求土坡安全系数

介绍了非连续变形分析(DDA)方法和强度折减法的基本理论,提出了基于DDA的强度折减法求土坡安全系数的方法。分析了在计算连续介质时块体的划分方法,提出应预先根据费伦纽斯经验方法假定土坡潜在滑动面的位置和形状,依据强度折减法,分别求出各条滑动面在失稳破坏时的折减系数,即为此条滑动面的安全系数。然后绘曲线找出最小值,即为土坡的稳定安全系数。提出了DDA法判定土坡失稳破坏的标准,通过算例证明了此法在计算土坡稳定安全系数时的可行性,所得到的安全系数较其他几种方法偏小。     

显微硬度工作基准装置测量不确定度评定

基于显微硬度的数学定义公式 ,对建立的数显式显微硬度工作基准装置的测量不确定度进行了评定。     

试析体育教学对大学生非智力因素的培养

非智力因素在人的成才过程中起重要作用,对培养富有创造性思维的创新人才具有重要的战略意义。体育教学在培养大学生非智力因素中起着积极作用,为此针对体育教师如何结合教学培养学生的非智力因素提出建议。     

Comparison of the mean quality factors for astronauts calculated using the Q-functions proposed by ICRP,ICRU, and NASA

For the estimation of the radiation risk for astronauts, not only the organ absorbed doses but also their mean quality factors must be evaluated. Three functions have been proposed by different organizations for expressing the radiation quality, including the Q(L), Q(y), and Q_NASA(Z, E) relationships as defined in International Committee of Radiological Protection (ICRP) Publication 60, International Commission on Radiation Units and Measurements (ICRU) Report 40, and National Aeronautics and Space Administration (NASA) TP-2011-216155, respectively. The Q(L) relationship is the most simple and widely used for space dosimetry, but the use of the latter two functions enables consideration of the difference in the track structure of various charged particles during the risk estimation.     

Calculation of the effect of opacity in the solar spectral lines of carbon ions

In this paper, using the intensity ratio of carbon ions emission lines, we determined the optical depths at the line center of the CI at about 165.7 nm, CII at about 133.5 nm, CIII at about 117.5 nm and CIV at about 154.9 nm emission lines by escape factor treatment. For CI and CII emission lines, we discuss the intensity ratio of two lines arising from the common upper levels; while for CIII and CIV emission lines, we discuss the intensity ratio of two lines arising from the common lower levels. By introducing the measured abundance of carbon and the results of ionization balance calculations, we make an estimate of the line-of-sight physical thickness of the regions of carbon ions. This discussion will provide some results in the discussion of opacity on the solar ultraviolet (UV) or extreme-ultraviolet (EUV) spectrum.