一种融合个体属性与社交关系的民航旅客价值度量方法

针对目前民航旅客关系网络中旅客关系类别单一、旅客价值计算滞后、旅客潜在价值计算没有考虑旅客之间的相互影响,使得一些具有极大消费潜力的旅客因为目前乘机次数较少而被航空公司忽略的现状,提出了一种融合个体属性与社交关系的民航旅客价值度量方法,采用RFM_c模型计算旅客个体价值,并采用多关系评价（MRE）模型分析旅客关系,然后通过改进的PageRank算法设计实现融合旅客个体价值和社交关系的民航旅客价值排序（CAPV-Rank）算法,实现旅客价值度量、旅客价值预测和潜在高价值旅客挖掘。实验结果表明：设计实现的CAPV-Rank算法可通过调整权重因子实现多种模式下的旅客价值计算,满足各种业务需求,并能实现旅客价值预测、潜在高价值旅客挖掘,旨在为民航旅客价值度量和预测提供灵活、高效的解决方案。     

独立桨距控制对直升机飞行性能的影响

为研究旋翼独立桨距控制对直升机飞行性能的影响,在已验证的直升机性能分析模型基础上,以UH-60A直升机为样例,通过输入不同阶次、幅值和相位角的独立桨距,分析直升机的需用功率和升阻比变化,在此基础上给出了旋翼桨盘内迎角和阻力系数的分布,探讨了独立桨距控制提升直升机性能的机理。分析结果表明：高速时,2阶和3阶的独立桨距控制可降低旋翼需用功率、提高直升机的升阻比,但提升效果有限,直升机起飞重量较大时,效果更明显;2阶耦合3阶的独立桨距控制对旋翼性能的提升效果比单独的2阶或3阶桨距输入更好,样例直升机的需用功率最多降低了4.5%,4阶的独立桨距输入则不利于提升旋翼性能;输入独立桨距后,旋翼桨盘迎角分布改善,后行侧迎角减小,有利于推迟失速,桨盘的后行侧的阻力系数减小,可有效降低旋翼的需用功率,提升直升机飞行性能。     

XMM-Newton observations across the Cygnus Loop from northeastern rim to southwestern rim

We have observed the Cygnus Loop from the northeast (NE) to the southwest (SW) with XMM-Newton. We extracted spectra from 3′-spaced annular regions across the Loop and fitted them either with a one-kT_e-component non-equilibrium ionization (NEI) model or with two-kT_e-component NEI model. We found that the two-kT_e-component model yields significantly better fits in almost all the spectra than the one-kT_e-component model. Judging from the abundances, the high-kT_e-component in the two-temperature model must be fossil ejecta while the low-kT_e-component comes from the swept-up interstellar medium (ISM). The distributions of Ne, Mg, Si, and S for fossil ejecta appear to retain the onion-skin structure at the time of a supernova explosion, suggesting that significant overturning of the ejecta has not occurred yet. Comparing the relative abundances of fossil ejecta estimated for the entire Cygnus Loop with those from theoretical calculations for Type-II SN, the mass of the progenitor star is likely to be ∼13 M_⊙. The trends of the radial profiles of kT_e and emission integral for the swept-up ISM are adequately described by the Sedov model, suggesting that the swept-up ISM is concentrated in a shell-like structure. Comparing our data with the Sedov model, we found the ambient medium density to be ∼0.7 cm⁻³. Then, we estimated the total mass of the swept-up ISM and the age of the remnant to be ∼130 M_⊙ and 13,000 years, respectively. Note that if the explosion occurred within a stellar wind cavity, then the density in the cavity, the total swept-up mass in the cavity, and the age of the remnant are estimated to be ∼0.14 cm⁻³, ∼25 M_⊙, and ∼10,000 years, respectively.     

苏豫两省城镇居民收入水平及决定因素

从宏观层面对江苏和河南两省城镇居民收入水平的现状进行了比较，并从微观层面对两省城镇居民收入决定因素进行了探究。分析表明，改革开放以来，虽然两省城镇居民收入水平都有大幅增长，但两省城镇居民可支配收入差距呈渐进扩大趋势，江苏城镇居民收入水平大约为河南的1．3-1．4倍，进入21世纪以来，这种收入差距似有缩小态势。基于微观层面的原因探究发现，体现人力资本的教育水平及工作经历，都显著地影响着两省的居民收入水平。而其他一些因素诸如性别、就业单位性质、职业类型等也都不同程度地对居民收入产生影响。     

图象匹配中的仿射透视近似

提出了在图象匹配中使用的一些新的仿射透视近似投影不变量。文中引进了点的仿射透视近似的概念，分析了线段的透视投影与其仿射透视近似间的最大相对误差，获得了一个有实用价值的距离三角形误差判决准则。基于此准则，研究了物体上同一空间平面中，平行线段长度比，同底面积比等仿射不变量，近似用作透视不变量的可能性。实验结果证实了分析的可靠性。     

高职院校ESP教师的角色定位与个体发展研究

以Freeman的语言教师学习理论和Dudley—Evans＆St．John的角色理论为指导,以三所高职院校的ESP教师和部分学生为调查对象,通过问卷调查、个体访谈等研究工具探讨ESP教师在角色定位方面的偏差和个体发展方面的不足,并提出促进个体发展的措施。     

Delayed outburst of H 1743–322 in 2003 and relation with its other outbursts

The Galactic transient black hole candidate H 1743–322 exhibited a long duration outburst in 2003 after more than two and a half decades of inactivity. The 2003 event was extensively studied in multi-wavelength bands by many groups. The striking feature is that the total energy released is extremely high as compared to that in tens of outbursts which followed. In this paper, we look at this event and study both the spectral and temporal properties of the source using two component advective flow (TCAF) paradigm. We extract accretion flow parameters for each observation from spectral properties of the decay phase and determine the mass of the black hole. We computed the energy released during all the known outbursts since 2003 and showed that on an average, the energy release in an outburst is proportional to the duration of the quiescent state just prior to it, with the exception of the 2004 outburst. A constant rate of supply of matter from the companion cannot explain the energy release in 2004 outburst. However, if the energy release of 2003 is incomplete and the leftover is released in 2004, then the companion’s rate of matter supply can be constant since 1977 till date. We believe that erratic behaviour of viscosity at the accumulation radius $X_p$ of matter as well as location the $X_p$ itself, rather than the random variation of mass transfer rate from the companion, could be responsible for non-uniformity in outburst pattern. We discuss several factors on which the waiting time and duration of the next outburst could depend.     

Individual Differences in Representational Precision Predict Spatial Working Memory Span

Perhaps the signature feature of working memory is that it is limited. In the same subjects, we used two different retrieval tasks to independently measure two different limits of spatial memory. Precision was measured by asking participants to localize a missing target item among a field of other targets and distracters. Capacity was measured with a similar task where participants identified, rather than localized, a set of remembered targets from within a larger set of identical items. Across participants, the precision of localization was positively correlated with the number of successfully retrieved items. These data suggest that an individual's representational capacity may ultimately be constrained by their ability to form precise representations of space.     

柔性自供能技术在防护救生领域的应用探讨

柔性自供能技术作为微能源领域新秀,近年来获得长足发展,目前处于实验室向工业技术转化的关键阶段。文中通过对应用场景分析探讨,认为在航空飞行员防护救生领域,柔性自供能技术的主要应用方向是智能穿戴设备的能源供应,具有应用场景广泛、使用方便、可全周期供能等技术优势。文中对柔性自供能技术在防护救生领域实现技术应用面临的问题,给出了对应的解决方案,可以为后续研究工作提供思路：研究制备多效应融合发电器件可实现对环境中多种微能量的广泛收集,可构建全固态柔性超级储能器件,以满足高效储能以及航空环境使用的安全需求,设计充放电并行控制电路以解决全任务场景长时效供能技术难题。