民用飞机个人通风送风温度对人体舒适性的影响

通过对某真实客机座舱进行建模，使用计算流体力学（CFD）的方法计算出不同个人通风送风温度下座舱内的温度场和流场分布。然后提取乘客头部区域温度与试验结果进行对比，验证模拟的可信度。最后结合基于人体平均皮肤温度的热舒适评价方法，对不同个人通风送风温度情况下的乘客舒适性进行研究。结果表明：不同个人通风送风温度对乘客头部区域温度影响较小，随着个人通风送风温度从7℃上升到14℃，乘客头部区域温度变化不超过0.8℃。不同个人通风送风温度对乘客平均皮肤温度以及热舒适性的影响较小，随着个人通风送风温度从7℃上升到14℃，目标乘客平均皮肤温度上升0.33℃。     

面向Flash存储器的FAT文件系统可靠性增强机制

FAT文件系统针对Flash存储器使用时,其FAT表存储位置不确定且各个簇之间的擦写次数不均衡,导致其可靠性降低.针对上述问题,提出了两种解决方案,分别是FAT表可控迁移和空闲簇磨损均衡.前者在Flash上预留多个块存储FAT表,每次更新FAT表时在其中选择擦除次数最小的块,预留一个块记录最新FAT表的入口地址;后者在Flash上预留一个块记录FAT表中各个簇的擦写次数,每次分配空间时选择擦写次数小于擦除阈值的空闲簇.测试结果表明,改进后的FAT文件系统能够在可控范围内可靠地存储FAT表,同时有效地均衡了各个簇的擦写次数,这些都增强了FAT文件系统的可靠性.     

Reverberation time lags in the high luminosity quasar PG 1247+267

Virial estimates of the black hole mass in the center of AGNs, derived from single-epoch observations of luminosity and emission line widths, are now available for several thousands of objects at all redshifts and luminosities, so that studies of the cosmological evolution of the AGN mass function are becoming possible. These estimates are based on the empirical luminosity-size relation measured through reverberation mapping at low redshifts and luminosities. For this reason the spectrophotometric monitoring of 4 luminous quasars was started in 2003, with the 1.8 m telescope of the Asiago Observatory. To measure the reverberation time lag we adopt a method, recently introduced by Zu et al. (2011), which takes advantage of the available statistical information on variability autocorrelation and makes simple assumptions on the continuum-emission line transfer function. We present the estimate of the broad line region size for the quasar PG 1247+267, which is the most luminous object with reverberation measures to date. Virial products computed for C iv and C iii] emission lines provide consistent results. A possible flattening of the size-luminosity relation for C iv at high luminosity is suggested.     

基于修正Rife算法的脉冲回波相参积累算法

针对目标径向运动导致回波在波门内出现距离走动的情况,提出了一种针对径向匀速运动目标回波信号长时间相参积累的方法。该方法根据傅里叶变换的时移性质——不同时刻回波频谱相关序列的频率包含了各回波到达的时间延迟,通过修正Rife算法估计此时间延迟,最终确定并补偿各个回波的距离走动分量。仿真结果表明:提出的方法可以有效补偿各回波间的距离走动;信噪比低至-6dB时,算法的性能即可达到最优;补偿后积累信号的信噪比可以达到理想积累情况下的93%。     

Integrated Framework for Understanding Relationship Between Human Error and Aviation Safety

Introducing a framework for understanding the relationship between human error and aviation safety from multiple perspectives and using multiple models. The first part of the framework is the perspective of individual operator using the information processing model. The second part is the group perspective with the Crew Resource Management （CRM） model. The third and final is the organization perspective using Reason＇s Swiss cheese model. Each of the perspectives and models has been in existence for a long time, but the integrated framework presented allows a systematic understanding of the complex relationship between human error and aviation safety, along with the numerous factors that cause or influence error. The framework also allows the identification of mitigation measures to systematically reduce human error and improve aviation safety.     

非英语专业本科生学习风格探究及启示

研究学习风格和英语学习成绩之间存在的关系。利用PLSPQ对河南省洛阳市三所高校的479名非英语专业二年级学生进行调查问卷,以学生的四级成绩为依据,分析其学习风格总体状况及其偏好以及在学习风格上所呈现出的差异。结果表明,非英语专业本科生触觉型学习风格的倾向性最为明显,听觉型学习风格倾向最弱,就学习风格而言,英语学习成绩优异者与成绩较差者存在较为明显的差异。结论是学习风格与学习成绩之间并没有显著的关系。     

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.     

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。     

星载合成孔径雷达快视成像

通过对星载合成孔径雷达 (SAR)原始回波信号的分析 ,推导出星载SAR快视成像算法 (SPECAN算法 ) ,并分析了SPECAN算法的主要难点。最后用SPECAN算法对实际星载SAR回波数据进行成像 ,进一步验证了用SPECAN算法进行快视成像的高效性。