正极粉中钙含量的测试技术

提出了一种N2O-C2H2火焰原子吸收光谱法测试热电池正极粉中钙含量。并对样品消化处理条件和干扰因素进行了综合考虑。该方法具有很好的灵敏度、很好的重现性、同时具有方法步骤简单,操作容易掌握,干扰少等特点。测试样品钙含量,相对标准偏差均小于1.0%(n=10),标准加入回收率均在97.0%~102.0%(n=6)范围。达到了实验室的仪器分析质量与测试技术质量控制要求。     

Crashworthiness analysis of aircraft fuselage with sine-wave beam structure

An integrated design concept for crashworthy fuselage using sine-wave beam and strut is proposed and investigated. The finite element model of aircraft fuselage is built first. The structures above cabin floor, occupant and seat are simplified as two rigid blocks. The fuselage frame is redesigned, and the sine-wave beam is arranged under the frame. The impact dynamic performance of the aircraft with bottom sine-wave beam structure is studied and compared with that of conventional type. To obtain better crashworthiness performance, different rigidity of strut is combined with the sine-wave beam bottom structure. Numerical simulation result shows that the proposed sine-wave beam bottom structure could not only dissipate more proportion of impact kinetic energy but also reduce the initial peak acceleration. The structure and rigidity of strut have great influence on the crashworthiness performance. To give a better fuselage structure, both of the strut and bottom structure should be properly integrated and designed.     

亚毫米波大气传输计算及分析

主要研究了在近亚毫米波段的大气传输特性，通过分析红外区和毫米波区的大气２模型，给出了亚毫米波段的大气传输模型参及加权项的表达形式。在吸收模型的理论的基础上，推导了以宏观气象条件为参变量的解析表达式，并由实验数据加权后的模型进行了验证分析，加权模型与实验数据基本吻合。在散射模型中，提出了以粒子的统计分布均值代替一般的密度分布，从而提高了计算精度。分别推导了Ｍｉｅ和Ｒａｙｌｅｉｇｈ散射系数求解的数学表     

活笥银粉中微量铜铁的测定

提出用空气－乙炔火焰原子吸收光谱法来测定银锌电池活性银粉中的微量铜铁，并对测定条件和干扰因素进行了综合考虑，该测定方法具有灵敏度、精确度高，干扰小，选择性和重现性好等优点。测定样品微量铜铁含量的相对标准偏差均小于１.5%(n=8）。标准加入回收率均在（９７.00-102.00)%(n=5)范围内，完全适用于银锌电池活性银粉中微量铜铁含量的控制和样品系统分析，实际应用中取得了很好的效果。     

铆钉间距对二维SRAM蒙皮隐身性的影响分析

首先分析了二维电磁散射问题的有限元算法理论,编写了相应计算程序;然后对一布置有两铆钉的二维SRAM蒙皮模型在铆钉间距为20、40和60mm情况下计算分析了铆钉间距对其隐身性能的影响,结果显示铆钉间距越大,蒙皮结构的隐身性能越好。     

太阳活动区R9077引起的强烈吸收事件

利用南极中山站的观测数据分析了太阳活动区R9077所引起的强烈吸收事件，其中2000年7月14日的太阳质子事件引起了持续3天多强烈的极盖吸收，同时，激烈的太阳活动使磁层处于极度扰动状态，磁层高能粒子沉降使许多持续时间较短的吸收峰叠加在极盖吸收背景之上，最突出的是7月1日的吸收增强事件，其最大值达26dB。这是自1997年2月中山站安装成像式宇宙噪声接收机以来观测到的最强的吸收，另一个较突出的吸收峰发生在14日1753UT前后，本文还讨论了产生这些吸收的原由。     

Numerical Simulations of the Warm-Hot Intergalactic Medium

In this paper we review the current predictions of numerical simulations for the origin and observability of the warm hot intergalactic medium (WHIM), the diffuse gas that contains up to 50 per cent of the baryons at z∼0. During structure formation, gravitational accretion shocks emerging from collapsing regions gradually heat the intergalactic medium (IGM) to temperatures in the range T∼10⁵–10⁷ K. The WHIM is predicted to radiate most of its energy in the ultraviolet (UV) and X-ray bands and to contribute a significant fraction of the soft X-ray background emission. While O vi and C iv absorption systems arising in the cooler fraction of the WHIM with T∼10⁵–10^5.5 K are seen in FUSE and Hubble Space Telescope observations, models agree that current X-ray telescopes such as Chandra and XMM-Newton do not have enough sensitivity to detect the hotter WHIM. However, future missions such as Constellation-X and XEUS might be able to detect both emission lines and absorption systems from highly ionised atoms such as O vii, O viii and Fe xvii.     

Modelling the effects of microgravity on the permeability of air interface respiratory epithelial cell layers

Although it has been suggested that microgravity might affect drug absorption in vivo, drug permeability across epithelial barriers has not yet been investigated in vitro during modelled microgravity. Therefore, a cell culture/diffusion chamber was designed specifically to accommodate epithelial cell layers in a 3D-clinostat and allow epithelial permeability to be measured under microgravity conditions in vitro with minimum alteration to established cell culture techniques. Human respiratory epithelial Calu-3 cell layers were used to model the airway epithelium. Cells grown at an air interface in the diffusion chamber from day 1 or day 5 after seeding on 24-well polyester Transwell cell culture inserts developed a similar transepithelial electrical resistance (TER) to cells cultured in conventional cell culture plates. Confluent Calu-3 layers exposed to modelled microgravity in the 3D-clinostat for up to 48 h maintained their high TER. The permeability of the paracellular marker ¹⁴C-mannitol was unaffected after a 24 h rotation of the cell layers in the 3D-clinostat, but was increased 2-fold after 48 h of modelled microgravity. It was demonstrated that the culture/diffusion chamber developed is suitable for culturing epithelial cell layers and, when subjected to rotation in the 3D-clinostat, will be a valuable in vitro system in which to study the influence of microgravity on epithelial permeability and drug transport.     

一种敏感电路式露点测量方法

针对大气湿度测量问题,提出一种基于敏感电路的露点测量方法.把考比兹电路中的石英晶体作为湿敏元件,用半导体制冷器对其进行制冷直到有结露产生时使得石英晶体处于液相环境中,整个考比兹电路将停止振动,利用考比兹电路这一敏感特性对露点进行识别,可以得到相应的露点温度.通过理论数据与实验数据对比分析,露点温度的最大误差为1.59℃,此方法可以从定性的角度作为一种湿度快速识别方法,并具有测量方法简单、灵敏度高、可靠性好和成本低等优点.