微量气味成分的自由基簇射技术脱除

研究了密闭体系中微量气味污染物的脱除作用与机理。采用电晕放电自由基簇射技术，实现了人工环境下氧化性自由基的产生；以电子自旋共振技术（ESR）对气态羟基自由基实施了捕集和检测，验证了在羟基自由基的存在下NH3被氧化为N2。通过U—I获得反应能耗和污染物去除效率为：NH3脱除效率为90．6％时，能耗1．0W。研究表明：自由基簇射技术产生的氧化性自由基可有效去除密闭生存环境中产生的NH3等微量有害气味成分，将在空间站等密闭生存系统内空气净化中有很好的应用前景。     

“小信号谐振放大器”的教学策略

小信号谐振放大器是高频电子线路课程的基本单元电路之一,主要应用在通信系统的接收机电路中,高频放大和中频放大是信号传输电路中的核心部分。掌握小信号谐振放大器的分析方法,对电子信息类、通信工程类专业学生的学习及工作是非常关键的。     

α-l型区间可靠性分析方法及其工程应用

在区间非概率可靠性模型的基础上,以区间长度l和区间下限α为结构系统变量的输入参数,重新定义了一种新的可靠性指标,分析得到了这种可靠性分析方法的判定依据;在此基础上,在线性和非线性条件下讨论了结构可靠度的计算方法.以某型飞机防冰引气管结构为例,进一步探讨了所提方法在共振可靠性分析当中的工程应用.     

不同环境因素对引压管腔动态特性影响

为了探索引压管腔在动态压力校准和使用中不同环境因素对动态特性的影响,推导了管腔传压模型和谐振频率关系式,确立了影响管腔动态特性的参数,包括静态压力、温度、气体介质等。采用引压管腔专用实验装置进行了不同环境参数状态的实验验证,结果表明:静态压力仅会影响管腔在谐振频率附近的输出,随着静态压力的增大而非线性增大,对动态特性并无明显改变;温度会改变管腔的谐振频率和动态特性,随着温度的升高,谐振频率增大但输出幅值随之减小;气体介质的不同会彻底改变管腔动态特性,主要取决于介质的声速。该研究为引压管腔在使用环境下数据的评价和数据修正上提供了一定参考依据。     

酸性磺酞类染料共振Rayleigh散射光谱法测定奈替米星

用共振Rayleigh散射（RRS）光谱研究了酸性磺酞类染料溴甲酚绿和溴酚蓝分别与奈替米星的相互作用.溴甲酚绿和溴酚蓝在酸性介质中分别与奈替米星相互作用,导致RRS光谱显著增强,最大的RRS峰分别位于606nm和572nm处,散射强度与奈替米星的质量浓度在一定的范围内成正比.此方法具有很高的灵敏度,对于奈替米星的检测限（3σ）分别为30ng/mL和10ng/mL,据此发展了一种测定奈替米星的新方法.     

Improved predictions of equatorial TEC for real time applications

It is important to use models developed specifically for the equatorial ionospheric estimation for real-time applications, particularly in Satellite Navigation. This work demonstrates a methodology for improved predictions of VTEC in real time using the model developed for the equatorial ionosphere by the authors. This work has been done using TEC data of the low solar activity period of 2005 obtained using dual frequency GPS receivers installed under the GAGAN project of ISRO. For the purpose, the model is first used in conjunction with Kriging technique. Improvement in accuracy is observed when compared with the estimations from the model alone using the measurements as true reference. Further improvement is obtained by Bayesian combination of these estimates with independent Neural Network based predictions. Statistical performance of improvement is provided. An improvement of ∼1 m in confidence level of estimation of VTEC is obtained.     

Spectroscopic Constraints on Models of Ion-cyclotron Resonance Heating in the Polar Solar Corona

Using empirical velocity distributions derived from UVCS and SUMER ultraviolet spectroscopy, we construct theoretical models of anisotropic ion temperatures in the polar solar corona. The primary energy deposition mechanism we investigate is the dissipation of high frequency (10-10000 Hz) ion-cyclotron resonant Alfvén waves which can heat and accelerate ions differently depending on their charge and mass. We find that it is possible to explain the observed high perpendicular temperatures and strong anisotropies with relatively small amplitudes for the resonant waves. There is suggestive evidence for steepening of the Alfvén wave spectrum between the coronal base and the largest heights observed spectroscopically. Because the ion-cyclotron wave dissipation is rapid, even for minor ions like O⁵⁺, the observed extended heating seems to demand a constantly replenished population of waves over several solar radii. This indicates that the waves are generated gradually throughout the wind rather than propagated up from the base of the corona. This revised version was published online in June 2006 with corrections to the Cover Date.     

一种新型正弦压力发生器

介绍了一种利用压电叠堆激励管道内液体介质发生谐振产生正弦压力的发生装置.与其它正弦压力发生器相比,本装置压力源的激励方式新颖,工作频率较高,所产生的正弦压力波的幅值较大,失真度较小.     

基于起落架参数设计的某直升机地面共振及参数影响分析

建立了某直升机地面共振分析力学模型,计算了起落架在桨毂中心处的等效刚度和阻尼,针对某直升机进行了地面共振分析,同时分析了摆振铰外伸量、质量静距、桨毂中心有效刚度等对地面共振的影响,为避免地面共振及参数改进提供依据。     

有磁场时电子在航天器光电子鞘层中的漂移运动

采用二级漂移近似理论，研究了在航天器光电子鞘层中与电流收集有关的电子在磁场中的运动轨道和收集电子有关的磁瓶结构，结果表明当磁场越强，航天器表面电势越弱，磁瓶在无穷远处横截面积就越小。在光电子鞘层中，势垒对电流收集影响较大，磁瓶的横截面积在略远于垫垒处有极大值，磁瓶在无穷远处的横截面积并非随着势垒距航天器距离的远近而单调变化。