飞行器振动智能分析与诊断

本文通过综合多个领域知识，引进功能特征描述概念，运用证据理论，提出了对飞行器等复杂系统进行分析诊断的一个新方法并初步完成了专家系统原型，通过具体实例，再现了故障现象     

复合材料壳体与喷管的卡环连接结构研究

较详细地对复合材料壳体与喷管卡环连接结构进行了有限元应力,应变分析,对卡环,接头及倒锥等多体接触问题进行研究;对“Ｉ”型及“Ｌ”型卡环结构分别进行了计算和比较,并给出计算结果及结果分析。     

空间相机中与大口径透镜有关的结构设计分析

某空间相机镜头在光学设计时，因透过率、吸收率等原因，为了满足光学系统要求，经过各方面平衡后，其中有一片透镜比正常径厚比设计的偏薄些。在镜头总体结构设计时，单独对该镜片及与之相配的结构件进行了有限元分析和实验检测，发现不同的结构形式对镜片面形影响不同。为了解决这一问题，在实验中进行了探讨，以保证整个相机系统满足空间相机的实用要求。     

有关压力传感器可靠性设计的若干问题

论述压力传感器的研制和应用中的经验教训。着重讨论从任务书要求，工程化设计，到生产过程有关压力信号特征、压力接口以及功能与结构相关性，功能与材料相关性等问题。     

环境专业教学体系结构改革探索——以就业市场需求为导向

通过对西安航专2006与2007年环境监测与治理技术专业毕业生就业情况的对比分析，认为目前环境类专业的就业形势发生良性转变，需求范围增加，同时就业单位对毕业生的专业技术能力、技术管理能力等也提出了更高的要求。据此，我们从专业发展方向、课程体系结构以及实验实训三个方面进行建设与调整来满足就业单位的需求。     

Observations of loops and prominences

We review recent observations by the Yohkoh-SXT in collaboration with other spacecraft and ground-based observatories of coronal loops and prominences. These new results point to problems that SoHO will be able to address. With a unique combination of rapid-cadence digital imaging (32 s full-disk and 2 s partial-frame images), high spatial resolution (2.5 arcsec pixels), high sensitivity (EM 10⁴² cm^–3), a low-scatter mirror, and large dynamic range, SXT can observe a vast range of targets on the Sun. Over the first 21 months of Yohkoh operations, SXT has taken over one million images of the corona and so is building up an invaluable long-term database on the large-scale corona and loop geometry. The most striking thing about the SXT images is the range of loop sizes and shapes. The active regions are a bright tangle of magnetic field lines, surrounded by a network of large-scale quiet-Sun loops stretching over distances in excess of 10⁵ km. The cross-section of most loops seems to be constant. Loops displaying significant increase in the ratio of the footpoint to loop-top diameter () are the exception, not the rule, implying the presence of widespread currents in the corona.All magnetic structures show changes. Time scales range from seconds to months. The question of how these structures are formed, become filled with hot plasma, and are maintained is still open. While we see the propagation of brightenings along the length of active-region loops and in X-ray jets with velocities of several hundred km/s, much higher velocities are seen in the quiet Sun. In XBP flares, for example, velocities of over 1000 km/s are common. Active-region loops seem to be in constant motion, moving slowly outward, carrying plasma with them. During flares, loops often produce localized brightenings at the base and later at the apex of the loop. Quiescent filaments and prominences have been observed regularly. Their coronal manifestation seems to be an extended arcade of loops overlying the filament. Reliable alignment of the ground-based data with the X-ray images make it possible to make a detailed intercomparison of the hot and cold plasma structures over extended periods. Hence we are able to follow the long-term evolution of these structures and see how they become destabilized and erupt.     

一种新颖的瞬时浮点放大器

介绍了瞬时浮点放大器的原理及构成，并给出一种结构新的具有２５６阶的瞬时浮点放大器，可有效地提高数据采集系统的测量范围。     

融合自适应步长与地图匹配的智能手机PDR室内定位算法

围绕全角半球谐振陀螺的典型使用环境特征,对谐振子结构方案进行了深入研究。仿真分析了“等壁厚”“上薄下厚”“上厚下薄”3种结构方案的振动特性差异,发现在谐振子平均尺寸相同的情况下,“上厚下薄”方案的工作频率最高,相邻模态频率间隔最大,且受冲击影响最小。进一步,定量仿真分析了内球面半径、内圆角半径及内支撑柱直径等结构参数对“上厚下薄”谐振子振动特性以及抗冲击性能的具体影响,为陀螺的设计加工提供了有效参考。     

《建筑结构》课程教学改革实践

为了在《建筑结构》课程教学中，体现高职教育的高等性和职业性，突出高职教育的职业特色，笔者在准确定位课程的教学目标、优化教学内容结构方面进行了探讨，并提出增加实践教学环节，创新教育手段，改革成绩评定方法等建议。