基于LabVIEW构建虚拟仪器系统

虚拟仪器是电子仪器技术。现代测量技术与计算机技术高速发展的产物，它将逐步取代传统电子仪器。本文介绍了虚拟仪器的概念，主要的功能和特点，虚拟仪器的系统构成，包括硬件构成及软件构成。还结合两个具体实例介绍了虚拟仪器技术的应用。     

典型零件压铸模智能CAD系统研究

建立了典型零件压铸模智能CAD系统，分析了系统各模块的组成及功能，并阐明了系统实现的关键技术。     

面对入世的机遇与挑战,我们如何应对

本文简要论述了中国加入世界贸易组织之后，我国各行各业面临的机遇与挑战，以及为了应付国外跨国公司的竞争，保护民族工商业，政府和企业应该采取的对策，强调企业和政府必须通力合作才能更好地应对加入世贸组织后所面临的挑战。     

用热像仪测试发动机燃气流场温度

通过试验研究，利用红外热像仪测试固体火箭发动机燃气流场的辐射温度，并通过高温风洞的标定数据，对测试结果进行了分析处理。提出了解决发动机燃气流场红外辐射测温时辐射系数设置的方法。     

目前我省在节能建筑发展中存在的问题与对策探讨

针对我省节能建筑发展的现状以及所存在的问题，本文详细地分析了问题产生的原因，并提出相应的解决这些问题的对策。     

The Chemical Evolution of the Milky Way Disk

A brief review is presented of our current understanding of the evolution of the Milky Way disk and of its relevance to "cosmic chemical evolution" studies. The implications of this understanding for the evolution of deuterium are emphasized.     

加装红外抑制器的直升机红外辐射的计算及测量

计算了光谱在3～5 μm及8～12 μm范围内,加装与机身结构一体化红外抑制器的某型直升机排气系统的红外辐射特性.计算中考虑了排气系统部分蒙皮的红外辐射、双喷管发动机喷气流的红外辐射、背景辐射及大气的吸收衰减对直升机排气系统红外辐射信号的影响.实验发现,一架加装与机身结构一体化红外抑制器的直升机排气系统红外辐射特性的计算结果,与实测结果基本一致.     

飞机备件需求量的确定方法

飞机备件需求量计算是航空备件计划管理的一项重要内容。对飞机备件的分类及其特性进行了分析，并建立了循环件、非循环件和消耗件的需求量计算实用关系式。对需求量计划在实际中的应用问题，提出些看法和建议。     

复制理论与二进码

基于复制理论的思想，分析了有关的二进码，指出了二进码本身具有的某种复制特性，并且根据组合思想提出了新的二进码－Ｋ码，根据平移复制和对称复制的等效性，证明了Ｋ码和自然二进制码的关系，揭示了Ｋ码的物理意义，提出了有趣的有关函数。     

Modeling the (upper) solar atmosphere including the magnetic field

The atmosphere of the Sun is highly structured and dynamic in nature. From the photosphere and chromosphere into the transition region and the corona plasma-β changes from above to below one, i.e., while in the lower atmosphere the energy density of the plasma dominates, in the upper atmosphere the magnetic field plays the governing role – one might speak of a “magnetic transition”. Therefore the dynamics of the overshooting convection in the photosphere, the granulation, is shuffling the magnetic field around in the photosphere. This leads not only to a (re-)structuring of the magnetic field in the upper atmosphere, but induces also the dynamic reaction of the coronal plasma, e.g., due to reconnection events. Therefore the (complex) structure and the interaction of various magnetic patches is crucial to understand the structure, dynamics and heating of coronal plasma as well as its acceleration into the solar wind.

The present article will emphasize the need for three-dimensional modeling accounting for the complexity of the solar atmosphere to understand these processes. Some advances on 3D modeling of the upper solar atmosphere in magnetically closed as well as open regions will be presented together with diagnostic tools to compare these models to observations. This highlights the recent success of these models which in many respects closely match the observations.