面向微纳卫星应用的激光数传技术

针对遥感微纳卫星对地高速数传需求,开展面向微纳卫星的激光数传技术研究,突破微纳卫星激光通信终端星地快速捕获建链和协同高精度稳定跟踪、天基终端轻小型化、复合光电组件等关键技术。完成微纳卫星的天基激光终端和地面激光终端研制,并开展星地传输试验验证,实现 1 230 km、10/50/100 Mbps 的星地数据传输,验证了相关技术,为后续我国微纳卫星对地遥感应用提供了理想的星地数传手段。     

非额定条件下变压器损耗测量研究

讨论了利用单片机技术测量变压器损耗的基本方法.推导了在非额定电压下测量变压器空载损耗的数学模型及其软件结构.最后给出实践结果.     

对搞好天津高校健康教育的初探

通过不同侧面说明在高校开展健康教育的意义，简要介绍了我市高校开展健康教育的现状，提出了促进我市高校开展健康教育的看法。     

基于B/S的沥青混合料搅拌设备远程监控系统

在分析比较客户器/服务器(C/S)和浏览器/服务器(B/S)结构模型的基础上,设计基于浏览器/服务器(B/S)结构模型的大型沥青混合料搅拌设备远程监控系统,并对系统实现中的现场总线技术、数据库技术以及A SP技术等关键技术进行了深入的研究。分析表明,B/S结构模型适用于构建大型沥青混合料搅拌设备的远程监控系统,该系统的构建对于提高我国公路施工关键设备的信息化水平具有重要意义。     

The Chemical Composition of Interstellar Matter at the Solar Location

The Local Interstellar Cloud (LIC) surrounds the Solar System and sets the boundary conditions for the heliosphere. Using both in situ and absorption line data towards ε CMa we are able to constrain both the ionization and the gas phase abundances of the LIC gas at the Solar Location. We find that the abundances are consistent with all of the carbonaceous dust grains having been destroyed, and in fact with a supersolar abundance of C. The constituents of silicate grains, Si, Mg, and Fe, appear to be sub-solar, indicating that silicate dust is present in the LIC. N, O and S are close to the solar values.     

网络融合的接入网技术

本文从电信网、广播电视网和因特网三种网络的不同特点入手，说明了三网合一的必要性和可行性，重点探讨了三网合一中关键的接入网技术。     

飞机电气设计系统在网络化中的安全

鉴于应用系统数据的重要性，本文提出了几种在飞机电气系统设计应用系统中保护数据的方法，对一些重要数据，如用户口令等采用了加密手段来保护，有效地防止了系统内和系统外对数据安全的威胁。系统的安全是分层实现的，特别是面向该系统的主要使用者－设计人员的应用层。     

The Composition of Cosmic Rays and the Mixing of the Interstellar Medium

The differences between the composition of Galactic cosmic rays and that of the interstellar medium are manifold, and they contain a wealth of information about the varying processes that created them. These differences reveal much about the initial mixing of freshly synthesized matter, the chemistry and differentiation of the interstellar medium, and the mechanisms and environment of ion injection and acceleration. Here we briefly explore these processes and show how they combine to create the peculiar, but potentially universal, composition of the cosmic rays and how measurements of the composition can provide a unique measure of the mixing ratio of the fresh supernova ejecta and the old interstellar medium in this initial phase of interstellar mixing. In particular, we show that the major abundance differences between the cosmic rays and the average interstellar medium can all result from cosmic ray ion injection by sputtering and scattering from fast refractory oxide grains in a mix of fresh supernova ejecta and old interstellar material. Since the bulk of the Galactic supernovae occur in the cores of superbubbles, the bulk of the cosmic rays are accelerated there out of such a mix. We show that the major abundance differences all imply a mixing ratio of the total masses of fresh supernova ejecta and old interstellar material in such cores is roughly 1 to 4. That means that the metallicity of ∼3 times solar, since the ejecta has a metallicity of ∼8 times that of the present interstellar medium.     

指导高职高专在校生专升本的研究与实践

正确地指导好高职高专在校生的专升本，是每位老师应尽的责任和义务。笔从近几年高职高专在校生专升本的实际出发，分析探讨了高职高专在校生专升本可能遇到的困难和问题，以及如何正确引导学生克服困难，找出解决这些问题的思路和方法。     

数据库设计工具ERwin的研究与实践

介绍了一种新的数据库设计工具ERwin的编程设计方法 ,对概念数据建模、物理数据建模的原理进行了分析 ,在对“物资管理系统”的需求做了分析之后 ,建立了概念模型 ,然后使用概念模型生成物理模型 ,并在物理层让它们与SQLServer 2 0 0 0建立了连接 ,最终在SQLServer 2 0 0 0中成功生成了数据库。