酸酐固化剂对硅橡胶低密度烧蚀材料施工期的影响

通过对延长硅橡胶密度烧蚀材料体系施工期的研究，发现酸酐固化剂可以将环氧改性硅橡胶低密度烧蚀材料的施工期延长到24h以上，从而可能实现真空热压罐大面积灌注密度烧蚀材料的成型工艺。通过对固化材料进行红外分析，发现加入酸酐固化剂后并未改变硅橡胶和环氧树脂各自的反应，没有新的反应特征峰出现，说明环氧和硅橡胶之间无反应，只是物理共混，从材料拉伸断面的扫描电镜观察可以证实硅橡胶和环氧树脂以海－岛结构存在。     

吸收剂填充体系的反应特性研究

对一种常用吸收剂填充的树脂混合体系的反应特性进行了研究，结果表明，吸收剂含量变化影响树脂混合体系的活化能、反应热、反应程度、凝胶时间。通过对吸收剂表面物质研究发现，吸收剂表面存在着与树脂体系发生反应的活性物质，引起吸收剂填充混合体系的反应特性发生变化。     

现代激励理论在规范地方政府行为中的作用研究

分析现代激励理论在研究地方政府行为中的作用，并运用现代激励理论提出了规范地方政府经济行为的若干建议。     

并行工程及其在航空电子产品研制中的应用

 概述了并行工程的运行特性,介绍了并行工程在空管应答机研制中的应用并分析了在缩短开发周期、提高产品质量、降低研制成本和改进售后服务方面的成效,总结了应用推广并行工程的经验与体会。     

全面国产化复合材料在XX旋翼国产化中的应用研究

本文概要地介绍了国产复合材料在XX旋翼国产化的应用研究总体思路,分析了国产复合材料的研究现状。通过国产化复合材料在旋翼桨叶上的设计应用分析,确定了国产材料性能的最低要求,并进行了典型样件—模型桨叶的验证考核。     

构建我国"绿色"税收体系的设想

通过阐述“绿色”税收体系的理论基础是外部性理论，分析了我国工业化进程中的环境现状，环境污染造成的危害，同时借鉴西方国家开征“绿色”税制的成功经验，提出了费改税、完善税种、开征新税、完善相关政策等构建我国“绿色”税收体系的初步设想。     

开放阅读是提高高校学报影响力的重要途径

目的推动高校学报开展开放阅读,有利于提高高校学报的影响力和社会效益。方法在简介开放阅读的概念,分析高校学报开展开放阅读的必要性和可行性的基础上,提出加入"科技图书文献资源共享平台"和"开放阅读期刊联盟"两种开放阅读的方式。结果实行开放阅读是由高校学报的学术性质所决定的,高校学报是以社会事业费和作者资助等社会资源维持出版的,其价值是其学术性而非商业性,因此没有理由为了赢利而拒绝更广泛地传播学术信息。结论开放阅读有利于提高高校学报的影响力,高校学报更应当回归学术,为学术研究服务。     

新一代数据采集器模拟量采集插件设计技术

数据采集器是飞行试验关键的测试设备,它的性能与现代飞机飞行试验有很大的关系.为满足现代飞机设计定型的需求,新一代数据采集器设计大量采用了FPGA和DSP器件,大大提高了采集器测量参数的采样率、通道数、测量参数类型和使用的灵活性.本文介绍的新一代采集器模拟量采集卡设计技术,用数字信号处理技术来实现信号的放大、滤波及偏置修正,并提供了对采集卡各个部分进行设计的理论依据.     

水听器自由场校准中不确定度的分析与评定

结合水声计量实际,较为详尽地分析了水听器的绝对和比较校准中不确定度的来源,并结合一次计量检定数据,对水听器校准中的不确定度的A类和B类评定,以及对合成不确定度、扩展不确定度的评定作了系统分析和论述。     

Emergence of a Habitable Planet

We address the first several hundred million years of Earth’s history. The Moon-forming impact left Earth enveloped in a hot silicate atmosphere that cooled and condensed over ∼1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ∼2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to the magma ocean. After the mantle solidified geothermal heat became climatologically insignificant, which allowed the steam atmosphere to condense, and left behind a ∼100 bar, ∼500 K CO₂ atmosphere. Thereafter cooling was governed by how quickly CO₂ was removed from the atmosphere. If subduction were efficient this could have taken as little as 10 million years. In this case the faint young Sun suggests that a lifeless Earth should have been cold and its oceans white with ice. But if carbonate subduction were inefficient the CO₂ would have mostly stayed in the atmosphere, which would have kept the surface near ∼500 K for many tens of millions of years. Hydrous minerals are harder to subduct than carbonates and there is a good chance that the Hadean mantle was dry. Hadean heat flow was locally high enough to ensure that any ice cover would have been thin (<5 m) in places. Moreover hundreds or thousands of asteroid impacts would have been big enough to melt the ice triggering brief impact summers. We suggest that plate tectonics as it works now was inadequate to handle typical Hadean heat flows of 0.2–0.5 W/m². In its place we hypothesize a convecting mantle capped by a ∼100 km deep basaltic mush that was relatively permeable to heat flow. Recycling and distillation of hydrous basalts produced granitic rocks very early, which is consistent with preserved >4 Ga detrital zircons. If carbonates in oceanic crust subducted as quickly as they formed, Earth could have been habitable as early as 10–20 Myrs after the Moon-forming impact.