三层壁喷管的不稳定导热

文章介绍了固体火箭发动机三层壁喷管的不稳定导热的计算方法,导出壁面温度分布规律和各层壁温的计算公式,并指出工作时间与内表面壁温和影响喷管烧蚀的关系。     

树脂基碳纤维复合材料的热物理性能之一——导热系数

本文讨论了树脂基碳纤维复合材料热导与各种纤维体积含量V_f及温度的关系,研究了树脂基碳纤维复合材料的传热机理,并给出了大量的导热系数数据。     

液体火箭发动机层板式预燃室液氧发汗冷却热控制

讨论了富氧预燃室液氧发汗冷却的分析计算方法。发汗流对燃气热流的阻隔分析采用Ｂａｒｔｌｅ－Ｌｅａｄｏｎ修正方法来完成,室壁温度分布和热穿透深度应用结构层板与发汗流存在温差的传热模型获得。讨论了发汗流压降和控制流道长度对预燃室壁温的控制作用。     

低太阳吸收率αs,高发射率ε有机硅热控涂层进展

本文总结了有机硅热控涂层的设计原理及其紫外真空降解原因,评述了涂层的国内外进展.     

Al2O3—Ti系梯度功能材料的优化设计

对Ａｌ３Ｏ３－Ｔｉ系梯度功能材料在制备过程中产生的残余热应力进行了弹性有限元法分析。讨论了梯度层数目,梯度层厚度和成分梯度指数对应力大小和分布的影响,优化出了各项最佳参数。非线度功能材料与优化后的梯度功能材料的残余热应力对比结果显示;梯度功能材料缓和热应力的效果十分显著。     

深空探测对航天器热控技术的推动

工程热物理学广泛应用于航天领域,一方面解决了具体航天工程问题,另一方面逐步发展成为交叉学科——空间热物理。随着我国在深空探测领域不断拓展,以深空探测器研制中的工程热物理问题为需求背景,推动着航天器热控制技术、防热技术等取得新的发展。文章在介绍深空探测器技术体系的基础上,分析了热设计、热分析、热试验、热控硬件、防热等方面的技术进步,并就深空探测领域进一步拓展对工程热物理发展的牵引进行了展望,分析了工程热物理学与航天技术间相互促进、相互推动的关系。     

ZnO/SBA-15无机热控涂层填料及涂层性能

开展高紫外-可见-近红外反射能力热控填料的制备,研制新型低吸收比(α_S)高发射率(ε_H)无机热控涂层。以自制SBA-15和ZnO前驱体为原料通过溶剂热浸渍和高温煅烧法制备ZnO/SBA-15填料,然后与硅酸钾(K_2SiO_3)制备无机热控涂层;采用SAXD、XRD、SEM、太阳反射光谱分析填料和涂层的性能。结果显示采用硝酸锌作为前驱体、m(ZnO)∶m(SBA-15)=3∶7、950℃下烧结3 h可以得到高紫外-可见-近红外反射能力的填料;ZnO/SBA-15/K_2SiO_3无机涂层的α_S为0.09,ε_H为0.91,涂层结合力等级为1级,经过100次-196～100℃热循环实验后,涂层无脱落和开裂现象。SBA-15改性ZnO可以获得具有高紫外反射率和低α_S的热控填料,ZnO/SBA-15填料制备的无机热控涂层同样具备高紫外反射率、低α_S和高ε_H,可以满足航天器高效散热的需求,应用前景良好。     

含金属相变材料温控组件的研究

研究使用一种含有金属相变材料（Phase Change material,PCM）的温控组件（Thermal Control Component,TCC）对航天器上的有效载荷进行温度控制。通过对载荷的温控需求分析,设计并制备了以Ga-Sn合金为PCM的TCC,并通过地面模拟实验对TCC的温控性能进行测试。实验结果表明这种含有Ga-Sn合金的TCC满足载荷的温控需求。最后在仿真软件中建立了TCC的相变传热仿真模型用于预测TCC的温控性能。结果表明：仿真模型计算所得结果与实验结果基本一致,可用于预测TCC的温控性能。     

New trade tree for manned mars missions

Recent studies on human missions to Mars suggest revisiting the parameters that have the most important impact on the complexity, the initial mass in low Earth orbit, the risks and the development costs for the first journey to the red planet. In the last NASA reference mission, a trade tree is proposed.     

Thick galactic cosmic radiation shielding using atmospheric data

NASA is concerned with protecting astronauts from the effects of galactic cosmic radiation and has expended substantial effort in the development of computer models to predict the shielding obtained from various materials. However, these models were only developed for shields up to about 120 g/cm² in mass thickness and have predicted that shields of this mass thickness are insufficient to provide adequate protection for extended deep space flights. Consequently, effort is underway to extend the range of these models to thicker shields and experimental data is required to help confirm the resulting code. In this paper empirically obtained effective dose measurements from aircraft flights in the atmosphere are used to obtain the radiation shielding function of the Earth's atmosphere, a very thick, i.e. high mass, shield. Obtaining this result required solving an inverse problem and the method for solving it is presented. The results are shown to be in agreement with current code in the ranges where they overlap. These results are then checked and used to predict the radiation dosage under thick shields such as planetary regolith and the atmosphere of Venus.