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2018 Joint Thermophysics and Heat Transfer Conference最新文献

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Thermophysical Properties of Temperature Sensitive Paint 温敏涂料的热物理性能
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3268
W. Stryczniewicz, A. Panas, R. Szczepaniak
The complex thermophysical property of temperature-sensitive paint (TSP) research is discussed. TSP is used for visualization of the surface temperature distribution in wind tunnel aerodynamic tests. The purpose of this research was to provide reliable, experimental, thermophysical data of the paint applied as a coating. As TSP is applied as thin surface layers, investigation of its final properties is challenging and demands the application of non-standard procedures. At present, most measurements were performed on composite specimens of TSP deposed onto a thin metallic film substrate or on TSP combined with a cellulose sheet support. The studies involved gravimetric„ thermogravimetric, and microcalorimetric analyses, transversal thermal diffusivity estimation from laser flash data and in-plane effective thermal diffusivity measurements done by the temperature oscillation technique. These results were complemented with scanning electron microcopy analysis, surface characterization and the results of dilatometric measurements performed on the TSP bulk specimens obtained from liquid substrate by casting. Complex analysis of the obtained results indicated an isotropic characteristic of the thermal diffusivity of the TSP layer and provided reliable data on all measured thermophysical parameters—they were revealed to be typical for insulators. Further to presenting these data, the paper, in brief, presents the applied investigation procedures.
对温敏涂料(TSP)的复杂热物性进行了研究。TSP用于风洞气动试验中表面温度分布的可视化。本研究的目的是为涂料提供可靠的、实验性的热物理数据。由于TSP作为薄表面层应用,对其最终性能的研究具有挑战性,需要应用非标准程序。目前,大多数测量都是在TSP沉积在薄金属薄膜衬底上的复合试样上进行的,或者是在TSP与纤维素片支架结合的情况下进行的。这些研究包括重量、热重和微热分析,从激光闪光数据估计横向热扩散系数,以及用温度振荡技术测量平面内有效热扩散系数。这些结果与扫描电子显微分析、表面表征和对通过铸造从液体基材中获得的TSP块状试样进行的膨胀测量结果相辅相成。对所得结果的复杂分析表明,TSP层的热扩散率具有各向同性特征,并为所有测量的热物性参数提供了可靠的数据-它们被揭示为典型的绝缘体。在介绍这些数据的基础上,简要介绍了应用的调查程序。
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引用次数: 3
On the Modelling of Shell and Tube Heat Exchanger Characteristics 管壳式换热器特性建模研究
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3906
E. Khalil, A. Adel, Gamal a. ElHarriri, W. Abdelmaksoud, E. Saad
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引用次数: 1
Extension of Kestrel to General Thermochemical Models, Part II 红隼扩展到一般热化学模型,第二部分
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3267
R. B. Bond, D. Stefanski
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引用次数: 7
Helical Droplet Heat Exchanger: A Novel Thermal Management Device 螺旋液滴热交换器:一种新型热管理装置
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-4183
W. Flaherty, R. Fontaine
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引用次数: 0
Numerical Calculation of the Effective Thermal Conductivity of Three-Dimensional Three-Scale Microstructures 三维三尺度微结构有效导热系数的数值计算
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3587
Lucas Prado Mattos, M. E. Cruz, J. Bravo-Castillero
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引用次数: 0
Experimental study of Saturn entry radiation with higher amount of diluent in an expansion tube 膨胀管中高稀释剂量土星进入辐射的实验研究
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-4070
Yu Liu, C. James, R. Morgan, T. Mcintyre
The aerodynamics of entry into gas giants are dominated by thermochemical processes occurring in the shock layers. These processes are specific to the gas giants, with their unique atmospheric composition of hydrogen and helium, and are not well understood. This paper used the condition with the maximum enthalpy which can be achieved in the expansion tube, X2, as well as increased helium content in the test gas, to generate a radiation field representative of blunt body Saturn entry. These are the first spectrally resolved radiation measurement ever performed in an impulse facility to study simulated Saturn entry. Both high speed imaging and spectrometry were employed to measure the atomic hydrogen radiation emitted from Balmer series of hydrogen atoms. The bright region in the radiation field merely exists near the model surface, indicative of the slow ionization process,which causes the electron number densities to build up only near the surface. From the central streamline spectral data, H-α was the strongest transition, while other transitions (n < 3) were negligible after the shock, and became brighter near the body. Both the horizontal radiance profile and high speed image were employed to locate the focused slices in vertical shots. It was also found by the Specair calculation that self-absorption is more likely to occur in H-α radiance than in H-β radiance with the line of sight in this study.
进入气态巨行星的空气动力学是由发生在激波层中的热化学过程控制的。这些过程是气态巨行星特有的,它们独特的大气成分是氢和氦,目前还没有得到很好的理解。本文利用膨胀管X2所能达到的最大焓,以及试验气体中氦气含量增加的条件,生成了一个钝体土星进入具有代表性的辐射场。这是有史以来第一次在脉冲设备上进行光谱分辨辐射测量,以研究模拟土星进入。采用高速成像和光谱法对Balmer系列氢原子发出的原子氢辐射进行了测量。辐射场中的明亮区域仅存在于模型表面附近,表明电离过程缓慢,这导致电子数密度仅在表面附近建立。从中心流线光谱数据来看,H-α是最强的跃迁,而其他跃迁(n < 3)在激波后可以忽略不计,在天体附近变得更亮。利用水平辐射廓线和高速图像对垂直镜头中的聚焦切片进行定位。Specair计算还发现,在本研究的视线范围内,H-α辐射比H-β辐射更容易发生自吸收。
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引用次数: 5
Spatially Resolved Analysis of Material Response to Destructive Environments Utilizing Three-Dimensional Scans 利用三维扫描对破坏性环境的材料响应进行空间分辨分析
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3761
J. Engerer, Alexander L. Brown
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引用次数: 1
Simulation of Radiative Heat Transfer in a Particle Laden Flow 粒子流中辐射传热的模拟
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-4288
K. Hansson, I. Boyd
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引用次数: 5
Molecular and Continuum Simulations of Binary Gas Mixture Flow Through Curved Micronozzles 二元气体混合物在弯曲微喷嘴中流动的分子和连续体模拟
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-4184
M. Darbandi, Moslem Sabouri, G. Schneider
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引用次数: 0
Computational Aerothermodynamic Environments for the Mars 2020 Entry Capsule 火星2020太空舱的计算空气热力学环境
Pub Date : 2018-06-24 DOI: 10.2514/6.2018-3116
A. Wise, D. Prabhu, C. Johnston, David Saunders, K. Edquist
The simulation tools and processes used to generate aerothermodynamic environment definitions for the Mars 2020 entry capsule are presented. The Mars 2020 capsule leverages the heritage Mars Science Laboratory design, but the entry will follow a different trajectory, landing at a different location and altitude onMars. The general strategy for creating theMars 2020mission-specific environments follows from theMars Science Laboratory experience. The primary difference is that now the effects of shock-layer radiation are modeled, with particular concern for the backshell.
介绍了火星2020返回舱空气热力学环境定义的仿真工具和过程。火星2020太空舱利用了传统的火星科学实验室设计,但进入将遵循不同的轨道,在火星上的不同位置和高度着陆。创建mars 2020任务特定环境的总体策略遵循火星科学实验室的经验。主要的区别是现在冲击波层辐射的影响是建模的,特别关注后壳。
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引用次数: 9
期刊
2018 Joint Thermophysics and Heat Transfer Conference
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