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The HYTHIRM Project: Flight Thermography of the Space Shuttle During the Hypersonic Re-entry

机译:HYTHIRM项目:高超音速再入期间航天飞机的飞行热成像

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摘要

This report describes a NASA Langley led endeavor sponsored by the NASA Engineering Safety Center, the Space Shuttle Program Office and the NASA Aeronautics Research Mission Directorate to demonstrate a quantitative thermal imaging capability. A background and an overview of several multidisciplinary efforts that culminated in the acquisition of high resolution calibrated infrared imagery of the Space Shuttle during hypervelocity atmospheric entry is presented. The successful collection of thermal data has demonstrated the feasibility of obtaining remote high-resolution infrared imagery during hypersonic flight for the accurate measurement of surface temperature. To maximize science and engineering return, the acquisition of quantitative thermal imagery and capability demonstration was targeted towards three recent Shuttle flights - two of which involved flight experiments flown on Discovery. In coordination with these two Shuttle flight experiments, a US Navy NP-3D aircraft was flown between 26-41 nautical miles below Discovery and remotely monitored surface temperature of the Orbiter at Mach 8.4 (STS-119) and Mach 14.7 (STS-128) using a long-range infrared optical package referred to as Cast Glance. This same Navy aircraft successfully monitored the Orbiter Atlantis traveling at approximately Mach 14.3 during its return from the successful Hubble repair mission (STS-125). The purpose of this paper is to describe the systematic approach used by the Hypersonic Thermodynamic Infrared Measurements team to develop and implement a set of mission planning tools designed to establish confidence in the ability of an imaging platform to reliably acquire, track and return global quantitative surface temperatures of the Shuttle during entry. The mission planning tools included a pre-flight capability to predict the infrared signature of the Shuttle. Such tools permitted optimization of the hardware configuration to increase signal-to-noise and to maximize the available dynamic range while mitigating the potential for saturation. Post flight, analysis tools were used to assess atmospheric effects and to convert the 2-D intensity images to 3-D temperature maps of the windward surface. Comparison of the spatially resolved global thermal measurements to surface thermocouples and CFD prediction is made. Successful demonstration of a quantitative, spatially resolved, global temperature measurement on the Shuttle suggests future applications towards hypersonic flight test programs within NASA, DoD and DARPA along with flight test opportunities supporting NASA's project Constellation.
机译:本报告介绍了由NASA工程安全中心,航天飞机计划办公室和NASA航空研究任务局赞助的NASA Langley领导的项目,以证明定量热成像功能。提出了背景和概述了多学科的努力,这些努力最终导致在超高速大气进入过程中获取航天飞机的高分辨率校准红外图像。热数据的成功收集证明了在高超声速飞行过程中获得远程高分辨率红外图像以精确测量表面温度的可行性。为了最大程度地提高科学和工程回报,获取定量热成像图像和进行能力演示的目标是最近进行的三趟航天飞机飞行,其中两趟涉及在发现号上进行的飞行实验。为了配合这两个航天飞机的飞行实验,一架美国海军NP-3D飞机在发现号下方26-41海里之间飞行,并以8.4马赫(STS-119)和14.7马赫(STS-128)远程监测了轨道器的表面温度使用称为Cast Glance的远程红外光学封装。这架海军飞机在成功完成哈勃维修任务(STS-125)返回期间,成功监视了大约14.3马赫飞行的轨道飞行器亚特兰蒂斯号。本文的目的是描述高超声速热力学红外测量团队用于开发和实施一套任务计划工具的系统方法,这些工具旨在建立对成像平台可靠地获取,跟踪和返回全局定量表面的能力的信心。进入期间航天飞机的温度。任务计划工具包括飞行前功能,可以预测航天飞机的红外信号。此类工具允许优化硬件配置,以增加信噪比并最大化可用动态范围,同时降低饱和的可能性。飞行后,使用分析工具评估大气影响并将2D强度图像转换为迎风面的3D温度图。比较了在空间上解析的整体热测量与表面热电偶以及CFD预测。在航天飞机上成功地进行了定量,空间分辨的全球温度测量的演示,表明了未来在NASA,DoD和DARPA中进行高超音速飞行测试程序的应用,以及支持NASA项目星座的飞行测试机会。

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