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Thermal design and analysis for the cryogenic MIDAS experiment

机译:低温MIDAS实验的热设计与分析

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The Materials in Devices as Superconductors (MIDAS) spaceflight experiment is a NASA payload which launched in September 1996 on the Shuttle, and was transferred to the Mir Space Station for several months of operation. MIDAS was developed and built at NASA Langley Research Center (LaRC). The primary objective of the experiment was to determine the effects of microgravity and spaceflight on the electrical properties of high-temperature superconductive (HTS) materials. The thermal challenge on MIDAS was to maintain the superconductive specimens at or below 80 K for the entire operation of the experiment, including all ground testing and 90 days of spaceflight operation. Cooling was provided by a small tactical cryocooler. The superconductive specimens and the coldfinger of the cryocooler were mounted in a vacuum chamber, with vacuum levels maintained by an ion pump. The entire experiment was mounted for operation in a stowage locker inside Mir, with the only heat dissipation capability provided by a cooling fan exhausting to the habitable compartment. The thermal environment on Mir can potentially vary over the range 5 to 40°C; this was the range used in testing, and this wide range adds to the difficulty in managing the power dissipated from the experiment's active components. Many issues in the thermal design are discussed, including; thermal isolation methods for the cryogenic samples; design for cooling to cryogenic temperatures; cryogenic epoxy bonds; management of ambient temperature components' self-heating; and fan cooling of the enclosed locker. Results of the design are also considered, including the thermal gradients across the HTS samples and cryogenic thermal strap, electronics and thermal sensor cryogenic performance, and differences between ground and flight performance. Modeling was performed in both SINDA-85 and MSC/PATRAN (with direct geometry import from the CAD design tool Pro/Engineer). Advantages of both types of models are discussed. Correlation of several models to ground testing and flight data (where available) is presented. Both SINDA and PATRAN models predicted the actual thermal performance of the experiment well, even without post-flight correlation adjustments of the models.
机译:器件中的材料作为超导体(Midas)的空间实验是1996年9月在班车上发布的NASA有效载荷,并转移到MIR空间站的几个月运行。 Midas于Nasa Langley研究中心(LARC)开发和建造。实验的主要目的是确定微匍匐和空云对高温超导(HTS)材料的电气性质的影响。 Midas上的热挑战是在80 k处维持超导样本,在实验的整个操作中,包括所有地面测试和90天的航天操作。冷却由小型战术冷冻机提供。通过离子泵保持真空水平的真空腔中的超导样品和冷冻机的冷鳍片。整个实验安装在MIR内的装载储物柜中进行操作,唯一的散热能力由冷却风扇排出到可居住的隔间。 MIR上的热环境可能会在5至40°C的范围内变化;这是测试中使用的范围,这一广泛范围增加了管理从实验活动组件消耗的功率的难度。讨论了热设计中的许多问题,包括;低温样品的热隔离方法;冷却到低温温度的设计;低温环氧键;环境温度分量的自加热;和风扇冷却封闭的储物柜。还考虑了设计的结果,包括HTS样品的热梯度和低温热带,电子和热传感器低温性能,以及地面和飞行性能之间的差异。建模在Sinda-85和MSC / Patran(CAD设计工具Pro / ENGINEER中直接几何导入)。讨论了两种模型的优点。提出了几种模型与地面测试和飞行数据(可用)的相关性。 Sinda和Patan模型都预测了实验的实际热性能,即使没有模型的飞行后相关性调整。

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