共查询到19条相似文献,搜索用时 78 毫秒
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EAST超导托卡马克的纵场和极向场磁体均采用NbTi超导材料,由3.8 K超临界氦冷却.在托卡马克实验运行时,极向场的放电脉冲和等离子体破裂产生的交流损耗带来的热负荷增加,经过超临界氦流带到低温系统控制阀箱内的液氦槽和过冷槽,造成槽内的液氦蒸发量增加.蒸发的氦回到制冷机中,从而影响制冷机的稳定运行.通过对实际超临界管道和液氦槽、过冷槽中换热过程建立换热模型,进行热工分析,分析液氦槽和过冷槽中的压力等参数的变化,指导低温系统的设计. 相似文献
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目前超导电力输送电缆的研制方案需要在4.5K~14K范围内操作的低温制冷机,该温度范围只能利用氦作为最后制冷剂而获得。这种氦制冷机应用对投资、外形尺寸、运转可靠性及运转费用在经济性方面影响很大。由于氦的分子量比较小,目前氦制冷机设计的技术水平取决于采用费用大、易于维修的大型高效往复式压缩机,还是采用效率较低的紧凑的喷油螺杆压缩机。 相似文献
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HT- 7U超导托卡马克的纵场磁体和极向场磁体均采用 3.8K超临界氦迫流冷却。其低温系统氦制冷机在 4K温区的基本设计容量为 10 5 0 W/3.5 K 2 0 0 W/4 .4K 13g/s· L He。给出了氦制冷机的基本流程 ,对其制冷循环进行了热力学分析 ,得到了影响制冷循环的关键独立参数。并以 2台串联透平膨胀机的排气温度为独立变量对氦制冷循环进行了优化 ,得到了氦制冷循环设计的最优参数值及它们对所需压缩机流量的影响 相似文献
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A variation of visualization techniques such as Shadowgraph, Schlieren and holographic interferometry, has been so far applied to visualize thermo-fluid phenomena in cryogenic fluids, superfluid helium (He II) and supercritical nitrogen, by some researchers. This paper is a review of these visualization techniques used in cryogenic fluids as well as an introduction of visualization techniques. 相似文献
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氦气净化技术是国家大科学工程北京正负电子对撞机重大改造(BEPC-Ⅱ)中低温系统的关键技术之一.在充分调研国内外大型低温系统氦气净化技术的基础上,结合自身情况,创造性提出氦气储罐内部处理及真空置换方案,一次性充入氦气,将储罐内氦气不纯度控制在40 vpm之内,同时辅之以80 K外置低温吸附器对氦气储罐内以及冷箱和超导设备端的氦气进行净化.高效而又经济的解决了BEPC-Ⅱ低温系统中的氦气纯度问题,成功地进行了制冷机的验收测试和超导设备的调试及运行. 相似文献
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Subsystems for a “proof of concept” cryogenic payload have been developed to demonstrate the ability to accommodate low temperature science investigations within the constraints of the Hitchhiker siderail (HH-S) carrier on the Space Shuttle. These subsystems include: a hybrid solid neon – superfluid helium cryostat, a multi-channel Versa Modular European (VME) architecture Germanium Resistance Thermometer (GRT) readout and heater control servo system, and a multiple thermal isolation stage “probe” for thermal control of helium samples. The analysis and tests of these subsystems have proven the feasibility of a cryogenic HH-S carrier payload. 相似文献
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《低温学》2018
ASTRO-H was an X-ray astronomy satellite that the Japan Aerospace Exploration Agency (JAXA) developed to study the evolution of the universe and physical phenomena yet to be discovered. The primary scientific instrument of ASTRO-H was the Soft X-ray Spectrometer (SXS). Its detectors were to be cooled to 50 m K using a complex cryogenic system with a multistage adiabatic demagnetization refrigerator (ADR) developed by the National Aeronautics and Space Administration (NASA), and a cryogenic system developed by Sumitomo Heavy Industries, Ltd. (SHI). SHI’s cryogenic system was required to cool the ADR’s heatsink to 1.3 K or less in orbit for three years or longer. To meet these requirements, SHI developed a hybrid cryogenic system consisting of a liquid helium tank, a 4 K Joule-Thomson cooler, and two two-stage Stirling coolers.ASTRO-H was launched from Tanegashima Space Center on February 17, 2016. The initial operation of the SXS cryogenic system in orbit was completed successfully. The cooling performance was as expected and could have exceeded the lifetime requirement of three years.This paper describes results of ground tests, results of top-off filling of superfluid liquid helium just before launch, and cooling performance in orbit. 相似文献