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Cooling a Solar Telescope Enclosure: Plate Coil Thermal Analysis

机译:冷却太阳望远镜外壳:板线圈热分析

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The climate of Haleakala requires the observatories to actively adapt to changing conditions in order to produce the best possible images. Observatories need to be maintained at a temperature closely matching ambient or the images become blurred and unusable. The Daniel K. Inouye Solar Telescope is a unique telescope as it will be active during the day as opposed to the other night-time stellar observatories. This means that it will not only need to constantly match the ever-changing temperature during the day, but also during the night so as not to sub-cool and affect the view field of other telescopes while they are in use. To accomplish this task, plate coil heat exchanger panels will be installed on the DKIST enclosure that are designed to keep the temperature at ambient temperature +0°C/-4°C. To verify the feasibility of this and to validate the design models, a test rig has been installed at the summit of Haleakala. The project's purpose is to confirm that the plate coil panels are capable of maintaining this temperature throughout all seasons and involved collecting data sets of various variables including pressures, temperatures, coolant flows, solar radiations and wind velocities during typical operating hours. Using MATLAB, a script was written to observe the plate coil's thermal performance. The plate coil did not perform as expected, achieving a surface temperature that was generally 2°C above ambient temperature. This isn't to say that the plate coil does not work, but the small chiller used for the experiment was undersized resulting in coolant pumped through the plate coil that was not supplied at a low enough temperature. Calculated heat depositions were about 23% lower than that used as the basis of the design for the hillers to be used on the full system, a reasonable agreement given the fact that many simplifying assumptions were used in the models. These were not carried over into the testing. The test rig performance showing a 23% margin provides a high degree of confidence for the performance of the full system when it is installed. If time allows, additional testing could be done that includes additional incident angles and times of day. This would allow a more complete analysis. If additional testing were to be performed, it's recommended to use a larger chiller capable of reaching lower temperatures. The test rig design could also be optimized in order to bring the plate coil up to its maximum efficiency. In the future, the script could be rewritten in a different computer language, so that the data could be solved for quicker. Further analysis could also include different types of coolants.
机译:哈雷阿卡拉(Haleakala)的气候要求天文台积极适应不断变化的条件,以产生最佳的图像。天文台需要保持在与周围环境非常匹配的温度下,否则图像会变得模糊且无法使用。 Daniel K. Inouye太阳望远镜是一款独特的望远镜,因为它将在白天运行,而不是其他夜间恒星观测站。这意味着它不仅需要在白天不断地适应不断变化的温度,而且在夜间也要不断变化,以免在使用过程中过冷并影响其他望远镜的视场。为了完成此任务,板式线圈热交换器面板将安装在DKIST机柜上,该机柜的设计目的是将温度保持在环境温度+ 0°C / -4°C。为了验证此方法的可行性并验证设计模型,在哈雷阿卡拉(Haleakala)峰会上安装了测试台。该项目的目的是确认板式线圈板能够在所有季节中保持该温度,并涉及收集典型运行期间各种变量的数据集,包括压力,温度,冷却剂流量,太阳辐射和风速。使用MATLAB,编写了一个脚本来观察印版线圈的热性能。板状线圈的性能不如预期,达到的表面温度通常比环境温度高2°C。这并不是说板式盘管不起作用,而是用于实验的小型冷却器尺寸过小,导致冷却剂泵送通过板式盘管,而冷却剂的供应温度不足。计算的热量沉积比整个系统上使用的Hillers的设计基础低约23%,考虑到模型中使用了许多简化假设的事实,这是一个合理的协议。这些没有被带入测试。测试设备的性能显示出23%的裕量,为整个系统在安装时的性能提供了高度的可信度。如果时间允许,可以进行其他测试,其中包括其他入射角度和一天中的时间。这样可以进行更完整的分析。如果要进行其他测试,建议使用能够达到较低温度的较大冷却器。还可以优化测试台的设计,以使印版线圈达到最大效率。将来,可以用另一种计算机语言来重写脚本,以便可以更快地解决数据。进一步的分析可能还包括不同类型的冷却剂。

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