Thermal Wake Studies During the August 21st 2017 Total Solar Eclipse

Kaye Smith, E. Agrimson, Brittany Craig, Rachel DuBose, Alynie Xiong, Grace Maki, Peace Sinyigaya, Vina Onyangoro-Robshaw, Ana Taylor, Rachel Lang, J. Flaten, G. Mcintosh
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引用次数: 1

Abstract

A thermal wake occurs when a high altitude balloon (HAB) influences and changes the surrounding ambient atmospheric temperature of the air through which it passes. This effect warms the air below the balloon to greater than the ambient temperatures during daytime flights, and cooler than ambient temperatures during nighttime flights. The total solar eclipse of August 21st, 2017, provided us with an opportunity to study these balloon induced temperature transitions from daytime, to eclipsed induced night conditions over the scale of a single flight. To measure these transitions, St. Catherine University and the University of Minnesota, Morris, flew over 40 temperature sensors suspended beneath weather balloons ascending within the path of totality. Stratospheric temperature data collected during the eclipse show evidence of both daytime and nighttime wake temperature profiles.
2017年8月21日日全食期间的热尾流研究
当高空气球(HAB)影响并改变其所经过的周围大气温度时,就会产生热尾迹。这种效应使气球下面的空气在白天飞行时比环境温度高,而在夜间飞行时比环境温度低。2017年8月21日的日全食为我们提供了一个机会,在单次飞行的范围内研究这些由气球引起的温度从白天到日食引起的夜间条件的变化。为了测量这些变化,圣凯瑟琳大学和明尼苏达大学莫里斯分校在气象气球下放置了40多个温度传感器,这些温度传感器在日全食的路径上上升。在日食期间收集的平流层温度数据显示了白天和夜间尾流温度分布的证据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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