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In search of water vapor on Jupiter: Laboratory measurements of the microwave properties of water vapor and simulations of Jupiter's microwave emission in support of the Juno Mission.

机译:在木星上寻找水蒸气:为支持朱诺任务而进行的水蒸气微波特性的实验室测量和模拟木星的微波发射。

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摘要

This research has involved the conduct of a series of laboratory measurements of the centimeter-wavelength opacity of water vapor along with the development of a hybrid radiative transfer ray-tracing simulator for the atmosphere of Jupiter which employs a model for water vapor opacity derived from the measurements. For this study an existing Georgia Tech high-sensitivity microwave measurement system (Hanley and Steffes, 2007) has been adapted for pressures ranging from 12--100 bars, and a corresponding temperature range of 293--525°K. Water vapor is measured in a mixture of hydrogen and helium. Using these measurements which covered a wavelength range of 6--20 cm, a new model is developed for water vapor absorption under Jovian conditions. In conjunction with our laboratory measurements, and the development of a new model for water vapor absorption, we conduct sensitivity studies of water vapor microwave emission in the Jovian atmosphere using a hybrid radiative transfer ray-tracing simulator. The approach has been used previously for Saturn (Hoffman, 2001), and Venus (Jenkins et al., 2001).;This model has been adapted to include the antenna patterns typical of the NASA Juno Mission microwave radiometer (NASA/Juno-MWR) along with Jupiter's geometric parameters (oblateness), and atmospheric conditions. Using this adapted model we perform rigorous sensitivity tests for water vapor in the Jovian atmosphere. This work will directly improve our understanding of microwave absorption by atmospheric water vapor at Jupiter, and improve retrievals from the Juno microwave radiometer. Indirectly, this work will help to refine models for the formation of Jupiter and the entire solar system through an improved understanding of the planet-wide abundance of water vapor which will result from the successful opreation of the Juno Microwave Radiometer (Juno-MWR).
机译:这项研究涉及对水蒸气的厘米-波长不透明度进行一系列的实验室测量,以及针对木星大气的混合辐射转移射线追踪模拟器的开发,该模拟器采用了由测量。为了进行这项研究,现有的佐治亚理工学院高灵敏度微波测量系统(Hanley and Steffes,2007)已经适应了12--100 bar的压力以及293--525°K的相应温度范围。在氢和氦的混合物中测量水蒸气。使用覆盖6--20 cm波长范围的这些测量结果,开发了一种新的模型,用于在木星条件下吸收水蒸气。结合我们的实验室测量和水蒸气吸收新模型的开发,我们使用混合辐射转移射线追踪模拟器对木星大气中水蒸气微波发射的敏感性进行了研究。该方法先前已用于土星(Hoffman,2001)和金星(Jenkins等,2001).;已对该模型进行了修改,以包括NASA Juno Mission微波辐射计(NASA / Juno-MWR)的典型天线方向图。 )以及木星的几何参数(扁率)和大气条件。使用这个改编的模型,我们对木星大气中的水蒸气进行了严格的灵敏度测试。这项工作将直接增进我们对木星大气水蒸气吸收微波的理解,并改善从朱诺微波辐射计获​​得的数据。间接地,这项工作将通过更好地了解朱诺微波辐射计(Juno-MWR)成功产生的结果,来提高行星范围内水汽的丰度,从而有助于完善木星和整个太阳系形成的模型。

著录项

  • 作者

    Karpowicz, Bryan Mills.;

  • 作者单位

    Georgia Institute of Technology.;

  • 授予单位 Georgia Institute of Technology.;
  • 学科 Planetology.;Remote Sensing.;Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2010
  • 页码 332 p.
  • 总页数 332
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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