The Role of Remote Sensing Displays in Earth Climate and Planetary Atmospheric Research

A. Delgenio, J. Hansen
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Abstract

The communities of scientists who study the Earth's climate and the atmospheres of the other planets barely overlap, but the types of questions they pose and the resulting implications for the use and interpretation of remote sensing data sets have much in common. Both seek to determine the characteristic behavior of three-dimensional fluids that also evolve in time. Climate researchers want to know how and why the general patterns that define our climate today might be different in the next century. Planetary scientists try to understand why circulation patterns and clouds on Mars, Venus, or Jupiter are different from those on Earth. Both disciplines must aggregate large amounts of data covering long time periods and several altitudes to have a representative picture of the rapidly changing atmosphere they are studying. This emphasis separates climate scientists from weather forecasters, who focus at any one time on a limited number of images. Likewise, it separates planetary atmosphere researchers from planetary geologists, who rely primarily on single images (or mosaics of images covering the globe) to study two-dimensional planetary surfaces that are mostly static over the duration of a spacecraft mission yet reveal dynamic processes acting over thousands to millions of years. Remote sensing displays are usually two-dimensional projections that capture an atmosphere at an instant in time. How scientists manipulate and display such data, how they interpret what they see, and how they thereby understand the physical processes that cause what they see, are the challenges I discuss in this chapter. I begin by discussing differences in how novices and experts in the field relate displays of data to the real world. This leads to a discussion of the use and abuse of image enhancement and color in remote sensing displays. I then show some examples of techniques used by scientists in climate and planetary research to both convey information and design research strategies using remote sensing displays.
遥感显示在地球气候和行星大气研究中的作用
研究地球气候和其他行星大气的科学家群体几乎没有重叠,但他们提出的问题类型以及由此产生的对遥感数据集的使用和解释的影响有很多共同点。两者都试图确定也随时间演化的三维流体的特征行为。气候研究人员想知道,今天定义我们气候的一般模式在下个世纪可能会如何以及为什么会有所不同。行星科学家试图理解为什么火星、金星或木星上的循环模式和云层与地球上的不同。这两个学科都必须收集涵盖长时间和多个高度的大量数据,才能对他们正在研究的快速变化的大气有一个有代表性的描述。这种强调将气候科学家与天气预报员区分开来,天气预报员在任何时候都只关注有限数量的图像。同样,它将行星大气研究人员与行星地质学家区分开来,后者主要依靠单一图像(或覆盖全球的图像马赛克)来研究二维行星表面,这些行星表面在航天器任务期间大部分是静态的,但揭示了数千年至数百万年的动态过程。遥感显示通常是二维投影,可以捕捉到某一时刻的大气。科学家如何操纵和显示这些数据,他们如何解释他们所看到的,以及他们如何因此理解导致他们所看到的物理过程,是我在本章中讨论的挑战。我将首先讨论该领域的新手和专家如何将数据显示与现实世界联系起来的差异。这导致了对遥感显示中图像增强和颜色的使用和滥用的讨论。然后,我展示了一些科学家在气候和行星研究中使用的技术的例子,这些技术使用遥感显示来传递信息和设计研究策略。
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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