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金星大气成分数据汇编

Venus Atmospheric Composition Data: A Compilation.

作者信息

Johnson Natasha M, de Oliveira Marta R R

机构信息

Astrochemistry Laboratory, Code 691, NASA Goddard Space Flight Center, USA.

European Space Agency HQ, France.

出版信息

Earth Space Sci. 2019 Jun 25;6(7):1299-1318. doi: 10.1029/2018EA000536.

DOI:10.1029/2018EA000536
PMID:31709275
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6839549/
Abstract

The Venus atmosphere is of significant interest yet only rudimentary solid data has been gathered about its composition and chemistry. These measurements are scattered through time and place and are limited by parameters such as resolution and error margins as well as reinterpretations. This paper presents an extensive compilation of published data for the atmospheric composition of Venus. It also includes remotely gathered measurements and some extrapolated and modeled data for the lower atmosphere. The composition tables are divided in four categories: noble gases, reactive gases, noble and non-noble isotopes. These tables were first presented in 2016 within the scientific heritage appendix of the Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) mission proposal. These tables provide respective measurements, error margins, techniques, altitudes, instruments, mission and references. The objective of this paper is to provide a simple, comprehensive list of available measurements to date; in particular, the data, to serve as a quick overall Venus atmosphere data reference.

摘要

金星大气层备受关注,但目前仅收集到关于其成分和化学性质的初步可靠数据。这些测量数据在时间和地点上分布零散,并且受到分辨率、误差范围以及重新解释等参数的限制。本文对已发表的金星大气成分数据进行了广泛汇编。它还包括遥感测量数据以及一些低层大气的外推和模拟数据。成分表分为四类:稀有气体、活性气体、稀有和非稀有同位素。这些表格最初于2016年出现在“金星深层大气稀有气体、化学和成像探测”(DAVINCI)任务提案的科学遗产附录中。这些表格提供了各自的测量数据、误差范围、技术、高度、仪器、任务和参考文献。本文的目的是提供一份简单、全面的迄今可用测量数据清单;特别是这些数据,以便作为快速的金星大气整体数据参考。

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引用本文的文献

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3
Narrow range of early habitable Venus scenarios permitted by modeling of oxygen loss and radiogenic argon degassing.模型模拟表明,氧气损失和放射性氩脱气作用下,金星可居住早期的范围很窄。
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Venus' Mass Spectra Show Signs of Disequilibria in the Middle Clouds.金星的质谱显示中层云存在不平衡迹象。
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本文引用的文献

1
A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO.金星冰冻圈中的一个温暖层以及对HF、HCl、H₂O和HDO的高空测量。
Nature. 2007 Nov 29;450(7170):646-9. doi: 10.1038/nature05974.
2
Venus was wet: a measurement of the ratio of deuterium to hydrogen.金星是湿的:氘氢比的测量。
Science. 1982 May 7;216(4546):630-3. doi: 10.1126/science.216.4546.630.
3
Composition and structure of the venus atmosphere: results from pioneer venus.金星大气的成分与结构:金星先锋号探测器的探测结果
Science. 1979 Jul 6;205(4401):49-52. doi: 10.1126/science.205.4401.49.
4
Deuterium on Venus: observations from Earth.金星上的氘:来自地球的观测结果。
Science. 1991 Feb 1;251:547-9. doi: 10.1126/science.251.4993.547.