One-Dimensional Model of Vertical Transport of Chemical Components in the Mars Atmosphere up to the Lower Thermosphere

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2024-05-20 DOI:10.1134/s0038094623700041
Y. Kylivnyk, A. S. Petrosyan, A. A. Fedorova, O. I. Korablev
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Abstract

This study is devoted to the analysis of transport of chemical components of the Mars atmosphere. We investigate the turbulent diffusion of chemical components of the Mars atmosphere. To solve this problem in the approximation of diffusion of the minor component, we composed the continuity equation and the corresponding difference scheme. We formulated the boundary conditions in accordance with the available experimental and theoretical data and obtained the required temperature and pressure profiles. For simulation, we chose two models of turbulent diffusion, which were used in subsequent calculations. The simulation was performed using the modified Newton method. The models showed significant differences in the distribution of minor components of the atmosphere, in particular, hydrogen-containing molecules, which indicates the importance of choosing a model for describing turbulent diffusion when constructing a one-dimensional photochemical model of the atmosphere.

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火星大气层中化学成分垂直迁移至低热层的一维模型
摘要--本研究致力于分析火星大气中化学成分的传输。我们研究了火星大气中化学成分的湍流扩散。为了在次要成分扩散近似条件下解决这个问题,我们建立了连续性方程和相应的差分方案。我们根据现有的实验和理论数据制定了边界条件,并获得了所需的温度和压力曲线。为了进行模拟,我们选择了两种湍流扩散模型,并在随后的计算中使用。模拟采用修正牛顿法进行。这两种模型在大气次要成分,特别是含氢分子的分布方面显示出明显的差异,这表明在构建大气一维光化学模型时选择描述湍流扩散的模型非常重要。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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