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Seasonal Cycle of Martian Climate: Experimental Data and Numerical Simulation

机译：火星气候的季节周期：实验数据和数值模拟

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摘要

The most adequate theoretical method of investigating the present-day Martian climate is numerical simulation based on a model of general circulation of the atmosphere. First and foremost, such models encounter the greatest difficulties in description of aerosols and clouds, which in turn essentially influence temperature fields, the atmosphere circulation, and transport of water in the atmosphere. On the basis of the method of moments, we proposed and implemented as a model of general circulation of the Martian atmosphere a mathematical tool which allows one to calculate ab initio microphysical processes in water clouds and their macroscopic properties. We present some examples of comparing the model with the data of recent Martian missions and consider the influence of separate elements of the climate system on the seasonal hydrologic cycle of the planet.
机译：研究当今火星气候最合适的理论方法是基于大气总环流模型的数值模拟。首先，这种模型在描述气溶胶和云层时遇到了最大的困难，这反过来又从根本上影响温度场，大气环流和大气中水的输送。在矩量法的基础上，我们提出并实现了一种作为火星大气总环流模型的数学工具，该工具可用来计算水云的从头开始的微观物理过程及其宏观特性。我们提供了一些将模型与最近的火星飞行任务的数据进行比较的示例，并考虑了气候系统各个要素对地球季节性水文循环的影响。

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