Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method
In this paper, an initiative Martian dust fluid simulating research based on the energy dissipation method was developed to simulate the deposition process of Martian dust fluid which was caused by surface adhesion between particles and Martian rovers. Firstly, an energy dissipation model of particl...
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Format: | Article |
Language: | English |
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Wiley
2020-01-01
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Series: | International Journal of Aerospace Engineering |
Online Access: | http://dx.doi.org/10.1155/2020/2370385 |
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author | Tianxiang Ding Xuyan Hou Man Li Guangyu Cao Jixuan Liu Xianlin Zeng Zongquan Deng |
author_facet | Tianxiang Ding Xuyan Hou Man Li Guangyu Cao Jixuan Liu Xianlin Zeng Zongquan Deng |
author_sort | Tianxiang Ding |
collection | DOAJ |
description | In this paper, an initiative Martian dust fluid simulating research based on the energy dissipation method was developed to simulate the deposition process of Martian dust fluid which was caused by surface adhesion between particles and Martian rovers. Firstly, an energy dissipation model of particles based on the Discrete Element Method (DEM) was established because of the characteristics of Martian dust particles such as tiny size and viscoelasticity. This model is based on the existing DMT model to analyze the collision deposition of dust fluid particles, including particle-spacecraft collision and particle-particle collision. Secondly, this paper analyzed the characteristics of particles after their first collision, then, established the stochastic model of critical wind speed for the particle deposition process. Finally, a series of simulations of the Martian dust fluid particle deposition process were done based on DEM-CFD. The results verified the accuracy of the energy dissipation model and the stochastic model, which could also verify the feasibility and effectiveness of the computing method of Martian dust fluid based on the DEM-CFD technology. |
format | Article |
id | doaj-art-d98f0980a4a94ecca618f81c8d0a9417 |
institution | Kabale University |
issn | 1687-5966 1687-5974 |
language | English |
publishDate | 2020-01-01 |
publisher | Wiley |
record_format | Article |
series | International Journal of Aerospace Engineering |
spelling | doaj-art-d98f0980a4a94ecca618f81c8d0a94172025-02-03T06:06:55ZengWileyInternational Journal of Aerospace Engineering1687-59661687-59742020-01-01202010.1155/2020/23703852370385Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation MethodTianxiang Ding0Xuyan Hou1Man Li2Guangyu Cao3Jixuan Liu4Xianlin Zeng5Zongquan Deng6State Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaState Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaBeijing Institute of Spacecraft Environment Engineering, China Academy of Space Technology, No. 104 Youyi Street, Haidian, Beijing, 100094, ChinaState Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaState Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaState Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaState Key Laboratory of Robotics and System, Harbin Institute of Technology, No. 2 Yikuang Street, Nangang, Harbin City, Heilongjiang Province, 150080, ChinaIn this paper, an initiative Martian dust fluid simulating research based on the energy dissipation method was developed to simulate the deposition process of Martian dust fluid which was caused by surface adhesion between particles and Martian rovers. Firstly, an energy dissipation model of particles based on the Discrete Element Method (DEM) was established because of the characteristics of Martian dust particles such as tiny size and viscoelasticity. This model is based on the existing DMT model to analyze the collision deposition of dust fluid particles, including particle-spacecraft collision and particle-particle collision. Secondly, this paper analyzed the characteristics of particles after their first collision, then, established the stochastic model of critical wind speed for the particle deposition process. Finally, a series of simulations of the Martian dust fluid particle deposition process were done based on DEM-CFD. The results verified the accuracy of the energy dissipation model and the stochastic model, which could also verify the feasibility and effectiveness of the computing method of Martian dust fluid based on the DEM-CFD technology.http://dx.doi.org/10.1155/2020/2370385 |
spellingShingle | Tianxiang Ding Xuyan Hou Man Li Guangyu Cao Jixuan Liu Xianlin Zeng Zongquan Deng Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method International Journal of Aerospace Engineering |
title | Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method |
title_full | Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method |
title_fullStr | Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method |
title_full_unstemmed | Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method |
title_short | Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method |
title_sort | investigation on computing method of martian dust fluid based on the energy dissipation method |
url | http://dx.doi.org/10.1155/2020/2370385 |
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