Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow
Explorations involving long-endurance and maneuvering flights in the upper atmosphere, as well as research on atmospheric entries of space debris or asteroids, call for a full understanding of hypersonic rarefied flows. The inverse Magnus effect occurs in the hypersonic rarefied flow past a rotating...
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MDPI AG
2024-01-01
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author | Yazhong Jiang Yuxing Ling Shikang Zhang |
author_facet | Yazhong Jiang Yuxing Ling Shikang Zhang |
author_sort | Yazhong Jiang |
collection | DOAJ |
description | Explorations involving long-endurance and maneuvering flights in the upper atmosphere, as well as research on atmospheric entries of space debris or asteroids, call for a full understanding of hypersonic rarefied flows. The inverse Magnus effect occurs in the hypersonic rarefied flow past a rotating sphere, but the aerodynamic behavior is contrary to the Magnus effect in the continuum flow regime. In this article, a series of such flows are numerically studied using the direct simulation Monte Carlo (DSMC) method. By analyzing the flow fields, as well as the distributions of pressure and shear stress on the sphere, the formation of the inverse Magnus force can be attributed to the tangential momentum transfer between incident gas molecules and the windward surface. The variation laws of aerodynamic parameters with the rotation rate are presented and discussed. |
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language | English |
last_indexed | 2024-03-08T04:00:35Z |
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spelling | doaj.art-766af41c71194c3f88954b6cb447999f2024-02-09T15:07:29ZengMDPI AGApplied Sciences2076-34172024-01-01143104210.3390/app14031042Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied FlowYazhong Jiang0Yuxing Ling1Shikang Zhang2Hubei Key Laboratory of Theory and Application of Advanced Materials Mechanics, School of Science, Wuhan University of Technology, Wuhan 430070, ChinaSchool of Science, Wuhan University of Technology, Wuhan 430070, ChinaSchool of Mechanical and Electronic Engineering, Wuhan University of Technology, Wuhan 430070, ChinaExplorations involving long-endurance and maneuvering flights in the upper atmosphere, as well as research on atmospheric entries of space debris or asteroids, call for a full understanding of hypersonic rarefied flows. The inverse Magnus effect occurs in the hypersonic rarefied flow past a rotating sphere, but the aerodynamic behavior is contrary to the Magnus effect in the continuum flow regime. In this article, a series of such flows are numerically studied using the direct simulation Monte Carlo (DSMC) method. By analyzing the flow fields, as well as the distributions of pressure and shear stress on the sphere, the formation of the inverse Magnus force can be attributed to the tangential momentum transfer between incident gas molecules and the windward surface. The variation laws of aerodynamic parameters with the rotation rate are presented and discussed.https://www.mdpi.com/2076-3417/14/3/1042hypersonicrarefied gas effectMagnus effectDSMC methodupper atmosphere |
spellingShingle | Yazhong Jiang Yuxing Ling Shikang Zhang Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow Applied Sciences hypersonic rarefied gas effect Magnus effect DSMC method upper atmosphere |
title | Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow |
title_full | Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow |
title_fullStr | Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow |
title_full_unstemmed | Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow |
title_short | Investigation of the Inverse Magnus Effect on a Rotating Sphere in Hypersonic Rarefied Flow |
title_sort | investigation of the inverse magnus effect on a rotating sphere in hypersonic rarefied flow |
topic | hypersonic rarefied gas effect Magnus effect DSMC method upper atmosphere |
url | https://www.mdpi.com/2076-3417/14/3/1042 |
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