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This article investigates the inverse Magnus effect on a rotating sphere in hypersonic rarefied flow, highlighting its significance for understanding maneuvering flights and atmospheric entries of space debris. Using the direct simulation Monte Carlo (DSMC) method, the study analyzes flow fields and aerodynamic characteristics, revealing that the inverse Magnus force arises from tangential momentum transfer in rarefied conditions. The findings contribute to predicting trajectories of space debris and enhanc

Author

tareq.mh15

Language

EN