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À propos de : DSMC simulation of the vertical structure of planetary rings        

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Title
  • DSMC simulation of the vertical structure of planetary rings
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Abstract
  • A statistical Monte Carlo method (DSMC) is developed to simulate granular flows occurring in dense planetary rings. The accuracy of the method is assessed through a comparison with existing molecular dynamics simulations of the vertical structure of planetary rings with and without self-gravity effects.
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  • aa1328
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  • © ESO, 2001
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  • ESO
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