Abstract
In this chapter we are concerned with the Magnus effect: the phenomenon governing the deflection of the trajectory of a spinning body (for example, a golf ball or a soccer ball). Surprisingly enough, in highly rarefied media (on Mars or in the thin atmosphere at a height corresponding to low Earth orbits: between 100 and 1,000 km) the inverse effect takes place; this means that the trajectory deflection has opposite signs in sparse and in dense media.
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Notes
- 1.
All the computational tests were performed on a PC with a Pentium IV, 2.0 GHz, and 512 MB RAM and using the optimization package Xpress-IVE, Version 1.19.00, with the modeler MOSEL.
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Plakhov, A. (2012). The Magnus Effect and the Dynamics of a Rough Disc. In: Exterior Billiards. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4481-7_7
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