Influence of the drag coefficient model on the dynamics of particle motion in the shock wave from the descent vehicle

Author:

Polyansky Timofey,Zaitsev Alexander

Publisher

AIP Publishing

Reference8 articles.

1. E. B. Vasilevskii, A. V. Chirikhin, and A. N. Osiptsov, “Heat Transfer to a Stagnation Region of a Blunt Body in a Hypersonic Gas Flowwith and Admixture of Solid Particles,” in Aerothermodynamics for space vehicles, ESA Special Publication, Vol. 426, edited by R. A. Harris (1999) pp. 301–307.

2. Physical properties of the particles composing the Martian dust storm of 1971–1972

3. Vertical Structure of Martian Dust Measured by Solar Infrared Occultations from the Phobos Spacecraft

4. Investigation of Martian-Dust Drag and Heat Transfer for Mars Sample Return Mission

5. H. J. Melosh and T. J. Goldin, “Heat and Drag Coefficients for Reentry of Impact Ejecta,” in Lunar and Planetary Science Conference, Lunarand Planetary Science Conference (2008) p. 2457.

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