Molecular shield of “OKA-T” spacecraft


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Resumo

Here, we present the results of computational studies of gas parameters in the high rarefaction zone formed behind a molecular shield mounted on the OKA-T spacecraft. The method of accounting for the effect of solar cell rotation on the rarefaction zone is described. The influence of jets of on-site engines and gas emission of the apparatus on the rarefaction zone has been estimated.

Sobre autores

A. Kashkovsky

Khristianovich Institute of Theoretical and Applied Mechanics SB RAS

Autor responsável pela correspondência
Email: sasa@itam.nsc.ru
Rússia, Novosibirsk

P. Vashchenkov

Khristianovich Institute of Theoretical and Applied Mechanics SB RAS

Email: sasa@itam.nsc.ru
Rússia, Novosibirsk

A. Krylov

RSC “Energia”

Email: sasa@itam.nsc.ru
Rússia, Korolev

L. Mishina

RSC “Energia”

Email: sasa@itam.nsc.ru
Rússia, Korolev

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Declaração de direitos autorais © Kutateladze Institute of Thermophysics, Siberian Branch of the Russian Academy of Sciences, 2018