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pro vyhledávání: '"H. K. Kadal"'
Publikováno v:
47th AIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition.
Plasma flow in co-axial accelerators for space propulsion applications is highly viscous despite large values of velocity. This is due to the low density of the plasma. Reynolds number estimates for flow in plasma engines can lie in as low a range as