An investigation has been made of the extent to which outgassed or emitted molecules return to a spacecraft as a result of intermolecular collisions with ambient freestream molecules. The governing parameters are discussed and heuristic arguments are used to predict the combination of parameters that is most likely to describe the return flux ratio. This is then tested by an extensive set of numerical calculations using the direct simulation Monte Carlo method. Computations have been made for the flow past spheres and past circular cylinders with their axes normal in the stream. The numerical results lead to empirical expressions that can be used for engineering estimates in spacecraft contamination studies.
Spacecraft outgas ambient flow interaction
01.02.1981
Sonstige
Keine Angabe
Englisch
Spacecraft outgas ambient flow interaction
AIAA | 1981
|Numerical Study of Behavior of Outgas from Heat Shield of Solar Probe
Online Contents | 2006
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