The Evaluation of Oxygen Interaction with Materials III experiment, down by
NASA on STS-46, allowed the characterization of the Space Shuttle local en
vironment and the products of material erosion by atomic oxygen (AO) by mas
s spectrometry. Relatively complex transport mechanisms were involved in th
at environment, namely, gasphase collisions and wall reflections. Several s
ituations were simulated by a numerical model: quiescent period or thruster
operation, orientation of spectrometer to analyze Shuttle environment or e
rosion products, and materials directly exposed to ram flux or covered by a
baffle. The comparison between numerical and experimental results yielded
good agreement. That contributed to the experiment interpretation and the v
alidation of the model. It pushed model parameters toward a large AO accomm
odation and a small Kapton(R) erosion efficiency at low AO energy.