Abstract
To understand the interaction between the SPT-100 thruster and the spacecraft, accurate knowledge of exhaust plume properties must be obtained. This investigation utilized a suite of interrelated diagnostic probes in an effort to provide detailed knowledge of the exhaust plume on a molecular kinetic level. Probes used for the investigation included a retarding potential analyzer, a planar Faraday probe, an emissive probe, both totaland radiant-heat- ux probes, as well as a newly developed neutral particle ux probe. Combining the knowledge gained from these probes it was possible to quantify the transport of mass, energy, and charge within the plume at 0.5and 1.0-m radius from the thruster exit. Among the phenomena uncovered were a high-energy ionic annulus surrounding a narrow low-energy core within the plume at 0.5-m radius from the thruster exit. This core structure was lled in at 1.0-m radius. Additionally, a population of energetic charge-exchange neutrals was found within 25 deg of the thruster centerline along with the corresponding low-energy charge-exchange ions attributed to plume/background gas interactions.
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