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NASA NTRS · 20180004172

Electrical Characteristics of the Mars Electrostatic Precipitator

Abstract

NASA's next generation Mars missions will include chemical processing plants to convert the Martian atmosphere into consumable products needed to support astronaut activities. The thin, mostly carbon dioxide atmosphere of Mars is estimated to have 5-10 particles/cu. cm which have a radius of 1.6-2.27 microns on average. These dust particles could potentially foul the chemical process or reduce the purity of the products. Electrostatic precipitation is one possible solution to remove dust particles from the ingested Mars atmosphere. The Electro-statics and Surface Physics Laboratory at NASA's Kennedy Space Center has developed an electrostatic precipitator testbed to understand the intricacies of corona discharges in dusty flows simulating Mars atmospheric conditions. Current-voltage trends have been estab-lished for a number of precipitator flow conditions. Corona onset voltage and streamer onset voltage trends versus pressure are also established.

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BibTeXRIS

Johansen, Michael R., Phillips, James R., III, Wang, Jerry J., Mulligan, Jaysen, Mackey, Paul J., Clements, J. Sid, Calle, Carlos I.. 2018-06-18. Electrical Characteristics of the Mars Electrostatic Precipitator. https://ntrs.nasa.gov/citations/20180004172

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