Electrical Characteristics of the Mars Electrostatic PrecipitatorNASA'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 Electrostatics 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 established for a number of precipitator flow conditions. Corona onset voltage and streamer onset voltage trends versus pressure are also established.
Document ID
20180004171
Acquisition Source
Kennedy Space Center
Document Type
Conference Paper
Authors
Johansen, Michael R. (NASA Kennedy Space Center Cocoa Beach, FL, United States)
Phillips, James R., III (NASA Kennedy Space Center Cocoa Beach, FL, United States)
Wang, Jerry J. (NASA Kennedy Space Center Cocoa Beach, FL, United States)
Mulligan, Jaysen (University of Central Florida Orlando, FL, United States)
Mackey, Paul J. (NASA Kennedy Space Center Cocoa Beach, FL, United States)
Calle, Carlos I. (NASA Kennedy Space Center Cocoa Beach, FL, United States)
Clements, Judson S. (Appalachian State Univ. Boone, NC, United States)