タイトル | Plume mass flow and optical damage distributions for an MMH/N2O4 RCS thruster |
本文(外部サイト) | http://hdl.handle.net/2060/19740003483 |
著者(英) | Jack, J. R.; Bowman, R. L.; Spisz, E. W. |
著者所属(英) | NASA Lewis Research Center |
発行日 | 1973-01-01 |
言語 | eng |
内容記述 | The data obtained from two recent experiments conducted in a continuing series of experiments at the Lewis Research Center into the contamination characteristics of a 5-pound thrust MMH/N2O4 engine are presented. The primary objectives of these experiments were to establish the angular distribution of condensible exhaust products within the plume and the corresponding optical damage angular distribution of transmitting optical elements attributable to this contaminant. The plume mass flow distribution was measured by five quartz crystal microbalances (QCM's) located at the engine axis evaluation. The fifth QCM was located above the engine and 15 deg behind the nozzle exit plane. The optical damage was determined by ex-situ transmittance measurements for the wavelength range from 0.2 to 0.6 microns on 2.54 cm diameter fused silica discs also located at engine centerline elevation. Both the mass deposition and optical damage angular distributions followed the expected trend of decreasing deposition and damage as the angle between sensor or sample and the nozzle axis increased. A simple plume gas flow equation predicted the deposition distribution reasonably well for angles of up to 55 degrees. The optical damage measurements also indicated significant effects at large angles. |
NASA分類 | PROPULSION SYSTEMS |
レポートNO | 74N11596 NASA-TM-X-71465 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/196794 |