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Effluent sampling of Titan 3 C vehicle exhaustDownwind in situ ground-level measurements of the exhaust from a Titan 3 C launch vehicle were made during a normal launch. The measurement activity was conducted as part of an overall program to obtain field data for comparison with the multilayer dispersion model currently being used to predict the behavior of rocket vehicle exhaust clouds. All measurements were confined to land, ranging from the launch pad to approximately 2 kilometers downwind from the pad. Measurement systems included detectors for hydrogen chloride (HCl), carbon dioxide (CO2), and particulates (Al2O3). Airborne and ground-based optical systems were employed to monitor exhaust cloud rise, growth, and movement. These measurement systems, located along the ground track (45 deg azimuth from the launch pad) of the exhaust cloud, showed no effluents attributable to the launch. Some hydrogen chloride and aluminum oxide were detected in the surface wind direction (15 deg azimuth) from the pad. Comparisons with the model were made in three areas: (1) assumption of cloud geometry at stabilization; (2) prediction of cloud stabilization altitude; and (3) prediction of the path of cloud travel. In addition, the importance of elemental analyses of the particulate samples is illustrated.
Document ID
19750020488
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Gregory, G. L.
(NASA Langley Research Center Hampton, VA, United States)
Storey, R. W., Jr.
(NASA Langley Research Center Hampton, VA, United States)
Date Acquired
September 3, 2013
Publication Date
August 1, 1975
Subject Category
Environment Pollution
Report/Patent Number
L-10120
NASA-TM-X-3228
Accession Number
75N28561
Funding Number(s)
PROJECT: RTOP 989-15-20-01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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