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Plume-Free Stream Interaction Heating Effects During Orion Crew Module ReentryDuring reentry of the Orion Crew Module (CM), vehicle attitude control will be performed by firing reaction control system (RCS) thrusters. Simulation of RCS plumes and their interaction with the oncoming flow has been difficult for the analysis community due to the large scarf angles of the RCS thrusters and the unsteady nature of the Orion capsule backshell environments. The model for the aerothermal database has thus relied on wind tunnel test data to capture the heating effects of thruster plume interactions with the freestream. These data are only valid for the continuum flow regime of the reentry trajectory. A Direct Simulation Monte Carlo (DSMC) analysis was performed to study the vehicle heating effects that result from the RCS thruster plume interaction with the oncoming freestream flow at high altitudes during Orion CM reentry. The study was performed with the DSMC Analysis Code (DAC). The inflow boundary conditions for the jets were obtained from Data Parallel Line Relaxation (DPLR) computational fluid dynamics (CFD) solutions. Simulations were performed for the roll, yaw, pitch-up and pitch-down jets at altitudes of 105 km, 125 km and 160 km as well as vacuum conditions. For comparison purposes (see Figure 1), the freestream conditions were based on previous DAC simulations performed without active RCS to populate the aerodynamic database for the Orion CM. Other inputs to the analysis included a constant Orbital reentry velocity of 7.5 km/s and angle of attack of 160 degrees. The results of the study showed that the interaction effects decrease quickly with increasing altitude. Also, jets with highly scarfed nozzles cause more severe heating compared to the nozzles with lower scarf angles. The difficulty of performing these simulations was based on the maximum number density and the ratio of number densities between the freestream and the plume for each simulation. The lowest altitude solutions required a substantial amount of computational resources (up to 1800 processors) to simulate approximately 2 billion molecules for the refined (adapted) solutions.
Document ID
20120007843
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Marichalar, J.
(Jacobs Engineering Group, Inc. Houston, TX, United States)
Lumpkin, F.
(NASA Johnson Space Center Houston, TX, United States)
Boyles, K.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 25, 2013
Publication Date
May 18, 2012
Subject Category
Fluid Mechanics And Thermodynamics
Report/Patent Number
JSC-CN-26304
JSC-CN-27436
Meeting Information
Meeting: JANNAF 33rd Exhaust Plume aud Signatures Joint
Location: Monterey, CA
Country: United States
Start Date: December 3, 2012
End Date: December 7, 2012
Sponsors: Department of the Army, Department of the Air Force, American Inst. of Aeronautics and Astronautics, Department of the Navy, NASA Headquarters
Funding Number(s)
CONTRACT_GRANT: NNJ05HI05C
Distribution Limits
Public
Copyright
Public Use Permitted.
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