A wind-tunnel investigation of a 0.009 scale model of the Space Launch System (SLS) was conducted in the NASA Langley Unitary Plan Wind Tunnel to characterize the aerodynamics of the core and solid rocket boosters (SRBs) during booster separation. High-pressure air was used to simulate plumes from the booster separation motors (BSMs) located on the nose and aft skirt of the SRBs. Force and moment data were acquired on the core and SRBs. These data were used to corroborate computational fluid dynamics (CFD) calculations that were used in developing a booster separation database. The SRBs could be remotely positioned in the x-, y-, and z-direction relative to the core. Data were acquired continuously while the SRBs were moved in the axial direction. The primary parameters varied during the test were: core pitch angle; SRB pitch and yaw angles; SRB nose x-, y-, and z-position relative to the core; and BSM plenum pressure. The test was conducted at a free-stream Mach number of 4.25 and a unit Reynolds number of 1.5 million per foot.
[1]
Stuart E. Rogers,et al.
Inviscid and Viscous CFD Analysis of Booster Separation for the Space Launch System Vehicle
,
2016
.
[2]
Stuart E. Rogers,et al.
Output-Based Adaptive Meshing Applied to Space Launch System Booster Separation Analysis
,
2015
.
[3]
J. Marroquin,et al.
Results of SRB separation tests using the 0.010-scale SSV model 75-OTS in the AEDC VKF tunnel A(IA142), volume 1
,
1977
.
[4]
W A Crosby,et al.
Integrated Aerodynamic Tests of the Space Shuttle Vehicle during Solid Rocket Booster Separation at Mach 4.5 (IA193).
,
1982
.
[5]
Russ D. Rausch,et al.
An Overview of the Characterization of the Space Launch Vehicle Aerodynamic Environments
,
2014
.