Fluid-Structure Interaction Simulations of Supersonic Parachute Inflation
Speaker: François Cadieux, Computational Aerosciences Branch, NASA Ames Research Center
Presentation
Seminar Slide Deck (PDF-10.7MB)
Abstract
NASA has three upcoming interplanetary robotic exploration missions for which parachutes are a critical component: Mars Sample Return (Mars 2028), DaVinci (Venus 2031), and DragonFly (Titan, 2034). NASA’s Entry Systems Modeling project is funding research and development toward improving our understanding of parachutes and our ability to predict their behavior during inflation where peak loads occur and where the parachute is most likely to fail. As part of this effort, the Launch, Ascent, and Vehicle Aerodynamics (LAVA) team is developing the capability to simulate supersonic parachute inflation. To validate and improve this new capability, we perform fluid-structure interaction (FSI) simulations of the Advanced Supersonic Parachute Inflation Research Experiments' (ASPIRE) third flight test (SR03), which helped certify the Mars 2020 (Perseverance) parachute, for which load pin and accelerometer data is available along with high-speed imagery. We investigate the effects of refining the parachute structural model, the effect of modeling the deceleration of the whole system, and the effect of the initial assumed shape and cross-sectional area of the parachute through several FSI simulations. Results demonstrate improved agreement with the ASPIRE SR03 flight test as the model fidelity is increased. The combined improvements bring the FSI predictions within flight-to-flight variability in many respects.
This work is supported by NASA’s Entry Systems Modeling (ESM) project.
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