Abstract
To identify the mechanism triggering boundary layer transition on a spherical forebody of an Apollo type re-entry capsule direct numerical simulations of perturbed flow are analyzed. The perturbations are generated by deterministic distributed surface roughnesses that resemble model surface imperfections that are mounted on a capsule model and are experimentally investigated in Radespiel et al. [J. Spacecr. Rockets 56, 405 (2019)]. Therein, the role of distributed roughness in the transition scenario was highlighted but the mechanism remained unclear. In this manuscript, the sensitivity of the flow perturbations with respect to the roughness layout is investigated. The great span of spatial scales, i.e., capsule diameter, boundary layer thickness, and micro-size roughness, define the requirements of the numerical method. Modifications to a finite-volume unstructured Cartesian cut-cell method to meet these requirements are presented. The receptivity of the capsule boundary layer to the roughness and the subsequent disturbance growth are analyzed. The roughness properties at the most downstream position govern the flow perturbation. The impact of the streamwise character of the roughness layout is intensified by increasing the Reynolds number of the flow. The growth mechanism is identified as transient growth and the most amplified disturbances are compared to the results of optimal transient growth theory. Streamwise vortices cause growth via the lift-up effect. However, the wall normal scales of optimal and roughness induced disturbance differ significantly leading to suboptimal growth.
14 More- Received 13 September 2019
- Accepted 30 April 2020
DOI:https://doi.org/10.1103/PhysRevFluids.5.063903
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