Direct numerical simulation of complete transition to turbulence via oblique breakdown at Mach 3
By Christian S. J. Mayer, Dominic von Terzi, Hermann F. Fasel. Journal of Fluid Mechanics, 2011
132 citations recorded by the source corpus.
Subfields: Aerospace Engineering, Computational Mechanics
View Paper: https://www.semanticscholar.org/paper/cf66dbf2cbee9d5606d9803e9fcda038cd7e0745
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Aerospace Engineering
- Sanjiva K. Lele
- Kenneth J. Franko
- Christoph Hader
- Hermann F. Fasel
- Christophe Bogey
- Christophe Bailly
- Sergio Pirozzoli
- Tim Colonius
In Computational Mechanics
- Christoph Hader
- Sanjiva K. Lele
- Kenneth J. Franko
- Hermann F. Fasel
- Tim Colonius
- Christophe Bailly
- Christophe Bogey
- Sergio Pirozzoli
Citations in the corpus
- Direct numerical simulations of hypersonic boundary-layer transition for a flared cone: fundamental breakdown (2019, methodology): “…wall units obtained for the fundamental breakdown DNS are comparable to the wall units used to resolve a turbulent boundary layer for a flat plate at Mach 3 (Mayer et al. 2011), suggesting that the grid resolution was adequate to capture the main effects of the laminar–turbulent transition process.”
- Breakdown mechanisms and heat transfer overshoot in hypersonic zero pressure gradient boundary layers (2013, methodology): “Mayer et al. (2011) computed in detail the transition of a Mach 3.0 boundary layer due to oblique breakdown.”