Hydrodynamic Stability: Contents
By P. Drazin, W. H. Reid. 2004
848 citations recorded by the source corpus.
Subfields: Computational Mechanics
View Paper: https://www.semanticscholar.org/paper/23f1f9f1faec1b71cd945ef6668e5d4678f15926
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Computational Mechanics
- Ati S. Sharma
- B. McKeon
- Ben Thornber
- David Youngs
- R. Williams
- Dimitris Drikakis
- E. Chiang
- Fang Q. Hu
Citations in the corpus
- Forming Planetesimals in Solar and Extrasolar Nebulae (2009, background): “…be a fair analogue for actual vertically shearing flows in disks—the KHI can develop when the Richardson number Ri = (g/ρ)∂ρ/∂z (∂vφ/∂z)2 1 4 (30) somewhere (Drazin & Reid 2004), where g is the vertical gravitational acceleration and ρ = ρp + ρg (see Garaud & Lin 2004, for the applicability of…”
- A Perfectly Matched Layer absorbing boundary condition for linearized Euler equations with a non-uniform mean flow (2005, methodology): “(13) This eigenvalue problem will be solved by a spectral collocation method which is a standard method in hydrodynamic stability analysis[25,10,22].”
- A critical-layer framework for turbulent pipe flow (2010, background): “The scaling of the width of these regions can be determined by consideration of the appropriate terms in (4.5) (for plane flow see Maslowe 1981; Schmid & Henningson 2001; Drazin & Reid 2004).”
- The engine behind (wall) turbulence: perspectives on scale interactions (2017, background): “The manifestation of these resolvent modes appears to be closely described, at least phenomenologically, as a three-dimensional equivalent of Kelvin’s two-dimensional ‘cats’ eyes’ (Drazin & Reid 2004; Sharma & McKeon 2013b).”
- Nonlinear instability of ideal plane flows (2004, neutral): “See [3],[4] and the references therein.”
- The influence of initial conditions on turbulent mixing due to Richtmyer–Meshkov instability† (2010, background): “It is assumed that the acceleration g(t) is very large and occurs over a very short period of time (see e.g. Richtmyer 1960; Drazin & Reid 2004), giving da dt = µk ua+0 At +, (2.1) where At+ = (ρ+2 − ρ+1 )/(ρ+1 + ρ+2 ) is the Atwood number, the plus (+) indicates a post-shock quantity, and µ is a…”