Turbulence: An Introduction for Scientists and Engineers
By P. Davidson. 2015
1,247 citations recorded by the source corpus.
Subfields: Computational Mechanics
View Paper: https://www.semanticscholar.org/paper/9d4da8300918b1d3cdb3f433c76fe01bcc197d7b
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In Computational Mechanics
Citations in the corpus
- Detecting gravitational waves from cosmological phase transitions with LISA: an update (2019, background): “e decorrelates, which eectively reduces its lifetime to ˝ v ’ H 1 , as re ected in (24). At the integral scale L f, the autocorrelation time of the turbulent ow corresponds to one eddy turnover time [56]; it therefore features the same parametric dependence as the shock appearance time, ˝ tu ˘L f=U ”
- The turbulent/non-turbulent interface and entrainment in a boundary layer (2012, methodology): “To characterise this difference in ˙ m c ( s ), we turn to the analogous structure function of velocity and the way it is used to characterise the dominant size of eddies (Davidson 2004).”
- Scaling regimes in spherical shell rotating convection (2016, background): “The proportionality relation between the typical time scale at the integral length `⊥ and at the dissipation scale `diss is a distinctive feature of two-dimensional turbulence (e.g. Davidson 2015).”
- Cascades and transitions in turbulent flows (2018, result): “rgy. Both cases have attracted the interest of turbulence research due to the applicability of stratified turbulence (both stable and unstable) to atmospheric dynamics, planetary and stellar interiors [4]. Recently a large number of new results have been revealed due to extensive numerical simulation”
- Holographic Quantum Matter (2016, background): “One of the most fascinating open problems in all of physics is the nonlinear and chaotic dynamics of turbulent fluids, a problem which has important practical and theoretical applications for classical fluids like water and air [164].”
- Solar Wind Turbulence and the Role of Ion Instabilities (2013, background): “dissipation scales ℓd as a function of (a) kρi, (b) kλi, (c) kρe and (d) f/fce. Figure from (Alexandrova et al. 2009), corrected for 3 STAFF-SA frequencies, as explained in (Alexandrova et al. 2012). Davidson 2004), for three different candidates for the dissipation scale ℓd, namely for ρi, λi and ρ”
- Rotating convective turbulence in Earth and planetary cores (2015, background): “…J 104 are typically turbulent, with a broad range of length and time scales as well as cross-scale energy transfers that allow for complex cascades of energy through the system (e.g., Davidson, 2004, 2013; Mininni and Pouquet, 2010; Nataf and Schaeffer, 2015; Ouellette, 2012; Rubio et al., 2014).”