Short-wavelength instabilities of Riemann ellipsoids
From MaRDI portal
Publication:3837453
DOI10.1098/rsta.1996.0037zbMath0885.76036OpenAlexW2322203817MaRDI QIDQ3837453
N. Lebovitz, Alexander Lipton-Lifschitz
Publication date: 29 April 1998
Published in: Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1098/rsta.1996.0037
potential theoryparameter spaceenergy estimatenon-rotating sphereastrophysical flowsfamily of irrotational ellipsoidsnarrow continuumrigidly rotating configurations of Maclaurin and Jacobi
General theory of rotating fluids (76U05) Hydrodynamic stability (76E99) Incompressible inviscid fluids (76B99)
Related Items
On nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem, Latitudinal libration driven flows in triaxial ellipsoids, Nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem with degenerate density dependent viscosities, Some results on Newtonian gaseous stars -- existence and stability, The influence of magnetic field on short-wavelength instability of Riemann ellipsoids, On the weakly nonlinear development of the elliptic instability, Short-wavelength instabilities of edge waves in stratified water, The magnetoelliptic instability of rotating systems, Acoustic and inertial modes in planetary-like rotating ellipsoids, The mathematical development of the classical ellipsoids, Existence of magnetic compressible fluid stars, Stability of stagnation points in rotating flows, Elliptic instability in two-dimensional flattened Taylor–Green vortices, Nonlinear dynamical stability of Newtonian rotating and non-rotating white dwarfs and rotating supermassive stars, Existence and nonlinear stability of rotating star solutions of the compressible Euler-Poisson equations, Inviscid instabilities in rotating ellipsoids on eccentric Kepler orbits, The mean electromotive force generated by elliptic instability
