Directory: ${PENCIL_HOME}/samples/2d-tests/GMSW1976 SVN Id: $Id$ Maintainer: Added: 13-Apr-2004 Status: succeeds # One of [succeeds|failing since |obsolete| ...] Recommended resolution: 128x128x128 (nu=eta=1.3e-3) Comments: Reproduce critical Rayleigh number for density ratio Z+1 = rho_bot/rho_top=11. and m=1. Assume dynamical viscosity mu=rho*nu and heat conductivity K to be constant. For these values, Gough et al. find a critical Rayleigh number Ra_crit and critical wave number k_crit of Ra_crit = 1189, k_crit*Lz = 2.42 , where Ra is defined as [dT/dz - (dT/dz)_ad)]*g*Lz^4 Ra = ------------------------------ , T*nu*chi K chi = --------- , c_p*rho with respect to the values in the mid-layer (z=-0.6 in our box which ranges from -1.1 to -0.1). The setup in this directory is such that the lowest horizontal mode corresponds to the above value of the critical wave number, and the values of nu and Kbot correspond to a Rayleigh number Ra = 1189.28 . At resolution nx×nz=20×201, we find Ra_crit ~ 1189.2 ; at nx×nz=20×101, Ra_crit ~ 1168.6 ; at nx×nz=20× 51, Ra_crit ~ 1130.1 . Note that we don't need more points in x, since the individual Fourier modes evolve independently as long as the perturbations are small (and the governing equations for perturbations are linear). For diagnostics, use the idL command sequence idL> .r ts idL> plot, ts.t, ts.uzrms ; plot rms of vertical velocity over time idL> plot, ts.t, deriv(ts.t,alog(ts.uzrms)) ; plot growth rate for time series, and idL> .r start idL> .r r idL> .r thermo idL> .r pvert ; vertical profiles idL> .r plot_uu+ss ; visualize velocity and entropy idL> .r Ra ; print Rayleigh number for looking at the latest snapshot. Reference: D. O. Gough, D. R. Moore, E. A. Spiegel, and N. O. Weiss: "Convective instability in a compressible atmosphere. II." Ap.J. 206, 536--542 (1976).