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[svn:einsteintoolkit] GRHydro/trunk/test/ (Rev. 254)
by ian.hinder＠aei.mpg.de 25 Jul '11

25 Jul '11

User: hinder Date: 2011/07/25 09:49 AM Modified: /trunk/test/GRHydro_test_tov_ppm_ML/ alp_maximum.xg, alp_norm1.xg, alp_norm2.xg, dens_3D_diagonal.xg, dens_minimum.xg, dens_norm1.xg, dens_x_[16][16].xg, dens_y_[16][16].xg, dens_z_[16][16].xg, eps_3D_diagonal.xg, eps_norm1.xg, eps_norm2.xg, eps_x_[16][16].xg, eps_y_[16][16].xg, eps_z_[16][16].xg, gxx_maximum.xg, gxx_minimum.xg, gxx_norm1.xg, gxx_norm2.xg, gxy_norm1.xg, gxy_norm2.xg, gxz_norm1.xg, gxz_norm2.xg, gyy_maximum.xg, gyy_minimum.xg, gyy_norm1.xg, gyy_norm2.xg, gyz_norm1.xg, gyz_norm2.xg, gzz_maximum.xg, gzz_minimum.xg, gzz_norm1.xg, gzz_norm2.xg, ham_3D_diagonal.xg, ham_maximum.xg, ham_minimum.xg, ham_norm1.xg, ham_norm2.xg, ham_x_[16][16].xg, ham_y_[16][16].xg, ham_z_[16][16].xg, kxx_maximum.xg, kxx_minimum.xg, kxx_norm1.xg, kxx_norm2.xg, kxy_norm1.xg, kxy_norm2.xg, kxz_norm1.xg, kxz_norm2.xg, kyy_maximum.xg, kyy_minimum.xg, kyy_norm1.xg, kyy_norm2.xg, kyz_norm1.xg, kyz_norm2.xg, kzz_maximum.xg, kzz_minimum.xg, kzz_norm1.xg, kzz_norm2.xg, momx_3D_diagonal.xg, momx_maximum.xg, momx_minimum.xg, momx_norm1.xg, momx_norm2.xg, momx_x_[16][16].xg, momx_y_[16][16].xg, momx_z_[16][16].xg, momy_3D_diagonal.xg, momy_maximum.xg, momy_minimum.xg, momy_norm1.xg, momy_norm2.xg, momy_x_[16][16].xg, momy_y_[16][16].xg, momy_z_[16][16].xg, momz_3D_diagonal.xg, momz_maximum.xg, momz_minimum.xg, momz_norm1.xg, momz_norm2.xg, momz_x_[16][16].xg, momz_y_[16][16].xg, momz_z_[16][16].xg, press_3D_diagonal.xg, press_x_[16][16].xg, press_y_[16][16].xg, press_z_[16][16].xg, rho_3D_diagonal.xg, rho_norm1.xg, rho_x_[16][16].xg, rho_y_[16][16].xg, rho_z_[16][16].xg, scon[0]_3D_diagonal.xg, scon[0]_norm1.xg, scon[0]_norm2.xg, scon[0]_x_[16][16].xg, scon[0]_y_[16][16].xg, scon[0]_z_[16][16].xg, scon[1]_3D_diagonal.xg, scon[1]_norm1.xg, scon[1]_norm2.xg, scon[1]_x_[16][16].xg, scon[1]_y_[16][16].xg, scon[1]_z_[16][16].xg, scon[2]_3D_diagonal.xg, scon[2]_norm1.xg, scon[2]_norm2.xg, scon[2]_x_[16][16].xg, scon[2]_y_[16][16].xg, scon[2]_z_[16][16].xg, tau_3D_diagonal.xg, tau_norm1.xg, tau_x_[16][16].xg, tau_y_[16][16].xg, tau_z_[16][16].xg, vel[0]_3D_diagonal.xg, vel[0]_maximum.xg, vel[0]_minimum.xg, vel[0]_norm1.xg, vel[0]_norm2.xg, vel[0]_x_[16][16].xg, vel[0]_y_[16][16].xg, vel[0]_z_[16][16].xg, vel[1]_3D_diagonal.xg, vel[1]_maximum.xg, vel[1]_minimum.xg, vel[1]_norm1.xg, vel[1]_norm2.xg, vel[1]_x_[16][16].xg, vel[1]_y_[16][16].xg, vel[1]_z_[16][16].xg, vel[2]_3D_diagonal.xg, vel[2]_maximum.xg, vel[2]_minimum.xg, vel[2]_norm1.xg, vel[2]_norm2.xg, vel[2]_x_[16][16].xg, vel[2]_y_[16][16].xg, vel[2]_z_[16][16].xg, w_lorentz_3D_diagonal.xg, w_lorentz_maximum.xg, w_lorentz_norm1.xg, w_lorentz_norm2.xg, w_lorentz_x_[16][16].xg, w_lorentz_y_[16][16].xg, w_lorentz_z_[16][16].xg /trunk/test/GRHydro_test_tov_ppm_ML_disable_internal_excision/ alp_maximum.xg, alp_norm1.xg, alp_norm2.xg, dens_3D_diagonal.xg, dens_minimum.xg, dens_norm1.xg, dens_x_[16][16].xg, dens_y_[16][16].xg, dens_z_[16][16].xg, eps_3D_diagonal.xg, eps_norm1.xg, eps_norm2.xg, eps_x_[16][16].xg, eps_y_[16][16].xg, eps_z_[16][16].xg, gxx_maximum.xg, gxx_minimum.xg, gxx_norm1.xg, gxx_norm2.xg, gxy_norm1.xg, gxy_norm2.xg, gxz_norm1.xg, gxz_norm2.xg, gyy_maximum.xg, gyy_minimum.xg, gyy_norm1.xg, gyy_norm2.xg, gyz_norm1.xg, gyz_norm2.xg, gzz_maximum.xg, gzz_minimum.xg, gzz_norm1.xg, gzz_norm2.xg, ham_3D_diagonal.xg, ham_maximum.xg, ham_minimum.xg, ham_norm1.xg, ham_norm2.xg, ham_x_[16][16].xg, ham_y_[16][16].xg, ham_z_[16][16].xg, kxx_maximum.xg, kxx_minimum.xg, kxx_norm1.xg, kxx_norm2.xg, kxy_norm1.xg, kxy_norm2.xg, kxz_norm1.xg, kxz_norm2.xg, kyy_maximum.xg, kyy_minimum.xg, kyy_norm1.xg, kyy_norm2.xg, kyz_norm1.xg, kyz_norm2.xg, kzz_maximum.xg, kzz_minimum.xg, kzz_norm1.xg, kzz_norm2.xg, momx_3D_diagonal.xg, momx_maximum.xg, momx_minimum.xg, momx_norm1.xg, momx_norm2.xg, momx_x_[16][16].xg, momx_y_[16][16].xg, momx_z_[16][16].xg, momy_3D_diagonal.xg, momy_maximum.xg, momy_minimum.xg, momy_norm1.xg, momy_norm2.xg, momy_x_[16][16].xg, momy_y_[16][16].xg, momy_z_[16][16].xg, momz_3D_diagonal.xg, momz_maximum.xg, momz_minimum.xg, momz_norm1.xg, momz_norm2.xg, momz_x_[16][16].xg, momz_y_[16][16].xg, momz_z_[16][16].xg, press_3D_diagonal.xg, press_x_[16][16].xg, press_y_[16][16].xg, press_z_[16][16].xg, rho_3D_diagonal.xg, rho_norm1.xg, rho_x_[16][16].xg, rho_y_[16][16].xg, rho_z_[16][16].xg, scon[0]_3D_diagonal.xg, scon[0]_norm1.xg, scon[0]_norm2.xg, scon[0]_x_[16][16].xg, scon[0]_y_[16][16].xg, scon[0]_z_[16][16].xg, scon[1]_3D_diagonal.xg, scon[1]_norm1.xg, scon[1]_norm2.xg, scon[1]_x_[16][16].xg, scon[1]_y_[16][16].xg, scon[1]_z_[16][16].xg, scon[2]_3D_diagonal.xg, scon[2]_norm1.xg, scon[2]_norm2.xg, scon[2]_x_[16][16].xg, scon[2]_y_[16][16].xg, scon[2]_z_[16][16].xg, tau_3D_diagonal.xg, tau_norm1.xg, tau_x_[16][16].xg, tau_y_[16][16].xg, tau_z_[16][16].xg, vel[0]_3D_diagonal.xg, vel[0]_maximum.xg, vel[0]_minimum.xg, vel[0]_norm1.xg, vel[0]_norm2.xg, vel[0]_x_[16][16].xg, vel[0]_y_[16][16].xg, vel[0]_z_[16][16].xg, vel[1]_3D_diagonal.xg, vel[1]_maximum.xg, vel[1]_minimum.xg, vel[1]_norm1.xg, vel[1]_norm2.xg, vel[1]_x_[16][16].xg, vel[1]_y_[16][16].xg, vel[1]_z_[16][16].xg, vel[2]_3D_diagonal.xg, vel[2]_maximum.xg, vel[2]_minimum.xg, vel[2]_norm1.xg, vel[2]_norm2.xg, vel[2]_x_[16][16].xg, vel[2]_y_[16][16].xg, vel[2]_z_[16][16].xg, w_lorentz_3D_diagonal.xg, w_lorentz_maximum.xg, w_lorentz_norm1.xg, w_lorentz_norm2.xg, w_lorentz_x_[16][16].xg, w_lorentz_y_[16][16].xg, w_lorentz_z_[16][16].xg /trunk/test/GRHydro_test_tov_ppm_no_trp_ML/ alp_maximum.xg, alp_norm1.xg, alp_norm2.xg, dens_3D_diagonal.xg, dens_minimum.xg, dens_norm1.xg, dens_x_[16][16].xg, dens_y_[16][16].xg, dens_z_[16][16].xg, eps_3D_diagonal.xg, eps_norm1.xg, eps_norm2.xg, eps_x_[16][16].xg, eps_y_[16][16].xg, eps_z_[16][16].xg, gxx_maximum.xg, gxx_minimum.xg, gxx_norm1.xg, gxx_norm2.xg, gxy_norm1.xg, gxy_norm2.xg, gxz_norm1.xg, gxz_norm2.xg, gyy_maximum.xg, gyy_minimum.xg, gyy_norm1.xg, gyy_norm2.xg, gyz_norm1.xg, gyz_norm2.xg, gzz_maximum.xg, gzz_minimum.xg, gzz_norm1.xg, gzz_norm2.xg, ham_3D_diagonal.xg, ham_maximum.xg, ham_minimum.xg, ham_norm1.xg, ham_norm2.xg, ham_x_[16][16].xg, ham_y_[16][16].xg, ham_z_[16][16].xg, kxx_minimum.xg, kxx_norm1.xg, kxx_norm2.xg, kxy_norm1.xg, kxy_norm2.xg, kxz_norm1.xg, kxz_norm2.xg, kyy_minimum.xg, kyy_norm1.xg, kyy_norm2.xg, kyz_norm1.xg, kyz_norm2.xg, kzz_minimum.xg, kzz_norm1.xg, kzz_norm2.xg, momx_3D_diagonal.xg, momx_maximum.xg, momx_minimum.xg, momx_norm1.xg, momx_norm2.xg, momx_x_[16][16].xg, momx_y_[16][16].xg, momx_z_[16][16].xg, momy_3D_diagonal.xg, momy_maximum.xg, momy_minimum.xg, momy_norm1.xg, momy_norm2.xg, momy_x_[16][16].xg, momy_y_[16][16].xg, momy_z_[16][16].xg, momz_3D_diagonal.xg, momz_maximum.xg, momz_minimum.xg, momz_norm1.xg, momz_norm2.xg, momz_x_[16][16].xg, momz_y_[16][16].xg, momz_z_[16][16].xg, press_3D_diagonal.xg, press_x_[16][16].xg, press_y_[16][16].xg, press_z_[16][16].xg, rho_3D_diagonal.xg, rho_norm1.xg, rho_x_[16][16].xg, rho_y_[16][16].xg, rho_z_[16][16].xg, scon[0]_3D_diagonal.xg, scon[0]_norm1.xg, scon[0]_x_[16][16].xg, scon[0]_y_[16][16].xg, scon[0]_z_[16][16].xg, scon[1]_3D_diagonal.xg, scon[1]_norm1.xg, scon[1]_x_[16][16].xg, scon[1]_y_[16][16].xg, scon[1]_z_[16][16].xg, scon[2]_3D_diagonal.xg, scon[2]_norm1.xg, scon[2]_x_[16][16].xg, scon[2]_y_[16][16].xg, scon[2]_z_[16][16].xg, tau_3D_diagonal.xg, tau_norm1.xg, tau_x_[16][16].xg, tau_y_[16][16].xg, tau_z_[16][16].xg, vel[0]_3D_diagonal.xg, vel[0]_maximum.xg, vel[0]_minimum.xg, vel[0]_norm1.xg, vel[0]_norm2.xg, vel[0]_x_[16][16].xg, vel[0]_y_[16][16].xg, vel[0]_z_[16][16].xg, vel[1]_3D_diagonal.xg, vel[1]_maximum.xg, vel[1]_minimum.xg, vel[1]_norm1.xg, vel[1]_norm2.xg, vel[1]_x_[16][16].xg, vel[1]_y_[16][16].xg, vel[1]_z_[16][16].xg, vel[2]_3D_diagonal.xg, vel[2]_maximum.xg, vel[2]_minimum.xg, vel[2]_norm1.xg, vel[2]_norm2.xg, vel[2]_x_[16][16].xg, vel[2]_y_[16][16].xg, vel[2]_z_[16][16].xg, w_lorentz_3D_diagonal.xg, w_lorentz_maximum.xg, w_lorentz_norm1.xg, w_lorentz_norm2.xg, w_lorentz_x_[16][16].xg, w_lorentz_y_[16][16].xg, w_lorentz_z_[16][16].xg Log: Regenerate test results File Changes: Directory: /trunk/test/GRHydro_test_tov_ppm_ML/ =============================================== File [modified]: alp_maximum.xg Delta lines: <Unavailable> File [modified]: alp_norm1.xg Delta lines: <Unavailable> File [modified]: alp_norm2.xg Delta lines: <Unavailable> File [modified]: dens_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: dens_minimum.xg Delta lines: <Unavailable> File [modified]: dens_norm1.xg Delta lines: <Unavailable> File [modified]: dens_x_[16][16].xg Delta lines: <Unavailable> File [modified]: dens_y_[16][16].xg Delta lines: <Unavailable> File [modified]: dens_z_[16][16].xg Delta lines: <Unavailable> File [modified]: eps_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: eps_norm1.xg Delta lines: <Unavailable> File [modified]: eps_norm2.xg Delta lines: <Unavailable> File [modified]: eps_x_[16][16].xg Delta lines: <Unavailable> File [modified]: eps_y_[16][16].xg Delta lines: <Unavailable> File [modified]: eps_z_[16][16].xg Delta lines: <Unavailable> File [modified]: gxx_maximum.xg Delta lines: <Unavailable> File [modified]: gxx_minimum.xg Delta lines: <Unavailable> File [modified]: gxx_norm1.xg Delta lines: <Unavailable> File [modified]: gxx_norm2.xg Delta lines: <Unavailable> File [modified]: gxy_norm1.xg Delta lines: <Unavailable> File [modified]: gxy_norm2.xg Delta lines: <Unavailable> File [modified]: gxz_norm1.xg Delta lines: <Unavailable> File [modified]: gxz_norm2.xg Delta lines: <Unavailable> File [modified]: gyy_maximum.xg Delta lines: <Unavailable> File [modified]: gyy_minimum.xg Delta lines: <Unavailable> File [modified]: gyy_norm1.xg Delta lines: <Unavailable> File [modified]: gyy_norm2.xg Delta lines: <Unavailable> File [modified]: gyz_norm1.xg Delta lines: <Unavailable> File [modified]: gyz_norm2.xg Delta lines: <Unavailable> File [modified]: gzz_maximum.xg Delta lines: <Unavailable> File [modified]: gzz_minimum.xg Delta lines: <Unavailable> File [modified]: gzz_norm1.xg Delta lines: <Unavailable> File [modified]: gzz_norm2.xg Delta lines: <Unavailable> File [modified]: ham_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: ham_maximum.xg Delta lines: <Unavailable> File [modified]: ham_minimum.xg Delta lines: <Unavailable> File [modified]: ham_norm1.xg Delta lines: <Unavailable> File [modified]: ham_norm2.xg Delta lines: <Unavailable> File [modified]: ham_x_[16][16].xg Delta lines: <Unavailable> File [modified]: ham_y_[16][16].xg Delta lines: <Unavailable> File [modified]: ham_z_[16][16].xg Delta lines: <Unavailable> File [modified]: kxx_maximum.xg Delta lines: <Unavailable> File [modified]: kxx_minimum.xg Delta lines: <Unavailable> File [modified]: kxx_norm1.xg Delta lines: <Unavailable> File [modified]: kxx_norm2.xg Delta lines: <Unavailable> File [modified]: kxy_norm1.xg Delta lines: <Unavailable> File [modified]: kxy_norm2.xg Delta lines: <Unavailable> File [modified]: kxz_norm1.xg Delta lines: <Unavailable> File [modified]: kxz_norm2.xg Delta lines: <Unavailable> File [modified]: kyy_maximum.xg Delta lines: <Unavailable> File [modified]: kyy_minimum.xg Delta lines: <Unavailable> File [modified]: kyy_norm1.xg Delta lines: <Unavailable> File [modified]: kyy_norm2.xg Delta lines: <Unavailable> File [modified]: kyz_norm1.xg Delta lines: <Unavailable> File [modified]: kyz_norm2.xg Delta lines: <Unavailable> File [modified]: kzz_maximum.xg Delta lines: <Unavailable> File [modified]: kzz_minimum.xg Delta lines: <Unavailable> File [modified]: kzz_norm1.xg Delta lines: <Unavailable> File [modified]: kzz_norm2.xg Delta lines: <Unavailable> File [modified]: momx_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momx_maximum.xg Delta lines: <Unavailable> File [modified]: momx_minimum.xg Delta lines: <Unavailable> File [modified]: momx_norm1.xg Delta lines: <Unavailable> File [modified]: momx_norm2.xg Delta lines: <Unavailable> File [modified]: momx_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momx_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momx_z_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momy_maximum.xg Delta lines: <Unavailable> File [modified]: momy_minimum.xg Delta lines: <Unavailable> File [modified]: momy_norm1.xg Delta lines: <Unavailable> File [modified]: momy_norm2.xg Delta lines: <Unavailable> File [modified]: momy_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_z_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momz_maximum.xg Delta lines: <Unavailable> File [modified]: momz_minimum.xg Delta lines: <Unavailable> File [modified]: momz_norm1.xg Delta lines: <Unavailable> File [modified]: momz_norm2.xg Delta lines: <Unavailable> File [modified]: momz_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_z_[16][16].xg Delta lines: <Unavailable> File [modified]: press_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: press_x_[16][16].xg Delta lines: <Unavailable> File [modified]: press_y_[16][16].xg Delta lines: <Unavailable> File [modified]: press_z_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: rho_norm1.xg Delta lines: <Unavailable> File [modified]: rho_x_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_y_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[0]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[0]_norm2.xg Delta lines: <Unavailable> File [modified]: scon[0]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[1]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[1]_norm2.xg Delta lines: <Unavailable> File [modified]: scon[1]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[2]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[2]_norm2.xg Delta lines: <Unavailable> File [modified]: scon[2]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: tau_norm1.xg Delta lines: <Unavailable> File [modified]: tau_x_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_y_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_z_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: vel[0]_maximum.xg Delta lines: <Unavailable> File [modified]: vel[0]_minimum.xg Delta lines: <Unavailable> File [modified]: vel[0]_norm1.xg Delta lines: <Unavailable> File [modified]: vel[0]_norm2.xg Delta lines: <Unavailable> File [modified]: vel[0]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[1]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: vel[1]_maximum.xg Delta lines: <Unavailable> File [modified]: vel[1]_minimum.xg Delta lines: <Unavailable> File [modified]: vel[1]_norm1.xg Delta lines: <Unavailable> File [modified]: vel[1]_norm2.xg Delta lines: <Unavailable> File [modified]: vel[1]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[1]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[1]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[2]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: vel[2]_maximum.xg Delta lines: <Unavailable> File [modified]: vel[2]_minimum.xg Delta lines: <Unavailable> File [modified]: vel[2]_norm1.xg Delta lines: <Unavailable> File [modified]: vel[2]_norm2.xg Delta lines: <Unavailable> File [modified]: vel[2]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[2]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[2]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: w_lorentz_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: w_lorentz_maximum.xg Delta lines: <Unavailable> File [modified]: w_lorentz_norm1.xg Delta lines: <Unavailable> File [modified]: w_lorentz_norm2.xg Delta lines: <Unavailable> File [modified]: w_lorentz_x_[16][16].xg Delta lines: <Unavailable> File [modified]: w_lorentz_y_[16][16].xg Delta lines: <Unavailable> File [modified]: w_lorentz_z_[16][16].xg Delta lines: <Unavailable> Directory: /trunk/test/GRHydro_test_tov_ppm_ML_disable_internal_excision/ ========================================================================= File [modified]: alp_maximum.xg Delta lines: <Unavailable> File [modified]: alp_norm1.xg Delta lines: <Unavailable> File [modified]: alp_norm2.xg Delta lines: <Unavailable> File [modified]: dens_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: dens_minimum.xg Delta lines: <Unavailable> File [modified]: dens_norm1.xg Delta lines: <Unavailable> File [modified]: dens_x_[16][16].xg Delta lines: <Unavailable> File [modified]: dens_y_[16][16].xg Delta lines: <Unavailable> File [modified]: dens_z_[16][16].xg Delta lines: <Unavailable> File [modified]: eps_3D_diagonal.xg Delta lines: 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[modified]: w_lorentz_maximum.xg Delta lines: <Unavailable> File [modified]: w_lorentz_norm1.xg Delta lines: <Unavailable> File [modified]: w_lorentz_norm2.xg Delta lines: <Unavailable> File [modified]: w_lorentz_x_[16][16].xg Delta lines: <Unavailable> File [modified]: w_lorentz_y_[16][16].xg Delta lines: <Unavailable> File [modified]: w_lorentz_z_[16][16].xg Delta lines: <Unavailable> Directory: /trunk/test/GRHydro_test_tov_ppm_no_trp_ML/ ====================================================== File [modified]: alp_maximum.xg Delta lines: <Unavailable> File [modified]: alp_norm1.xg Delta lines: <Unavailable> File [modified]: alp_norm2.xg Delta lines: <Unavailable> File [modified]: dens_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: dens_minimum.xg Delta lines: <Unavailable> File [modified]: dens_norm1.xg Delta lines: <Unavailable> File [modified]: dens_x_[16][16].xg Delta lines: <Unavailable> File [modified]: dens_y_[16][16].xg Delta lines: <Unavailable> File [modified]: 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[modified]: kxx_norm1.xg Delta lines: <Unavailable> File [modified]: kxx_norm2.xg Delta lines: <Unavailable> File [modified]: kxy_norm1.xg Delta lines: <Unavailable> File [modified]: kxy_norm2.xg Delta lines: <Unavailable> File [modified]: kxz_norm1.xg Delta lines: <Unavailable> File [modified]: kxz_norm2.xg Delta lines: <Unavailable> File [modified]: kyy_minimum.xg Delta lines: <Unavailable> File [modified]: kyy_norm1.xg Delta lines: <Unavailable> File [modified]: kyy_norm2.xg Delta lines: <Unavailable> File [modified]: kyz_norm1.xg Delta lines: <Unavailable> File [modified]: kyz_norm2.xg Delta lines: <Unavailable> File [modified]: kzz_minimum.xg Delta lines: <Unavailable> File [modified]: kzz_norm1.xg Delta lines: <Unavailable> File [modified]: kzz_norm2.xg Delta lines: <Unavailable> File [modified]: momx_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momx_maximum.xg Delta lines: <Unavailable> File [modified]: momx_minimum.xg Delta lines: <Unavailable> File [modified]: momx_norm1.xg Delta lines: <Unavailable> File [modified]: momx_norm2.xg Delta lines: <Unavailable> File [modified]: momx_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momx_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momx_z_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momy_maximum.xg Delta lines: <Unavailable> File [modified]: momy_minimum.xg Delta lines: <Unavailable> File [modified]: momy_norm1.xg Delta lines: <Unavailable> File [modified]: momy_norm2.xg Delta lines: <Unavailable> File [modified]: momy_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momy_z_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: momz_maximum.xg Delta lines: <Unavailable> File [modified]: momz_minimum.xg Delta lines: <Unavailable> File [modified]: momz_norm1.xg Delta lines: <Unavailable> File [modified]: momz_norm2.xg Delta lines: <Unavailable> File [modified]: momz_x_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_y_[16][16].xg Delta lines: <Unavailable> File [modified]: momz_z_[16][16].xg Delta lines: <Unavailable> File [modified]: press_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: press_x_[16][16].xg Delta lines: <Unavailable> File [modified]: press_y_[16][16].xg Delta lines: <Unavailable> File [modified]: press_z_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: rho_norm1.xg Delta lines: <Unavailable> File [modified]: rho_x_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_y_[16][16].xg Delta lines: <Unavailable> File [modified]: rho_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[0]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[0]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[0]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[1]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[1]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[1]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: scon[2]_norm1.xg Delta lines: <Unavailable> File [modified]: scon[2]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: scon[2]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: tau_norm1.xg Delta lines: <Unavailable> File [modified]: tau_x_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_y_[16][16].xg Delta lines: <Unavailable> File [modified]: tau_z_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: vel[0]_maximum.xg Delta lines: <Unavailable> File [modified]: vel[0]_minimum.xg Delta lines: <Unavailable> File [modified]: vel[0]_norm1.xg Delta lines: <Unavailable> File [modified]: vel[0]_norm2.xg Delta lines: <Unavailable> File [modified]: vel[0]_x_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_y_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[0]_z_[16][16].xg Delta lines: <Unavailable> File [modified]: vel[1]_3D_diagonal.xg Delta lines: <Unavailable> File [modified]: vel[1]_maximum.xg Delta lines: <Unavailable> File [modified]: vel[1]_minimum.xg Delta lines: <Unavailable> File [modified]: vel[1]_norm1.xg Delta lines: <Unavailable> File [modified]: vel[1]_norm2.xg Delta lines: <Unavailable> File [modified]: vel[1]_x_[16][16].xg Delta lines: <Unavailable> 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[svn:einsteintoolkit] GRHydro/trunk/test/ (Rev. 253)
by ian.hinder＠aei.mpg.de 25 Jul '11

25 Jul '11

User: hinder Date: 2011/07/25 09:47 AM Modified: /trunk/test/ GRHydro_test_tov_ppm_ML.par, GRHydro_test_tov_ppm_ML_disable_internal_excision.par, GRHydro_test_tov_ppm_no_trp_ML.par Log: Use 2 CoordBase boundary points instead of 1 in McLachlan tests McLachlan (ML_BSSN_O2) requires two ghost/boundary points due to the dissipation and upwinded advection operators. Kranc-generated thorns now check that the correct number of ghost and boundary points are available, and this check causes three GRHydro tests to fail as they use a boundary size of 1. It turns out that if you disable the check, the original GRHydro test suite still passes on Intel with Linux (Damiana) but segfaulted on GCC with Mac OS (my laptop). The dissipation and unwinding operators will be reading off the edge of the grid, so the behavior is undefined. Dissipation is set to 0 in this test, but a nonzero shift is used. This commit sets the CoordBase boundary size to 2 in the tests, and this requires the test data to be regenerated (the following commit). File Changes: Directory: /trunk/test/ ======================= File [modified]: GRHydro_test_tov_ppm_ML.par Delta lines: +7 -0 =================================================================== --- trunk/test/GRHydro_test_tov_ppm_ML.par 2011-07-20 18:06:13 UTC (rev 252) +++ trunk/test/GRHydro_test_tov_ppm_ML.par 2011-07-25 14:47:17 UTC (rev 253) @@ -48,6 +48,13 @@ driver::ghost_size = 3 driver::global_nsize = 33 +CoordBase::boundary_size_x_lower = 2 +CoordBase::boundary_size_y_lower = 2 +CoordBase::boundary_size_z_lower = 2 +CoordBase::boundary_size_x_upper = 2 +CoordBase::boundary_size_y_upper = 2 +CoordBase::boundary_size_z_upper = 2 + cactus::cctk_itlast = 7 methodoflines::ode_method = "icn" File [modified]: GRHydro_test_tov_ppm_ML_disable_internal_excision.par Delta lines: +7 -0 =================================================================== --- trunk/test/GRHydro_test_tov_ppm_ML_disable_internal_excision.par 2011-07-20 18:06:13 UTC (rev 252) +++ trunk/test/GRHydro_test_tov_ppm_ML_disable_internal_excision.par 2011-07-25 14:47:17 UTC (rev 253) @@ -48,6 +48,13 @@ driver::ghost_size = 3 driver::global_nsize = 33 +CoordBase::boundary_size_x_lower = 2 +CoordBase::boundary_size_y_lower = 2 +CoordBase::boundary_size_z_lower = 2 +CoordBase::boundary_size_x_upper = 2 +CoordBase::boundary_size_y_upper = 2 +CoordBase::boundary_size_z_upper = 2 + cactus::cctk_itlast = 7 methodoflines::ode_method = "icn" File [modified]: GRHydro_test_tov_ppm_no_trp_ML.par Delta lines: +7 -0 =================================================================== --- trunk/test/GRHydro_test_tov_ppm_no_trp_ML.par 2011-07-20 18:06:13 UTC (rev 252) +++ trunk/test/GRHydro_test_tov_ppm_no_trp_ML.par 2011-07-25 14:47:17 UTC (rev 253) @@ -48,6 +48,13 @@ driver::ghost_size = 3 driver::global_nsize = 33 +CoordBase::boundary_size_x_lower = 2 +CoordBase::boundary_size_y_lower = 2 +CoordBase::boundary_size_z_lower = 2 +CoordBase::boundary_size_x_upper = 2 +CoordBase::boundary_size_y_upper = 2 +CoordBase::boundary_size_z_upper = 2 + cactus::cctk_itlast = 7 methodoflines::ode_method = "icn"

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[svn:einsteintoolkit] GRHydro/trunk/src/ (Rev. 252)
by bcmsma＠astro.rit.edu 20 Jul '11

20 Jul '11

User: bmundim Date: 2011/07/20 01:06 PM Added: /trunk/src/ GRHydro_ENOReconstruct_drv.F90, GRHydro_PPMReconstruct_drv.F90, GRHydro_TVDReconstruct_drv.F90 Modified: /trunk/src/ GRHydro_Reconstruct.F90, make.code.defn Log: RIT GRMHD dev: split reconstruct routine. Comments: 1) The reconstruct routine is the most expensive routine in GRHydro and may require some serious thought in the future regarding optimization. 2) This routine was merged by the end of the last year. With too many loops, the compiler wasn't able to fully optimize it (and it would warn about that). 3) With this split, the code became easier to read, the compiler was able to fully optimize it, but we only have a marginal gain in the routine performance (3.2%). Further optimization and clean-up is still desirable. File Changes: Directory: /trunk/src/ ====================== File [added]: GRHydro_ENOReconstruct_drv.F90 Delta lines: <Unavailable> File [added]: GRHydro_PPMReconstruct_drv.F90 Delta lines: <Unavailable> File [modified]: GRHydro_Reconstruct.F90 Delta lines: <Unavailable> File [added]: GRHydro_TVDReconstruct_drv.F90 Delta lines: <Unavailable> File [modified]: make.code.defn Delta lines: <Unavailable>

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[svn:einsteintoolkit] manifest/trunk/ (Rev. 99)
by schnetter＠cct.lsu.edu 17 Jul '11

17 Jul '11

User: eschnett Date: 2011/07/17 11:20 AM Modified: /trunk/ einsteintoolkit.th Log: Undo accidental commit File Changes: Directory: /trunk/ ================== File [modified]: einsteintoolkit.th Delta lines: +2 -77 =================================================================== --- trunk/einsteintoolkit.th 2011-07-16 23:39:02 UTC (rev 98) +++ trunk/einsteintoolkit.th 2011-07-17 16:20:49 UTC (rev 99) @@ -28,7 +28,7 @@ # Simulation Factory !TARGET = $ROOT !TYPE = svn -!URL = https://svn.cct.lsu.edu/repos/numrel/$1/branches/PYSIM_2010 +!URL = https://svn.cct.lsu.edu/repos/numrel/$1/trunk !CHECKOUT = simfactory # Example parameter files @@ -221,18 +221,11 @@ !URL = http://svn.cactuscode.org/projects/$1/$2/trunk !CHECKOUT = ExternalLibraries/BLAS -ExternalLibraries/CGNS -ExternalLibraries/curl -ExternalLibraries/F5 -ExternalLibraries/flickcurl ExternalLibraries/GSL ExternalLibraries/HDF5 -ExternalLibraries/HYPRE ExternalLibraries/LAPACK ExternalLibraries/libjpeg -ExternalLibraries/libxml2 ExternalLibraries/LORENE -#ExternalLibraries/OpenCL ExternalLibraries/OpenSSL #ExternalLibraries/PETSc ExternalLibraries/zlib @@ -251,7 +244,6 @@ AEIThorns/AEILocalInterp AEIThorns/PunctureTracker AEIThorns/SystemStatistics -AEIThorns/TensorTypes @@ -260,12 +252,8 @@ !TYPE = svn !URL = https://svn.cct.lsu.edu/repos/numrel/$1/$2/trunk !CHECKOUT = -LSUDevelopment/Refluxing - -LSUThorns/Flickr LSUThorns/QuasiLocalMeasures LSUThorns/SummationByParts -LSUThorns/Twitter LSUThorns/Vectors @@ -292,8 +280,6 @@ McLachlan/ML_ADMQuantities McLachlan/ML_BSSN McLachlan/ML_BSSN_Helper -McLachlan/ML_BSSN_MP -McLachlan/ML_BSSN_MP_Helper McLachlan/ML_BSSN_O2 McLachlan/ML_BSSN_O2_Helper McLachlan/ML_BSSN_Test @@ -304,8 +290,7 @@ !TARGET = $ARR !TYPE = hg !AUTH_URL = ssh://carpetmercurial@carpetcode.org/carpet -!URL = ssh://carpetmercurial@carpetcode.org/carpet -#!URL = http://www.carpetcode.org/hg/carpet +!URL = http://www.carpetcode.org/hg/carpet # For the git version of Carpet, comment the previous three lines and uncomment # the next three #!TYPE = git @@ -329,69 +314,9 @@ Carpet/CarpetTracker Carpet/LoopControl -CarpetDev/CarpetIOF5 -CarpetDev/CarpetIONirvana -CarpetExtra/AMRToy -CarpetExtra/Nirvana - - -# Llama -!TARGET = $ARR -!TYPE = git -!URL = llama-dev@llamacode.org:Llama -#!URL = login-damiana.aei.mpg.de:/home/ianhin/repositories/Llama -!REPO_PATH= $2 -!CHECKOUT = Llama/ParFiles Llama/README Llama/Thornlists Llama/doc -Llama/ADMDerivatives -Llama/Coordinates -Llama/Gaussian -Llama/GlobalDerivative -Llama/HarmonicDecomposition -Llama/Interpolate -Llama/Interpolate2 -Llama/LlamaHeatToy -Llama/LlamaWaveToy -Llama/MergerHandler -Llama/SphericalSlice -Llama/WaveExtractL -Llama/WorldTube - - - -# CTGamma -!TARGET = $ARR -!TYPE = git -!URL = llama-dev@llamacode.org:CTGamma -!REPO_PATH= $2 -!CHECKOUT = CTGamma/To-Do CTGamma/doc CTGamma/par -CTGamma/CTGBase -CTGamma/CTGConstraints -CTGamma/CTGEvolution -CTGamma/CTGGauge -CTGamma/CTGMatter -CTGamma/CTGRadiativeBC -CTGamma/CartesianCoordinates -CTGamma/Psiclops - - - -# Zelmani -!TARGET = $ARR -!TYPE = git -!URL = carpetgit@stellarcollapse.org:Zelmani.git -!REPO_PATH= $2 -!CHECKOUT = -Zelmani/CoreCollapseControl -Zelmani/ZelmaniHybridCool -Zelmani/ZelmaniStarMapper -Zelmani/ZelmaniLeak - - - # Private thorns !TARGET = $ARR !TYPE = ignore !CHECKOUT = -CarpetExtra/CarpetProlongateTest

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[svn:einsteintoolkit] manifest/trunk/ (Rev. 98)
by schnetter＠cct.lsu.edu 16 Jul '11

16 Jul '11

User: eschnett Date: 2011/07/16 06:39 PM Modified: /trunk/ einsteintoolkit.bib Log: Only suggest citations for Cactus instead of requesting it File Changes: Directory: /trunk/ ================== File [modified]: einsteintoolkit.bib Delta lines: +8 -9 =================================================================== --- trunk/einsteintoolkit.bib 2011-07-16 23:35:30 UTC (rev 97) +++ trunk/einsteintoolkit.bib 2011-07-16 23:39:02 UTC (rev 98) @@ -288,7 +288,7 @@ @Article{Berti:2007nw, author = "Berti, E. and Cardoso, V. and Gonzalez, J. A. and Sperhake, - U. and Bruegmann, Bernd", + U. and Br{\"u}gmann, Bernd", title = "{Multipolar analysis of spinning binaries}", journal = "Class. Quantum Grav.", volume = "25", @@ -407,13 +407,13 @@ ##C ############################################################################ @Misc{Cactuscode:web, - requested-for ={Cactus/Cactus}, + suggested-for ={Cactus/Cactus}, note = {{Cactus} Computational Toolkit}, url = {http://www.cactuscode.org/}, } @Misc{CarpetCode:web, - requested-for ={Carpet/Carpet/Cactus}, + suggested-for ={Carpet/Carpet}, note = {{Carpet}: Adaptive Mesh Refinement for the {Cactus} Framework}, url = {http://www.carpetcode.org/}, @@ -433,8 +433,7 @@ } @Article{Campanelli:2006fg, - author = "Campanelli, Manuela and Lousto, C. O. and Zlochower, Yosef - ", + author = "Campanelli, Manuela and Lousto, C. O. and Zlochower, Yosef", title = "{Spin-orbit interactions in black-hole binaries}", journal = "Phys. Rev. D", volume = "74", @@ -613,7 +612,7 @@ } @InProceedings{Goodale:2002a, - requested-for ={Cactus/Cactus}, + suggested-for ={Cactus/Cactus}, author = {Tom Goodale and Gabrielle Allen and Gerd Lanfermann and Joan Mass{\'o} and Thomas Radke and Edward Seidel and John Shalf}, @@ -630,7 +629,7 @@ @Article{Gopakumar:2007vh, author = "Gopakumar, Achamveedu and Hannam, Mark and Husa, Sascha and - Bruegmann, Bernd", + Br{\"u}gmann, Bernd", title = "{Comparison between numerical relativity and a new class of post-Newtonian gravitational-wave phase evolutions: the non-spinning equal-mass case}", @@ -730,7 +729,7 @@ ##H ############################################################################ @Article{Hannam:2007wf, - author = "Hannam, Mark and Husa, Sascha and Bruegmann, Bernd and + author = "Hannam, Mark and Husa, Sascha and Br{\"u}gmann, Bernd and Gopakumar, Achamveedu", title = "{Comparison between numerical-relativity and post-Newtonian waveforms from spinning binaries: the orbital hang-up @@ -809,7 +808,7 @@ @Article{Husa:2007rh, author = "Husa, Sascha and Hannam, Mark and Gonzalez, Jose A. and - Sperhake, Ulrich and Bruegmann, Bernd", + Sperhake, Ulrich and Br{\"u}gmann, Bernd", title = "{Reducing eccentricity in black-hole binary evolutions with initial parameters from post-Newtonian inspiral}", journal = "Phys. Rev. D",

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[svn:einsteintoolkit] manifest/trunk/ (Rev. 97)
by schnetter＠cct.lsu.edu 16 Jul '11

16 Jul '11

User: eschnett Date: 2011/07/16 06:35 PM Modified: /trunk/ einsteintoolkit.bib, einsteintoolkit.th Log: Add Goodale 2002. Request citing web site for Cactus and Carpet. File Changes: Directory: /trunk/ ================== File [modified]: einsteintoolkit.bib Delta lines: +23 -5 =================================================================== --- trunk/einsteintoolkit.bib 2011-04-28 18:48:33 UTC (rev 96) +++ trunk/einsteintoolkit.bib 2011-07-16 23:35:30 UTC (rev 97) @@ -407,14 +407,16 @@ ##C ############################################################################ @Misc{Cactuscode:web, - note = {{Cactus} Computational Toolkit}, - url = {http://www.cactuscode.org/}, + requested-for ={Cactus/Cactus}, + note = {{Cactus} Computational Toolkit}, + url = {http://www.cactuscode.org/}, } @Misc{CarpetCode:web, - note = {{Carpet}: Adaptive Mesh Refinement for the {Cactus} - Framework}, - url = {http://www.carpetcode.org/}, + requested-for ={Carpet/Carpet/Cactus}, + note = {{Carpet}: Adaptive Mesh Refinement for the {Cactus} + Framework}, + url = {http://www.carpetcode.org/}, } @Article{Campanelli:2005dd, @@ -610,6 +612,22 @@ url = {http://www.gnu.org/software/gsl/}, } +@InProceedings{Goodale:2002a, + requested-for ={Cactus/Cactus}, + author = {Tom Goodale and Gabrielle Allen and Gerd Lanfermann + and Joan Mass{\'o} and Thomas Radke and Edward + Seidel and John Shalf}, + title = {The {Cactus} Framework and Toolkit: Design and + Applications}, + booktitle = {Vector and Parallel Processing -- VECPAR'2002, 5th + International Conference, Lecture Notes in Computer + Science}, + year = 2003, + address = {Berlin}, + publisher = {Springer}, + url = {http://edoc.mpg.de/3341}, +} + @Article{Gopakumar:2007vh, author = "Gopakumar, Achamveedu and Hannam, Mark and Husa, Sascha and Bruegmann, Bernd", File [modified]: einsteintoolkit.th Delta lines: +77 -2 =================================================================== --- trunk/einsteintoolkit.th 2011-04-28 18:48:33 UTC (rev 96) +++ trunk/einsteintoolkit.th 2011-07-16 23:35:30 UTC (rev 97) @@ -28,7 +28,7 @@ # Simulation Factory !TARGET = $ROOT !TYPE = svn -!URL = https://svn.cct.lsu.edu/repos/numrel/$1/trunk +!URL = https://svn.cct.lsu.edu/repos/numrel/$1/branches/PYSIM_2010 !CHECKOUT = simfactory # Example parameter files @@ -221,11 +221,18 @@ !URL = http://svn.cactuscode.org/projects/$1/$2/trunk !CHECKOUT = ExternalLibraries/BLAS +ExternalLibraries/CGNS +ExternalLibraries/curl +ExternalLibraries/F5 +ExternalLibraries/flickcurl ExternalLibraries/GSL ExternalLibraries/HDF5 +ExternalLibraries/HYPRE ExternalLibraries/LAPACK ExternalLibraries/libjpeg +ExternalLibraries/libxml2 ExternalLibraries/LORENE +#ExternalLibraries/OpenCL ExternalLibraries/OpenSSL #ExternalLibraries/PETSc ExternalLibraries/zlib @@ -244,6 +251,7 @@ AEIThorns/AEILocalInterp AEIThorns/PunctureTracker AEIThorns/SystemStatistics +AEIThorns/TensorTypes @@ -252,8 +260,12 @@ !TYPE = svn !URL = https://svn.cct.lsu.edu/repos/numrel/$1/$2/trunk !CHECKOUT = +LSUDevelopment/Refluxing + +LSUThorns/Flickr LSUThorns/QuasiLocalMeasures LSUThorns/SummationByParts +LSUThorns/Twitter LSUThorns/Vectors @@ -280,6 +292,8 @@ McLachlan/ML_ADMQuantities McLachlan/ML_BSSN McLachlan/ML_BSSN_Helper +McLachlan/ML_BSSN_MP +McLachlan/ML_BSSN_MP_Helper McLachlan/ML_BSSN_O2 McLachlan/ML_BSSN_O2_Helper McLachlan/ML_BSSN_Test @@ -290,7 +304,8 @@ !TARGET = $ARR !TYPE = hg !AUTH_URL = ssh://carpetmercurial@carpetcode.org/carpet -!URL = http://www.carpetcode.org/hg/carpet +!URL = ssh://carpetmercurial@carpetcode.org/carpet +#!URL = http://www.carpetcode.org/hg/carpet # For the git version of Carpet, comment the previous three lines and uncomment # the next three #!TYPE = git @@ -314,9 +329,69 @@ Carpet/CarpetTracker Carpet/LoopControl +CarpetDev/CarpetIOF5 +CarpetDev/CarpetIONirvana +CarpetExtra/AMRToy +CarpetExtra/Nirvana + + +# Llama +!TARGET = $ARR +!TYPE = git +!URL = llama-dev@llamacode.org:Llama +#!URL = login-damiana.aei.mpg.de:/home/ianhin/repositories/Llama +!REPO_PATH= $2 +!CHECKOUT = Llama/ParFiles Llama/README Llama/Thornlists Llama/doc +Llama/ADMDerivatives +Llama/Coordinates +Llama/Gaussian +Llama/GlobalDerivative +Llama/HarmonicDecomposition +Llama/Interpolate +Llama/Interpolate2 +Llama/LlamaHeatToy +Llama/LlamaWaveToy +Llama/MergerHandler +Llama/SphericalSlice +Llama/WaveExtractL +Llama/WorldTube + + + +# CTGamma +!TARGET = $ARR +!TYPE = git +!URL = llama-dev@llamacode.org:CTGamma +!REPO_PATH= $2 +!CHECKOUT = CTGamma/To-Do CTGamma/doc CTGamma/par +CTGamma/CTGBase +CTGamma/CTGConstraints +CTGamma/CTGEvolution +CTGamma/CTGGauge +CTGamma/CTGMatter +CTGamma/CTGRadiativeBC +CTGamma/CartesianCoordinates +CTGamma/Psiclops + + + +# Zelmani +!TARGET = $ARR +!TYPE = git +!URL = carpetgit@stellarcollapse.org:Zelmani.git +!REPO_PATH= $2 +!CHECKOUT = +Zelmani/CoreCollapseControl +Zelmani/ZelmaniHybridCool +Zelmani/ZelmaniStarMapper +Zelmani/ZelmaniLeak + + + # Private thorns !TARGET = $ARR !TYPE = ignore !CHECKOUT = +CarpetExtra/CarpetProlongateTest

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[svn:einsteintoolkit] incoming/ (Rev. 49)
by yosef＠astro.rit.edu 30 Jun '11

30 Jun '11

User: zlochower Date: 2011/06/30 04:31 PM Added: /PITTNullCode/FFTW3/ FFTW3.sh, README, configuration.ccl, interface.ccl, param.ccl, schedule.ccl /PITTNullCode/FFTW3/dist/ fftw-3.2.2.tar.gz /PITTNullCode/FFTW3/src/ make.code.defn Log: A thorn that provides the FFTW3 library. Directory Changes: Directory: /svn:mime-type/ ========================== + application/octet-stream File Changes: Directory: /PITTNullCode/FFTW3/ =============================== File [added]: FFTW3.sh Delta lines: +155 -0 =================================================================== --- PITTNullCode/FFTW3/FFTW3.sh (rev 0) +++ PITTNullCode/FFTW3/FFTW3.sh 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1,155 @@ +#! /bin/bash + +################################################################################ +# Prepare +################################################################################ + +# Set up shell +set -x # Output commands +set -e # Abort on errors + + + +################################################################################ +# Search +################################################################################ + +if [ -z "${FFTW3_DIR}" ]; then + echo "BEGIN MESSAGE" + echo "FFTW3 selected, but FFTW3_DIR not set. Checking some places..." + echo "END MESSAGE" + + FILES="include/fftw3.h" + DIRS="/usr /usr/local /usr/local/fftw3 /usr/local/packages/fftw3 /usr/local/apps/fftw3 ${HOME} c:/packages/fftw3" + for dir in $DIRS; do + FFTW3_DIR="$dir" + for file in $FILES; do + if [ ! -r "$dir/$file" ]; then + unset FFTW3_DIR + break + fi + done + if [ -n "$FFTW3_DIR" ]; then + break + fi + done + + if [ -z "$FFTW3_DIR" ]; then + echo "BEGIN MESSAGE" + echo "FFTW3 not found" + echo "END MESSAGE" + else + echo "BEGIN MESSAGE" + echo "Found FFTW3 in ${FFTW3_DIR}" + echo "END MESSAGE" + fi +fi + + + +################################################################################ +# Build +################################################################################ + +if [ -z "${FFTW3_DIR}" -o "${FFTW3_DIR}" = 'BUILD' ]; then + echo "BEGIN MESSAGE" + echo "Building FFTW3..." + echo "END MESSAGE" + + # Set locations + THORN=FFTW3 + NAME=fftw-3.2.2 + SRCDIR=$(dirname $0) + BUILD_DIR=${SCRATCH_BUILD}/build/${THORN} + INSTALL_DIR=${SCRATCH_BUILD}/external/${THORN} + DONE_FILE=${SCRATCH_BUILD}/done/${THORN} + FFTW3_DIR=${INSTALL_DIR} + +( + exec >&2 # Redirect stdout to stderr + set -x # Output commands + set -e # Abort on errors + cd ${SCRATCH_BUILD} + if [ -e ${DONE_FILE} -a ${DONE_FILE} -nt ${SRCDIR}/dist/${NAME}.tar.gz \ + -a ${DONE_FILE} -nt ${SRCDIR}/FFTW3.sh ] + then + echo "FFTW3: The enclosed FFTW3 library has already been built; doing nothing" + else + echo "FFTW3: Building enclosed FFTW3 library" + + # Should we use gmake or make? + MAKE=$(gmake --help > /dev/null 2>&1 && echo gmake || echo make) + # Should we use gtar or tar? + TAR=$(gtar --help > /dev/null 2> /dev/null && echo gtar || echo tar) + + # Set up environment + unset LIBS + if echo '' ${ARFLAGS} | grep 64 > /dev/null 2>&1; then + export OBJECT_MODE=64 + fi + + echo "FFTW3: Preparing directory structure..." + mkdir build external done 2> /dev/null || true + rm -rf ${BUILD_DIR} ${INSTALL_DIR} + mkdir ${BUILD_DIR} ${INSTALL_DIR} + + echo "FFTW3: Unpacking archive..." + pushd ${BUILD_DIR} + ${TAR} xzf ${SRCDIR}/dist/${NAME}.tar.gz + + echo "FFTW3: Configuring..." + cd ${NAME} + ./configure --prefix=${FFTW3_DIR} + + echo "FFTW3: Building..." + ${MAKE} + + echo "FFTW3: Installing..." + ${MAKE} install + popd + + echo "FFTW3: Cleaning up..." + rm -rf ${BUILD_DIR} + + date > ${DONE_FILE} + echo "FFTW3: Done." + fi +) + + if (( $? )); then + echo 'BEGIN ERROR' + echo 'Error while building FFTW3. Aborting.' + echo 'END ERROR' + exit 1 + fi + +fi + + + +################################################################################ +# Configure Cactus +################################################################################ + +# Set options +if [ "${FFTW3_DIR}" = '/usr' -o "${FFTW3_DIR}" = '/usr/local' ]; then + FFTW3_INC_DIRS='' + FFTW3_LIB_DIRS='' +else + FFTW3_INC_DIRS="${FFTW3_DIR}/include" + FFTW3_LIB_DIRS="${FFTW3_DIR}/lib" +fi +FFTW3_LIBS='fftw3' + +# Pass options to Cactus +echo "BEGIN MAKE_DEFINITION" +echo "HAVE_FFTW3 = 1" +echo "FFTW3_DIR = ${FFTW3_DIR}" +echo "FFTW3_INC_DIRS = ${FFTW3_INC_DIRS}" +echo "FFTW3_LIB_DIRS = ${FFTW3_LIB_DIRS}" +echo "FFTW3_LIBS = ${FFTW3_LIBS}" +echo "END MAKE_DEFINITION" + +echo 'INCLUDE_DIRECTORY $(FFTW3_INC_DIRS)' +echo 'LIBRARY_DIRECTORY $(FFTW3_LIB_DIRS)' +echo 'LIBRARY $(FFTW3_LIBS)' File [added]: README Delta lines: +30 -0 =================================================================== --- PITTNullCode/FFTW3/README (rev 0) +++ PITTNullCode/FFTW3/README 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1,30 @@ +Cactus Code Thorn FFTW3 +Author(s) : +Maintainer(s): +Licence : GPL +-------------------------------------------------------------------------- + +1. Purpose + +Distribute the FFTW Library; see +<http://www.fftw.org> + + + +From the web site: FFTW is a C subroutine library for computing the +discrete Fourier transform (DFT) in one or more dimensions, of +arbitrary input size, and of both real and complex data (as well as of +even/odd data, i.e. the discrete cosine/sine transforms or DCT/DST). +We believe that FFTW, which is free software, should become the FFT +library of choice for most applications. + +Our benchmarks, performed on on a variety of platforms, show that +FFTW's performance is typically superior to that of other publicly +available FFT software, and is even competitive with vendor-tuned +codes. In contrast to vendor-tuned codes, however, FFTW's performance +is portable: the same program will perform well on most architectures +without modification. Hence the name, "FFTW," which stands for the +somewhat whimsical title of "Fastest Fourier Transform in the West." + +The FFTW package was developed at MIT by Matteo Frigo and Steven G. +Johnson File [added]: configuration.ccl Delta lines: +8 -0 =================================================================== --- PITTNullCode/FFTW3/configuration.ccl (rev 0) +++ PITTNullCode/FFTW3/configuration.ccl 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1,8 @@ +# Configuration definitions for thorn FFTW3 + +PROVIDES FFTW3 +{ + SCRIPT FFTW3.sh + LANG bash + OPTIONS FFTW3_DIR FFTW3_LIBS +} File [added]: interface.ccl Delta lines: +3 -0 =================================================================== --- PITTNullCode/FFTW3/interface.ccl (rev 0) +++ PITTNullCode/FFTW3/interface.ccl 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1,3 @@ +# Interface definition for thorn FFTW3 + +IMPLEMENTS: FFTW3 File [added]: param.ccl Delta lines: +1 -0 =================================================================== --- PITTNullCode/FFTW3/param.ccl (rev 0) +++ PITTNullCode/FFTW3/param.ccl 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1 @@ +# Parameter definitions for thorn FFTW3 File [added]: schedule.ccl Delta lines: +1 -0 =================================================================== --- PITTNullCode/FFTW3/schedule.ccl (rev 0) +++ PITTNullCode/FFTW3/schedule.ccl 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1 @@ +# Schedule definitions for thorn FFTW3 Directory: /PITTNullCode/FFTW3/dist/ ==================================== File [added]: fftw-3.2.2.tar.gz Delta lines: +0 -0 =================================================================== (Binary files differ) Property changes on: PITTNullCode/FFTW3/dist/fftw-3.2.2.tar.gz ___________________________________________________________________ Directory: /PITTNullCode/FFTW3/src/ =================================== File [added]: make.code.defn Delta lines: +7 -0 =================================================================== --- PITTNullCode/FFTW3/src/make.code.defn (rev 0) +++ PITTNullCode/FFTW3/src/make.code.defn 2011-06-30 21:31:41 UTC (rev 49) @@ -0,0 +1,7 @@ +# Main make.code.defn file for thorn FFTW3 + +# Source files in this directory +SRCS = + +# Subdirectories containing source files +SUBDIRS =

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[svn:einsteintoolkit] incoming/PITTNullCode/SphericalHarmonicRecon/src/ (Rev. 48)
by yosef＠astro.rit.edu 30 Jun '11

30 Jun '11

User: zlochower Date: 2011/06/30 02:03 PM Added: /PITTNullCode/SphericalHarmonicRecon/src/ make.configuration.defn, make.configuration.deps /PITTNullCode/SphericalHarmonicRecon/src/util/ README, ascii_output.c, dampfilter.c, fftwfilter.c, findlast.c, printtime.c, readmeta.c, setmeta.c, util.c, util.h Log: utilities more CCE File Changes: Directory: /PITTNullCode/SphericalHarmonicRecon/src/ ==================================================== File [added]: make.configuration.defn Delta lines: <Unavailable> File [added]: make.configuration.deps Delta lines: <Unavailable> Directory: /PITTNullCode/SphericalHarmonicRecon/src/util/ ========================================================= File [added]: README Delta lines: <Unavailable> File [added]: ascii_output.c Delta lines: <Unavailable> File [added]: dampfilter.c Delta lines: <Unavailable> File [added]: fftwfilter.c Delta lines: <Unavailable> File [added]: findlast.c Delta lines: <Unavailable> File [added]: printtime.c Delta lines: <Unavailable> File [added]: readmeta.c Delta lines: <Unavailable> File [added]: setmeta.c Delta lines: <Unavailable> File [added]: util.c Delta lines: <Unavailable> File [added]: util.h Delta lines: <Unavailable>

1 0

[svn:einsteintoolkit] incoming/PITTNullCode/ (Rev. 47)
by yosef＠astro.rit.edu 30 Jun '11

30 Jun '11

User: zlochower Date: 2011/06/30 02:02 PM Modified: /PITTNullCode/SphericalHarmonicDecomp/doc/ documentation.tex /PITTNullCode/SphericalHarmonicRecon/doc/ documentation.tex Log: Instructions for use File Changes: Directory: /PITTNullCode/SphericalHarmonicDecomp/doc/ ===================================================== File [modified]: documentation.tex Delta lines: +151 -0 =================================================================== --- PITTNullCode/SphericalHarmonicDecomp/doc/documentation.tex 2011-06-30 15:44:22 UTC (rev 46) +++ PITTNullCode/SphericalHarmonicDecomp/doc/documentation.tex 2011-06-30 19:02:19 UTC (rev 47) @@ -99,6 +99,10 @@ % Add an abstract for this thorn's documentation \begin{abstract} + This thorns provides a mechanism to decompose grid functions in terms +of Spin Weighted spherical harmonics of arbitrary spin. This thorn will +also decompose the ADM metric on spherical shells for use in a subsequent +CCE null evolution. \end{abstract} @@ -106,13 +110,160 @@ % Remove them or add your own. \section{Introduction} + The idea behind this thorn was to decompose GFs on 2D spheres and +3D spherical shells in terms of spin-weighted spherical harmonics +and Chebyshev or Legendre polynomials in radius. This was used for +waveform extraction, compression of 3D data for visualization and CCE. +The code uses more ``collocation'' points than spectral functions. The idea +here was to try to smooth the data by using a least-squares fit to obtain +the spectral coefficients. This thorn provides aliased functions to perform +the decomposition. This will also dump the Cauchy metric. \section{Physical System} \section{Numerical Implementation} \section{Using This Thorn} + \subsection{Dumping Cauchy Data for CCE} + + The following is a section of a parfile appended to an ordinary Cauchy evolution run (see the par/ directory for the complete parfile) +\begin{verbatim} +ActiveThorns="SphericalHarmonicDecomp" + +SphericalHarmonicDecomp::extract_spacetime_metric_every=32 +SphericalHarmonicDecomp::num_radii=3 +SphericalHarmonicDecomp::EM_Rin[0]=18 +SphericalHarmonicDecomp::EM_Rout[0]=22 +SphericalHarmonicDecomp::EM_Rin[1]=47 +SphericalHarmonicDecomp::EM_Rout[1]=53 +SphericalHarmonicDecomp::EM_Rin[2]=94 +SphericalHarmonicDecomp::EM_Rout[2]=106 +SphericalHarmonicDecomp::num_l_modes=7 +SphericalHarmonicDecomp::num_n_modes=7 +SphericalHarmonicDecomp::num_mu_points=41 +SphericalHarmonicDecomp::num_phi_points=82 +SphericalHarmonicDecomp::num_x_points=28 + +\end{verbatim} +In this example we will extract the metric on 3 different shells + (num\_radii), the +first between r=18 and r=22, the second between r=47 and r=53, and +the third between r=94 and 106. The idea here is to make the shell +small enough that we can accurately calculate the radial derivatives +of the metric function, while also large enough that we can smooth out +the grid noise. We decompose the metric functions in terms of +7 $\ell$ modes (num\_l\_modes=7 or all modes from $\ell=0$ to $\ell=6$, + the m modes are automatically set) +and 7 radial modes (num\_n\_mode=7). The grid functions are evaluated +at 41 points in mu (mu=cos(theta)), 82 points in phi, and 28 points +in radius. Minimally, we would need the number of angular points to be +equal to the number of angular spectral functions $\ell^2 + 2\ell$, +in this case we have many more angular modes ($41*82$) than angular +spectral functions. Similarly num\_\x\_points must be greater than +num\_n\_modes. The number of n modes is set by the need to accurately +model the radial derivative of the mertric functions in the spherical +shell. The larger the difference between EM\_Rin[] and EM\_Rout[] the +more points required. The number of l modes is determined by the accuracy +requiremnts of the final CCE waveoform. in this case, choosin +num\_n\_modes=7 is marginally acceptable. + +Note that the parameters +\begin{verbatim} +SphericalHarmonicDecomp::Rin +SphericalHarmonicDecomp::Rout +\end{verbatim} +are not used for CCE metric extraction. These parameters affect the +3D decomposition of GFs using the + + SphericalHarmonicDecomp\_3D\_Decompose aliased function mechanism + + +\subsection{Aliased functions} + SphericalHarmonicDecomp provides a mechanism for other thorns to decompose +GFs either on 2D surfaces or 3D shells via aliased functions. +These two functions should be called in GLOBAL mode. + +\begin{verbatim} +CCTK_INT SphericalHarmonicDecomp_3D_Decompose ( + CCTK_POINTER_TO_CONST _GHp, + CCTK_POINTER_TO_CONST _name, + CCTK_INT re_gindx, + CCTK_INT im_gindx, + CCTK_INT spin ) + +e.g. + + SphericalHarmonicDecomp_3D_Decompose(cctkGH, "Psi4", + CCTK_VarIndex("WeylScal4::Psi4r"), + CCTK_VarIndex("WeylScal4::Psi4i"), -2); + +CCTK_INT FUNCTION sYlm_DecomposeField(\ + CCTK_POINTER_TO_CONST IN cctkGH,\ + CCTK_POINTER_TO_CONST IN name,\ + CCTK_INT IN re_gindx,\ + CCTK_INT IN im_gindx,\ + CCTK_REAL IN radius,\ + CCTK_INT IN spin) + +e.g. + + SphericalHarmonicDecomp_DecomposeField(cctkGH, "Psi4", + CCTK_VarIndex("WeylScal4::Psi4r"), + CCTK_VarIndex("WeylScal4::Psi4i"), 50, -2); + +\end{verbatim} + +\subsection{Parameters} + +\begin{verbatim} +SphericalHarmonicDecomp::extract_spacetime_metric_every how often + (in iterations) should the metric be decomposed and dumped. + +SphericalHarmonicDecomp::out_dir="" Output directory for all output, + usually set to "", which causes the + thorn to use IO::out_dir + +SphericalHarmonicDecomp::max_spin=2 Largest spin value. For most configuration + this should be set to 2. + +SphericalHarmonicDecomp::num_l_modes How many l modes. This affects all + output. Note this is not lmax-1 in general. + For spin-weight 2 GF, lmax will be num_l_modes+2-1 + +SphericalHarmonicDecomp::num_mu_points number of points in the mu (cos(theta)) + direction. Affects all output. + +SphericalHarmonicDecomp::num_phi_points number of points in phi direction. + Affects all output. + +SphericalHarmonicDecomp::num_x_points number of points in x (radial) direction. + Affects all 3D output including MetricDecomp + +SphericalHarmonicDecomp::Rin inner radius of 3D shell. Only affects fields + dumped using aliased function mechanism + +SphericalHarmonicDecomp::Rout outer radius of 3D shell. Only affects fields + dumped using aliased function mechanism + +SphericalHarmonicDecomp::EM_Rin an array of Rins used for the CCE Metric + extraction + +SphericalHarmonicDecomp::EM_Rout an array of Routs used for the CCE Metric + extraction + +SphericalHarmonicDecomp::output_m_max limit on the maximum abs(m) dumped to + output. These options are useful if you don't want to + dump all the m modes from -l to l. + +SphericalHarmonicDecomp::output_l_max limit on the maximum l dumped to + output. This option is useful if you want the maximum + l dumped to output to be independent of the spin of the + GF. +\end{verbatim} + + + \subsection{Obtaining This Thorn} \subsection{Basic Usage} Directory: /PITTNullCode/SphericalHarmonicRecon/doc/ ==================================================== File [modified]: documentation.tex Delta lines: +167 -1 =================================================================== --- PITTNullCode/SphericalHarmonicRecon/doc/documentation.tex 2011-06-30 15:44:22 UTC (rev 46) +++ PITTNullCode/SphericalHarmonicRecon/doc/documentation.tex 2011-06-30 19:02:19 UTC (rev 47) @@ -99,14 +99,180 @@ % Add an abstract for this thorn's documentation \begin{abstract} - +This thorn is used to reconstruct the metric data saved by +SphericalHarmonicDecomp. It also provides aliased functions +that are used by NullSHRExtract to construct the boundary data +for CCE. \end{abstract} % The following sections are suggestive only. % Remove them or add your own. \section{Introduction} + +\section{Using and Filtering Cauchy data from SphericalHarmonicDecomp} +The thorn SphericalHarmonicDecomp uses a least-squares fit of the metric +data in some spherical shell to a set of spectral functions (Chebyshev in +R and Ylm in angle). These data are dumped into files with names +metric\_obs\_0\_Decomp.h5, metric\_obs\_1\_Decomp.h5, etc., where +the 0,1,etc. refer to the spherical shell (several are allowed). +This thorn takes the data in one of these files and passes it to +NullSHRExtract, which uses them to construct the null boundary data. +Several utilities are provided in order to view and modify these data +files. These include a program to filter the data via an FFT and +calculate a smooth time derivative, which may be important in order +to obtain accurate waveforms. + +These utilities require the HDF5 and FFTW3 libraries and are +compiled using the gamke CONFIGNAME-utils mechanism. + +To filter the Cauchy data: + + In general a simulation will be run over multiple jobs, each one +producing an individual metric\_decomp.h5 file. You will need to +combine these files using hdf5\_merge. + +\begin{verbatim} +For example + hdf5\_merge Run1/metric_obs\_0\_Decomp.h5 \ + Run2/metric\_obs\_0\_Decomp.h5 \ + metric\_obs\_0\_Decomp.h5 +\end{verbatim} + +Once the files are merged, you will need to find the last timestep +using the "findlast" command + +\begin{verbatim} +./findlast metric\_obs\_0\_Decomp.h5 + 8086: 4.010913e+02 +\end{verbatim} + +Here 8086 is the last timestep, which corresponds to a time of 401.0913. + +Next it is a good idea to examine the data in one of the higher modes +you will use. In this case we will examine the n=1, l=4,m=4 mode +of gxx (the 0 below corresponds to gxx, see the source) + +\begin{verbatim} +./ascii\_output 8086 1 4 4 0 metric\_obs\_0\_Decomp.h5 > test\_out +\end{verbatim} + +We will use this data to ensure that only high-frequency junk is +filtered. In this case it was found that the true signal frequency +is smaller than 0.5 (omega). To be safe, we'll set the maximum +allowed frequency to 2. + +\begin{verbatim} +./fftwfilter 8086 2 1 metric\_obs\_0\_Decomp.h5 +\end{verbatim} + +Here the "2" corresponds to the maximum frequency, while the "1" +corresponds to the damping length. Note that the maximum frequency is +in units of 2*pi/(physical time), while the damping length is units of +integer frequency. Choosing a large damping length can lead to suppression +of the true signal. + +The output file is metric\_obs\_0\_Decomp\_ft.h5, which contains the +filtered metric data and the time derivatives of these data (which the +original file did not contain). The filtered data can now be used in a +Characteristic evolution. + +In order to use the Cauchy extraction data in a subsequent Characteristic +evolution, you need to know the timestep in the Cauchy data and +the region in radius that the data cover. The program "readmeta" will +give you this region. + +\begin{verbatim} +./readmeta metric\_obs\_0\_Decomp\_ft.h5 +Run Parameters +... nn = 7 +... na = 49 +... Rin = 1.800000e+01 +... Rout = 2.200000e+01 +\end{verbatim} + +Here we see that the data covers the interval 18<r<22. In this case, +we would choose an extraction radius of 20 and set the following +parameters in the parfile + +\begin{verbatim} + #Extraction radius--------------- + SphericalHarmonicRecon::r\_extract=20.0 + NullSHRExtract::cr = 20.0 + NullGrid::null\_rwt = 20.0 + + SphericalHarmonicRecon::time\_derivative\_in\_file = "yes" + SphericalHarmonicRecon::metric\_data\_filename = "metric\_obs\_0\_Decomp\_ft.h5" +\end{verbatim} + +Choosing a timestep for the characteristic evolution that is an integer +multiple of the Cauchy dump times will remove time interpolation +errors and can lead to smoother signals. To find these dump time, +use the "printtime" command. The syntax is "printtime iteration file" + +\begin{verbatim} +./printtime 1 metric\_obs\_0\_Decomp\_ft.h5 +1: 4.960317e-02 +\end{verbatim} + +In this case the dump times are separated by 0.04960317. + +For complete example parfiles for both the initial Cauchy evolution, +and subsequent null evolution, see SphericalHarmonicDecomp/par/ +and SphericalHarmonicRecon/par/ + +\subsection{Parameters} + +\begin{verbatim} +SphericalHarmonicRecon::order order used in time interpolation / + differentiation. Options are 2 or 4. + +SphericalHarmonicRecon::r_extract the radius of the worldtube. This + must be consistent with the setup of the null grid + +SphericalHarmonicRecon::metric_data_filename filename for the cauchy + metric data + +SphericalHarmonicRecon::time_derivative_in_file flag that indicates if + the time derivative of the metric is in the cauchy file. The + time derivative may be generated via the fftwfilter program mentioned + above. + +# the following parameters should only be used if the +# hdf5 was corrupted and extraction parameters +# are not recoverable. Of course, we should actually +# fix the extraction code so that this does not happen +BOOLEAN override_extraction_parameters "never set this" +{ +} no + +CCTK_INT override_spin "spin: never set this" +{ + *:* :: "anything, but you probably want 0" +} 0 + +CCTK_INT override_nn "number of Chabyshev coefficients: never use this" +{ + 1:* :: "positive: must actualy match the extraction run" +} 1 + +CCTK_INT override_na "number of angular coefficients: never use this" +{ + 1:* :: "positive: must actualy match the extraction run" +} 1 + +CCTK_REAL override_Rin "inner radius of extraction zone: ..." +{ + (0:* :: "positive" +} 1 + +CCTK_REAL override_Rout "outer radius of extraction zone: ..." +{ + (0:* :: "positive" +} 1 +\end{verbatim} + \section{Physical System} \section{Numerical Implementation}

1 0

[svn:einsteintoolkit] incoming/PITTNullCode/ (Rev. 46)
by yosef＠astro.rit.edu 30 Jun '11

30 Jun '11

User: zlochower Date: 2011/06/30 10:44 AM Added: /PITTNullCode/ COPYING, GPLv2 Modified: /PITTNullCode/ README Log: license for code File Changes: Directory: /PITTNullCode/ ========================= File [added]: COPYING Delta lines: +42 -0 =================================================================== --- PITTNullCode/COPYING (rev 0) +++ PITTNullCode/COPYING 2011-06-30 15:44:22 UTC (rev 46) @@ -0,0 +1,42 @@ +This code is available under the GPL General Public License, +version 2, or later (see GPLv2 file included). + +The code in this arrangement is a results of many years of work by +many different authors. Major contributors to this code include +(in alphabetical order) + +M.C. Babiuc +N. T. Bishop +R. Gomez +R. A. Isaacson +L. Lehner +P. Papadopoulos +C. Reisswig +B. Szilagyi +J. Welling +J. Winicour +Y. Zlochower + + +If you use this code, then we request that you cite the following papers: + +Title: Characteristic Extraction Tool for Gravitational Waveforms + Authors: M.C. Babiuc, B. Szilagyi, J. Winicour, Y. Zlochower + arXiv:1011.4223 + submitted to Physical Review D + +Title: Cauchy-characteristic matching + Authors: N. Bishop, R. Isaacson, R. Gomez, L. Lehner, B. Szilagyi, J. + Winicour arXiv: gr-qc/9801070 + In "Black Holes, Gravitational Radiation and the Universe" + eds. B. Iyer and B. Bhawal (Kluwer, Dordrecht, Boston,1999) + +This code is maintained by + +M. C.Babiuc <babiuc(a)marshall.edu> +B. Szilagyi <bela(a)caltech.edu> +C. Reisswig <reisswig(a)tapir.caltech.edu> +Y. Zlochower <yosef(a)astro.rit.edu> + +Please contact the maintainers of the code if you require +write access. 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Of course, the commands you use may +be called something other than `show w' and `show c'; they could even be +mouse-clicks or menu items--whatever suits your program. + +You should also get your employer (if you work as a programmer) or your +school, if any, to sign a "copyright disclaimer" for the program, if +necessary. Here is a sample; alter the names: + + Yoyodyne, Inc., hereby disclaims all copyright interest in the program + `Gnomovision' (which makes passes at compilers) written by James Hacker. + + <signature of Ty Coon>, 1 April 1989 + Ty Coon, President of Vice + +This General Public License does not permit incorporating your program into +proprietary programs. If your program is a subroutine library, you may +consider it more useful to permit linking proprietary applications with the +library. If this is what you want to do, use the GNU Lesser General +Public License instead of this License. File [modified]: README Delta lines: +10 -10 =================================================================== --- PITTNullCode/README 2011-06-30 15:43:02 UTC (rev 45) +++ PITTNullCode/README 2011-06-30 15:44:22 UTC (rev 46) @@ -1,4 +1,5 @@ -This code is available under the XXXX license (see license file included). +This code is available under the GPL General Public License, +version 2, or later (see GPLv2 file included). The code in this arrangement is a results of many years of work by many different authors. Major contributors to this code include @@ -10,8 +11,8 @@ R. A. Isaacson L. Lehner P. Papadopoulos +C. Reisswig B. Szilagyi -C. Reisswig J. Welling J. Winicour Y. Zlochower @@ -20,17 +21,16 @@ If you use this code, then we request that you cite the following papers: Title: Characteristic Extraction Tool for Gravitational Waveforms -Authors: M.C. Babiuc, B. Szilagyi, J. Winicour, Y. Zlochower -arXiv:1011.4223 -submitted to Physical Review D + Authors: M.C. Babiuc, B. Szilagyi, J. Winicour, Y. Zlochower + arXiv:1011.4223 + submitted to Physical Review D Title: Cauchy-characteristic matching -Authors: N. Bishop, R. Isaacson, R. Gomez, L. Lehner, B. Szilagyi, J. Winicour -arXiv: gr-qc/9801070 -Appeared in "On the Black Hole Trail" -eds. Bala Iyer and Biplab Bhawal (Kluwer) + Authors: N. Bishop, R. Isaacson, R. Gomez, L. Lehner, B. Szilagyi, J. + Winicour arXiv: gr-qc/9801070 + In "Black Holes, Gravitational Radiation and the Universe" + eds. B. Iyer and B. Bhawal (Kluwer, Dordrecht, Boston,1999) - This code is maintained by M. C.Babiuc <babiuc(a)marshall.edu>

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