! $Id$ ! ! MODULE_DOC: Runge-Kutta time advance, accurate to order itorder. ! MODULE_DOC: At the moment, itorder can be 1, 2, or 3. ! module Timestep ! use Cparam use Cdata ! implicit none ! private ! include 'timestep.h' ! contains !*********************************************************************** subroutine initialize_timestep ! ! Coefficients for up to order 3. ! 26-oct-21/wlyra: added 2N-RK4 coefficients. The coefficients are for ! for 4th order, but use 5 stages. Since itorder is used ! in the code for the number of stages, it should be 5 ! to use it. ! use Messages, only: fatal_error use General, only: itoa ! if (itorder==1) then alpha_ts=(/ 0.0, 0.0, 0.0, 0.0, 0.0 /) beta_ts =(/ 1.0, 0.0, 0.0, 0.0, 0.0 /) elseif (itorder==2) then alpha_ts=(/ 0.0, -1/2.0, 0.0, 0.0, 0.0 /) beta_ts =(/ 1/2.0, 1.0, 0.0, 0.0, 0.0 /) elseif (itorder==3) then !alpha_ts=(/ 0.0, -2/3.0, -1.0 /) !beta_ts =(/ 1/3.0, 1.0, 1/2.0 /) ! use coefficients of Williamson (1980) alpha_ts=(/ 0.0, -5/9.0 , -153/128.0, 0.0, 0.0 /) beta_ts =(/ 1/3.0, 15/16.0, 8/15.0 , 0.0, 0.0 /) elseif (itorder==5) then ! coefficients of Carpenter & Kennedy (1994) ! https://ntrs.nasa.gov/api/citations/19940028444/downloads/19940028444.pdf alpha_ts=(/0.0,-567301805773./1357537059087.,& -2404267990393./2016746695238.,& -3550918686646./2091501179385.,& -1275806237668./842570457699./) beta_ts=(/1432997174477./9575080441755.,& 5161836677717./13612068292357.,& 1720146321549./2090206949498.,& 3134564353537./4481467310338.,& 2277821191437./14882151754819./) ! !alpha_ts=(/0.0,-0.4812317431372,-1.049562606709,-1.602529574275,-1.778267193916/) !beta_ts =(/9.7618354692056e-2,0.4122532929155,0.4402169639311,1.426311463224,0.1978760537318/) else call fatal_error('initialize_timestep','Not implemented: itorder= '// & trim(itoa(itorder))) endif endsubroutine initialize_timestep !*********************************************************************** subroutine time_step(f,df,p) ! ! 2-apr-01/axel: coded ! 14-sep-01/axel: moved itorder to cdata ! use Boundcond, only: update_ghosts use BorderProfiles, only: border_quenching use Equ, only: pde, impose_floors_ceilings use Mpicomm, only: mpiallreduce_max,MPI_COMM_WORLD use Particles_main, only: particles_timestep_first, & particles_timestep_second use PointMasses, only: pointmasses_timestep_first, & pointmasses_timestep_second use Solid_Cells, only: solid_cells_timestep_first, & solid_cells_timestep_second use Shear, only: advance_shear use Sub, only: set_dt, shift_dt ! real, dimension (mx,my,mz,mfarray) :: f real, dimension (mx,my,mz,mvar) :: df type (pencil_case) :: p real :: ds, dtsub ! ! dt_beta_ts may be needed in other modules (like Dustdensity) for fixed dt. ! ! <<<<<<<<<<<<<< the following should be omitted at some point <<<<<<<<<<<<<< ! There is also an option to advance the time in progressively smaller ! fractions of the current time. This is used to model the end of inflation, ! when lfractional_tstep_negative should be used. ! If dt=.5 and tstart=20, then one has -20, -10, -5, -2.5, etc. ! From radiation era onward, lfractional_tstep_positive should be used ! to make sure the dt used in run.in is positive. ! if (.not. ldt) then ! if (lfractional_tstep_advance) then ! if (lfractional_tstep_negative) then ! dt_beta_ts=-dt*t ! else ! dt_beta_ts=dt*t ! endif ! else dt_beta_ts=dt*beta_ts ! endif endif ! >>>>>>>>>>>>>>>>>>>> until here >>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> ! ! Set up df and ds for each time sub. ! do itsub=1,itorder lfirst=(itsub==1) llast=(itsub==itorder) if (lfirst) then if (.not.lgpu) df=0.0 ds=0.0 else if (.not.lgpu) df=alpha_ts(itsub)*df !(could be subsumed into pde, but is dangerous!) ds=alpha_ts(itsub)*ds if (it_rmv>0) lrmv=.false. endif ! ! Set up particle derivative array. ! if (lparticles) call particles_timestep_first(f) ! ! Set up point masses derivative array ! if (lpointmasses) call pointmasses_timestep_first(f) ! ! Set up solid_cells time advance ! if (lsolid_cells) call solid_cells_timestep_first(f) ! ! Change df according to the chosen physics modules. ! call pde(f,df,p) ds=ds+1.0 ! ! If we are in the first time substep we need to calculate timestep dt. ! Takes minimum over and distributes to all processors. ! With GPUs this is done on the CUDA side. ! if (lfirst.and.ldt.and..not.lgpu) call set_dt(maxval(dt1_max)) ! ! Calculate dt_beta_ts. ! if (ldt) dt_beta_ts=dt*beta_ts if (ip<=6) print*, 'time_step: iproc, dt=', iproc_world, dt !(all have same dt?) dtsub = ds * dt_beta_ts(itsub) ! ! Apply border quenching. ! if (lborder_profiles) call border_quenching(f,df,dt_beta_ts(itsub)) ! ! Time evolution of grid variables. ! if (.not. lgpu) f(l1:l2,m1:m2,n1:n2,1:mvar) = f(l1:l2,m1:m2,n1:n2,1:mvar) & + dt_beta_ts(itsub)*df(l1:l2,m1:m2,n1:n2,1:mvar) ! ! Time evolution of point masses. ! if (lpointmasses) call pointmasses_timestep_second(f) ! ! Time evolution of particle variables. ! if (lparticles) call particles_timestep_second(f) ! ! Time evolution of solid_cells. ! if (lsolid_cells) call solid_cells_timestep_second(f,dt_beta_ts(itsub),ds) ! ! Advance deltay of the shear (and, optionally, perform shear advection ! by shifting all variables and their derivatives). ! if (lshear) then call impose_floors_ceilings(f) call update_ghosts(f) ! Necessary for non-FFT advection but unnecessarily overloading FFT advection call advance_shear(f, df, dtsub) endif ! call update_after_substep(f,df,dtsub,llast) ! ! Increase time. ! t = t + dtsub ! enddo ! substep loop ! ! Integrate operator split terms. ! call split_update(f) ! endsubroutine time_step !*********************************************************************** subroutine split_update(f) ! ! Integrate operator split terms. ! ! 14-dec-14/ccyang: coded ! use Density, only: split_update_density use Energy, only: split_update_energy use Magnetic, only: split_update_magnetic use Viscosity, only: split_update_viscosity use Particles_main, only: split_update_particles ! real, dimension(mx,my,mz,mfarray), intent(inout) :: f ! ! Dispatch to respective modules. ! if (ldensity) call split_update_density(f) if (lenergy) call split_update_energy(f) if (lmagnetic) call split_update_magnetic(f) if (lviscosity) call split_update_viscosity(f) ! if (lparticles) call split_update_particles(f, dt) ! endsubroutine split_update !*********************************************************************** subroutine update_after_substep(f,df,dtsub,llast) ! ! Hooks for modifying f and df after the timestep is performed. ! ! 12-03-17/wlyra: coded ! 28-03-17/MR: removed update_ghosts; checks for already communicated variables enabled. ! use Density, only: density_after_timestep use Hydro, only: hydro_after_timestep use Energy, only: energy_after_timestep use Magnetic, only: magnetic_after_timestep use Special, only: special_after_timestep use Particles_main, only: particles_special_after_dtsub ! logical, intent(in) :: llast real, dimension (mx,my,mz,mfarray) :: f real, dimension (mx,my,mz,mvar) :: df real :: dtsub ! ! Enables checks to avoid unnecessary communication ! ighosts_updated=0 ! ! Dispatch to respective modules. The module which communicates ! the biggest number of variables should come first here. ! if (lhydro) call hydro_after_timestep (f,df,dtsub) if (lmagnetic) call magnetic_after_timestep(f,df,dtsub) if (lenergy) call energy_after_timestep (f,df,dtsub) if (ldensity) call density_after_timestep (f,df,dtsub) if (lspecial) then call special_after_timestep(f, df, dtsub, llast) if (lparticles) call particles_special_after_dtsub(f, dtsub) endif ! ! Disables checks. ! ighosts_updated=-1 ! endsubroutine update_after_substep !*********************************************************************** subroutine pushpars2c(p_par) use Syscalls, only: copy_addr integer, parameter :: n_pars=2 integer(KIND=ikind8), dimension(n_pars) :: p_par call copy_addr(alpha_ts,p_par(1)) ! (3) call copy_addr(beta_ts ,p_par(2)) ! (3) endsubroutine pushpars2c !*********************************************************************** endmodule Timestep