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amun-code/src/evolution.F90

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Update the copyright info and fix the length of separating lines.
2010-10-13 03:32:10 -03:00
!!******************************************************************************
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!!
!! module: evolution - handling the time evolution of the block structure
!!
Update the copyright info and fix the length of separating lines.
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!! Copyright (C) 2008-2010 Grzegorz Kowal <grzegorz@gkowal.info>
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!!
Update the copyright info and fix the length of separating lines.
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!!******************************************************************************
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!!
!! This file is part of Godunov-AMR.
!!
!! Godunov-AMR is free software; you can redistribute it and/or modify
!! it under the terms of the GNU General Public License as published by
!! the Free Software Foundation; either version 3 of the License, or
!! (at your option) any later version.
!!
!! Godunov-AMR is distributed in the hope that it will be useful,
!! but WITHOUT ANY WARRANTY; without even the implied warranty of
!! MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
!! GNU General Public License for more details.
!!
!! You should have received a copy of the GNU General Public License
!! along with this program. If not, see <http://www.gnu.org/licenses/>.
!!
Update the copyright info and fix the length of separating lines.
2010-10-13 03:32:10 -03:00
!!******************************************************************************
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!!
!
module evolution
implicit none
integer, save :: n
SCHEME: move cmax parameter from module 'evolution' to 'scheme'.
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real , save :: t, dt, dtn
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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contains
!
Updated comments in the evolution module.
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!===============================================================================
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
Updated comments in the evolution module.
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! evolve: subroutine sweeps over all leaf blocks and performs one step time
! evolution for each according to the selected integration scheme
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
Updated comments in the evolution module.
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!===============================================================================
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
EVOLUTION: remove unused subroutines. - remove subroutine advance(); this subroutine is good for GALERKIN approach; it's gonna be reintroduced during this method implementation; - remove subroutine update_flux(); this subroutine is called from advance() and is not used in the GLM-MHD approach; - make GNU Fortran happy bu adding () to the subroutine calls;
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subroutine evolve()
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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EVOLUTION: evolve the forcing source terms. - call subroutine evolve_forcing() before the update of all blocks; this subroutine evolves the forcing source terms by an interval dt in the Fourier space; then during the update the forcing Fourier coefficients will be transformed to real space for each block separately;
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use blocks , only : block_data, list_data
use boundaries, only : boundary_variables
#ifdef FORCE
use forcing , only : evolve_forcing
#endif /* FORCE */
use mesh , only : update_mesh
use mesh , only : dx_min
use scheme , only : cmax
use timer , only : start_timer, stop_timer
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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implicit none
! local variables
!
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
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type(block_data), pointer :: pblock
EVOLUTION: add subroutine to update the maximum speed. - make the variable cmax global in the module 'evolution'; - add a new subroutine update_maximum_speed() which updates the maximum speed cmax in the system iterating over all data blocks; - use the subroutine update_maximum_speed() in evolve();
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real :: cm
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
Updated comments in the evolution module.
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!-------------------------------------------------------------------------------
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
EVOLUTION: evolve the forcing source terms. - call subroutine evolve_forcing() before the update of all blocks; this subroutine evolves the forcing source terms by an interval dt in the Fourier space; then during the update the forcing Fourier coefficients will be transformed to real space for each block separately;
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#ifdef FORCE
! evolve the forcing source terms by the time interval dt
!
call evolve_forcing(dt)
#endif /* FORCE */
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
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! iterate over all data blocks and perform one step of time evolution
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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!
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
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pblock => list_data
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
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do while (associated(pblock))
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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! check if this block is a leaf
!
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
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if (pblock%meta%leaf) &
New time integration method EULER.
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#ifdef EULER
call evolve_euler(pblock)
#endif /* EULER */
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
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#ifdef RK2
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
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call evolve_rk2(pblock)
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
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#endif /* RK2 */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
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#ifdef RK3
call evolve_rk3(pblock)
#endif /* RK3 */
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
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! assign pointer to the next block
!
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
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pblock => pblock%next
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
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end do
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
New module to handle the boundary conditions. The subroutine 'boundary' sweeps over all leaf blocks. For each block it sweeps over its neighbors and performs update of the boundaries. This is an initial version yet, it supports only neighboring blocks of the same level of refinement.
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! update boundaries
Store all variables in one array U. One array U, which is a field in the BLOCK structure, stores all variables. The number of variables is determined by the nvars parameter. To access each variable we use variable index now, like idn, imx, imy, mz, ien, etc.
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!
Refinement based on density. More cleanups.
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call start_timer(4)
EVOLUTION: remove unused subroutines. - remove subroutine advance(); this subroutine is good for GALERKIN approach; it's gonna be reintroduced during this method implementation; - remove subroutine update_flux(); this subroutine is called from advance() and is not used in the GLM-MHD approach; - make GNU Fortran happy bu adding () to the subroutine calls;
2010-12-01 15:14:07 -02:00
call boundary_variables()
Refinement based on density. More cleanups.
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call stop_timer(4)
Store all variables in one array U. One array U, which is a field in the BLOCK structure, stores all variables. The number of variables is determined by the nvars parameter. To access each variable we use variable index now, like idn, imx, imy, mz, ien, etc.
2008-12-08 12:14:13 -06:00
Use TVD interpolation in boundary update, update mesh before time step. BOUNDARY CONDITIONS - use TVD interpolation for prolongation of the boundary conditions CONFIGURATION - put lower limit for the number of ghost and domain cells HOST FILES - host files should not be included in the revision control INTERPOLATION - define all arrays as REAL, not REAL(KIND=8) since the precision of calculations is determined at the compilation stage - replace j0 and j1 indices with new more obvious il and ir MESH - update mesh before calculating new time step
2010-03-14 15:40:24 -03:00
! check refinement and refine
!
call start_timer(5)
EVOLUTION: remove unused subroutines. - remove subroutine advance(); this subroutine is good for GALERKIN approach; it's gonna be reintroduced during this method implementation; - remove subroutine update_flux(); this subroutine is called from advance() and is not used in the GLM-MHD approach; - make GNU Fortran happy bu adding () to the subroutine calls;
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call update_mesh()
Use TVD interpolation in boundary update, update mesh before time step. BOUNDARY CONDITIONS - use TVD interpolation for prolongation of the boundary conditions CONFIGURATION - put lower limit for the number of ghost and domain cells HOST FILES - host files should not be included in the revision control INTERPOLATION - define all arrays as REAL, not REAL(KIND=8) since the precision of calculations is determined at the compilation stage - replace j0 and j1 indices with new more obvious il and ir MESH - update mesh before calculating new time step
2010-03-14 15:40:24 -03:00
call stop_timer(5)
! update boundaries
!
call start_timer(4)
EVOLUTION: remove unused subroutines. - remove subroutine advance(); this subroutine is good for GALERKIN approach; it's gonna be reintroduced during this method implementation; - remove subroutine update_flux(); this subroutine is called from advance() and is not used in the GLM-MHD approach; - make GNU Fortran happy bu adding () to the subroutine calls;
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call boundary_variables()
Use TVD interpolation in boundary update, update mesh before time step. BOUNDARY CONDITIONS - use TVD interpolation for prolongation of the boundary conditions CONFIGURATION - put lower limit for the number of ghost and domain cells HOST FILES - host files should not be included in the revision control INTERPOLATION - define all arrays as REAL, not REAL(KIND=8) since the precision of calculations is determined at the compilation stage - replace j0 and j1 indices with new more obvious il and ir MESH - update mesh before calculating new time step
2010-03-14 15:40:24 -03:00
call stop_timer(4)
EVOLUTION: add subroutine to update the maximum speed. - make the variable cmax global in the module 'evolution'; - add a new subroutine update_maximum_speed() which updates the maximum speed cmax in the system iterating over all data blocks; - use the subroutine update_maximum_speed() in evolve();
2010-12-01 10:39:18 -02:00
! update the maximum speed
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
2008-12-09 14:51:33 -06:00
!
EVOLUTION: add subroutine to update the maximum speed. - make the variable cmax global in the module 'evolution'; - add a new subroutine update_maximum_speed() which updates the maximum speed cmax in the system iterating over all data blocks; - use the subroutine update_maximum_speed() in evolve();
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call update_maximum_speed()
! get maximum time step
!
dtn = dx_min / max(cmax, 1.0d-16)
!
!-------------------------------------------------------------------------------
!
end subroutine evolve
!
!===============================================================================
!
! update_maximum_speed: subroutine updates module variable cmax with the value
! corresponding to the maximum speed in the system
!
!===============================================================================
!
subroutine update_maximum_speed()
EVOLUTION: reduce cmax instead of dt. - now we reduce the maximum speed over all processors instead of the time step;
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use blocks , only : block_data, list_data
#ifdef MPI
use mpitools, only : mallreducemaxr
#endif /* MPI */
use scheme , only : maxspeed, cmax
EVOLUTION: add subroutine to update the maximum speed. - make the variable cmax global in the module 'evolution'; - add a new subroutine update_maximum_speed() which updates the maximum speed cmax in the system iterating over all data blocks; - use the subroutine update_maximum_speed() in evolve();
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implicit none
! local variables
!
type(block_data), pointer :: pblock
real :: cm
!
!-------------------------------------------------------------------------------
!
! reset the maximum speed
!
cmax = 1.0d-16
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
2008-12-09 14:51:33 -06:00
! iterate over all blocks in order to find the maximum speed
!
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
2009-09-14 18:28:17 -03:00
pblock => list_data
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
2008-12-09 14:51:33 -06:00
do while (associated(pblock))
! check if this block is a leaf
!
Evolve new list of data blocks. TIME INTEGRATION - now update the solution using new list of data blocks belonging to the current process only
2009-09-14 18:28:17 -03:00
if (pblock%meta%leaf) &
Added CFL condition and calculation of the new time step. The function to calculate the maximum speed in the block has been added. This function is used to determine the maximum speed globally, which is next used to estimate the next time step.
2008-12-09 14:51:33 -06:00
cm = maxspeed(pblock%u)
! compare global and local maximum speeds
!
cmax = max(cmax, cm)
! assign pointer to the next block
!
pblock => pblock%next
end do
EVOLUTION: reduce cmax instead of dt. - now we reduce the maximum speed over all processors instead of the time step;
2010-12-03 18:02:07 -02:00
#ifdef MPI
! reduce the maximum speed over all processes
!
call mallreducemaxr(cmax)
#endif /* MPI */
Implement FLUXCT integration of the induction equation. SCHEME - implement Flux-CT scheme for the staggered magnetic field integration; BLOCK STRUCTURE - use more space efficient storage of the variables, which means storing only staggered components of magnetic field; cell-centered components are calculated only when necessary; EVOLUTION - remove loops in the field updates; operations are performed on the arrays; BOUNDARY CONDITIONS - remove loops in the bnd_copy; operations are calculated on the whole array now; INTERPOLATION - subroutine magtocen() has been rewritten to avoid problems with the array allocation; now as an argument we enter the array of all variables; subroutine uses indices for the face-centered and cell-centered magnetic field components internally; MAKE - add flag defining Flux-CT scheme; PROBLEM - use predefined array variables instead of allocated;
2010-02-28 18:35:57 -03:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!-------------------------------------------------------------------------------
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
EVOLUTION: add subroutine to update the maximum speed. - make the variable cmax global in the module 'evolution'; - add a new subroutine update_maximum_speed() which updates the maximum speed cmax in the system iterating over all data blocks; - use the subroutine update_maximum_speed() in evolve();
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end subroutine update_maximum_speed
New time integration method EULER.
2008-12-09 21:06:21 -06:00
#ifdef EULER
!
!===============================================================================
!
! evolve_euler: subroutine evolves the current block using Euler integration
!
!===============================================================================
!
subroutine evolve_euler(pblock)
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
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use blocks , only : block_data
use config , only : im, jm, km
EVOLUTION: add forcing terms in the block update.
2010-12-08 21:48:43 -02:00
#ifdef FORCE
use forcing , only : real_forcing
#endif /* FORCE */
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
use mesh , only : adxi, adyi, adzi
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#ifdef SHAPE
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
2010-12-01 09:25:30 -02:00
use problem , only : update_shapes
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#endif /* SHAPE */
SCHEME: move cmax parameter from module 'evolution' to 'scheme'.
2010-12-01 13:13:27 -02:00
use scheme , only : update, cmax
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
2010-12-01 09:25:30 -02:00
use variables, only : nqt, nfl
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#ifdef MHD
use variables, only : ibx, ibz
#ifdef GLM
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
use config , only : alpha_p
use mesh , only : dx_min
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
use variables, only : iph
#endif /* GLM */
#endif /* MHD */
EVOLUTION: add forcing terms in the block update.
2010-12-08 21:48:43 -02:00
#ifdef FORCE
use variables, only : idn, imx, imy, imz
#endif /* FORCE */
New time integration method EULER.
2008-12-09 21:06:21 -06:00
implicit none
! input arguments
!
Initial support for the MHD equations. VARIABLES - add indices for the magnetic field components, both face and cell centered SOLVER, MHD - add support for the magnetohydrodynamic (MHD) equations to the subroutines cons2prim(), prim2cons() - add MHD flux and the fastest speed calculation in the subroutine fluxspeed() - include magnetosonic speed in the calculation of the maximum speed in the system required for estimation of the new time step - extend the HLL solver in subroutine hll() to support MHD - calculate the magnetic field update according to a CT scheme in the subroutine update() INTERPOLATION - add subroutine magtocen() to interpolate cell centered magnetic field EVOLUTION - add evolution of the magnetic field components in the evolve_euler() and evolve_rk2() time integration subroutines - also call the subroutine magtocen() in the right places BOUNDARY CONDITIONS - support for magnetic field boundary update only in the case of blocks with the same level so far; later we need to include proper restriction and prolongation for the magnetic field to keep its divergence equal zero PROBLEMS, BLAST - extend the blast problem to include the initial magnetic field IO, HDF5 - write down in a HDF5 file magnetic field components
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type(block_data), intent(inout) :: pblock
New time integration method EULER.
2008-12-09 21:06:21 -06:00
! local variables
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: dxi, dyi, dzi, ch2
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
#if defined MHD && defined GLM
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: decay
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
#endif /* MHD & GLM */
New time integration method EULER.
2008-12-09 21:06:21 -06:00
! local arrays
!
Remove flux calculation from the subroutine update(). SCHEME - remove the flux calculation from the subroutine update() and all dependent subroutines;
2010-09-19 00:08:20 +02:00
real, dimension(nqt,im,jm,km) :: du
EVOLUTION: add forcing terms in the block update.
2010-12-08 21:48:43 -02:00
#ifdef FORCE
real, dimension( 3,im,jm,km) :: f
#endif /* FORCE */
New time integration method EULER.
2008-12-09 21:06:21 -06:00
!
!-------------------------------------------------------------------------------
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
! prepare dxi, dyi, and dzi
!
dxi = adxi(pblock%meta%level)
dyi = adyi(pblock%meta%level)
dzi = adzi(pblock%meta%level)
EVOLUTION: add forcing terms in the block update.
2010-12-08 21:48:43 -02:00
#ifdef FORCE
! obtain the forcing terms in real space
!
call real_forcing(pblock%meta%level, pblock%meta%xmin, pblock%meta%ymin &
, pblock%meta%zmin, f(:,:,:,:))
#endif /* FORCE */
New time integration method EULER.
2008-12-09 21:06:21 -06:00
! 1st step of integration
!
EVOLUTION: add forcing terms in the block update.
2010-12-08 21:48:43 -02:00
call update(pblock%u(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + pblock%u(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + pblock%u(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + pblock%u(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#ifdef SHAPE
! restrict update in a defined shape
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update_shapes(pblock, du)
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#endif /* SHAPE */
New time integration method EULER.
2008-12-09 21:06:21 -06:00
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
! update the solution for the fluid variables
New time integration method EULER.
2008-12-09 21:06:21 -06:00
!
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
pblock%u(1:nfl,:,:,:) = pblock%u(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:)
#ifdef MHD
! update the solution for the magnetic variables
!
pblock%u(ibx:ibz,:,:,:) = pblock%u(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:)
#ifdef GLM
GLM-MHD: take into account the maximum speed in update. - the divergence of B propagates with the maximum speed c_h; take it into account while updating the solution for the scalar potential Psi;
2010-12-01 10:57:40 -02:00
! calculate c_h^2
!
ch2 = cmax * cmax
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
! update the solution for the scalar potential Psi
!
GLM-MHD: take into account the maximum speed in update. - the divergence of B propagates with the maximum speed c_h; take it into account while updating the solution for the scalar potential Psi;
2010-12-01 10:57:40 -02:00
pblock%u(iph,:,:,:) = pblock%u(iph,:,:,:) + ch2 * dt * du(iph,:,:,:)
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
! evolve Psi due to the source term
!
decay = exp(- alpha_p * cmax * dt / dx_min)
pblock%u(iph,:,:,:) = decay * pblock%u(iph,:,:,:)
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#endif /* GLM */
#endif /* MHD */
Initial support for the MHD equations. VARIABLES - add indices for the magnetic field components, both face and cell centered SOLVER, MHD - add support for the magnetohydrodynamic (MHD) equations to the subroutines cons2prim(), prim2cons() - add MHD flux and the fastest speed calculation in the subroutine fluxspeed() - include magnetosonic speed in the calculation of the maximum speed in the system required for estimation of the new time step - extend the HLL solver in subroutine hll() to support MHD - calculate the magnetic field update according to a CT scheme in the subroutine update() INTERPOLATION - add subroutine magtocen() to interpolate cell centered magnetic field EVOLUTION - add evolution of the magnetic field components in the evolve_euler() and evolve_rk2() time integration subroutines - also call the subroutine magtocen() in the right places BOUNDARY CONDITIONS - support for magnetic field boundary update only in the case of blocks with the same level so far; later we need to include proper restriction and prolongation for the magnetic field to keep its divergence equal zero PROBLEMS, BLAST - extend the blast problem to include the initial magnetic field IO, HDF5 - write down in a HDF5 file magnetic field components
2009-10-28 00:12:18 -02:00
!
New time integration method EULER.
2008-12-09 21:06:21 -06:00
!-------------------------------------------------------------------------------
!
end subroutine evolve_euler
#endif /* EULER */
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
#ifdef RK2
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!===============================================================================
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
! evolve_rk2: subroutine evolves the current block using the 2nd order
! Runge-Kutta method
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!===============================================================================
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
subroutine evolve_rk2(pblock)
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
2010-12-01 09:25:30 -02:00
use blocks , only : block_data
use config , only : im, jm, km
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
use forcing , only : real_forcing
#endif /* FORCE */
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
use mesh , only : adxi, adyi, adzi
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#ifdef SHAPE
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
2010-12-01 09:25:30 -02:00
use problem , only : update_shapes
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#endif /* SHAPE */
SCHEME: move cmax parameter from module 'evolution' to 'scheme'.
2010-12-01 13:13:27 -02:00
use scheme , only : update, cmax
Move variable indices to new module 'variables'. VARIABLES - create new module 'variables' which stores references to variable indices; we gonna store dofferent objects related to variables in this module;
2010-12-01 09:25:30 -02:00
use variables, only : nqt, nfl
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#ifdef MHD
use variables, only : ibx, ibz
#ifdef GLM
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
use config , only : alpha_p
use mesh , only : dx_min
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
use variables, only : iph
#endif /* GLM */
#endif /* MHD */
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
use variables, only : idn, imx, imy, imz
#endif /* FORCE */
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
implicit none
! input arguments
!
Initial support for the MHD equations. VARIABLES - add indices for the magnetic field components, both face and cell centered SOLVER, MHD - add support for the magnetohydrodynamic (MHD) equations to the subroutines cons2prim(), prim2cons() - add MHD flux and the fastest speed calculation in the subroutine fluxspeed() - include magnetosonic speed in the calculation of the maximum speed in the system required for estimation of the new time step - extend the HLL solver in subroutine hll() to support MHD - calculate the magnetic field update according to a CT scheme in the subroutine update() INTERPOLATION - add subroutine magtocen() to interpolate cell centered magnetic field EVOLUTION - add evolution of the magnetic field components in the evolve_euler() and evolve_rk2() time integration subroutines - also call the subroutine magtocen() in the right places BOUNDARY CONDITIONS - support for magnetic field boundary update only in the case of blocks with the same level so far; later we need to include proper restriction and prolongation for the magnetic field to keep its divergence equal zero PROBLEMS, BLAST - extend the blast problem to include the initial magnetic field IO, HDF5 - write down in a HDF5 file magnetic field components
2009-10-28 00:12:18 -02:00
type(block_data), intent(inout) :: pblock
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
! local variables
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: dxi, dyi, dzi, ch2
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
#if defined MHD && defined GLM
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: decay
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
#endif /* MHD & GLM */
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
! local arrays
!
Remove flux calculation from the subroutine update(). SCHEME - remove the flux calculation from the subroutine update() and all dependent subroutines;
2010-09-19 00:08:20 +02:00
real, dimension(nqt,im,jm,km) :: u1, du
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
real, dimension( 3,im,jm,km) :: f
#endif /* FORCE */
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!-------------------------------------------------------------------------------
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
! prepare dxi, dyi, and dzi
!
dxi = adxi(pblock%meta%level)
dyi = adyi(pblock%meta%level)
dzi = adzi(pblock%meta%level)
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
! obtain the forcing terms in real space
!
call real_forcing(pblock%meta%level, pblock%meta%xmin, pblock%meta%ymin &
, pblock%meta%zmin, f(:,:,:,:))
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#if defined MHD && defined GLM
! calculate c_h^2
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
!
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
ch2 = cmax * cmax
#endif /* MHD & GLM */
!! 1st step of integration
!!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update(pblock%u(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + pblock%u(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + pblock%u(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + pblock%u(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#ifdef SHAPE
! restrict update in a defined shape
!
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
call update_shapes(pblock, du(:,:,:,:))
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#endif /* SHAPE */
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
! update the solution for the fluid variables
!
u1(1:nfl,:,:,:) = pblock%u(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:)
#ifdef MHD
! update the solution for the magnetic variables
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
!
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
u1(ibx:ibz,:,:,:) = pblock%u(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:)
#ifdef GLM
! update the solution for the scalar potential Psi
!
GLM-MHD: take into account the maximum speed in update. - the divergence of B propagates with the maximum speed c_h; take it into account while updating the solution for the scalar potential Psi;
2010-12-01 10:57:40 -02:00
u1(iph,:,:,:) = pblock%u(iph,:,:,:) + ch2 * dt * du(iph,:,:,:)
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#endif /* GLM */
#endif /* MHD */
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
! 2nd step of integration
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update(u1(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
EVOLUTION: add forcing terms in the RK2 update.
2010-12-08 21:55:45 -02:00
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + u1(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + u1(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + u1(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#ifdef SHAPE
! restrict update in a defined shape
!
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
call update_shapes(pblock, du(:,:,:,:))
Add support for the shapes in the domain. Now, we can define any shape for a given problem inside the domain, which is not updated during the evolution. This allows for using the sources of any kind in the problem studies, such as the colliding winds in the binary stars.
2008-12-18 12:18:36 -06:00
#endif /* SHAPE */
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
! update the solution for the fluid variables
!
pblock%u(1:nfl,:,:,:) = 0.5d0 * (pblock%u(1:nfl,:,:,:) &
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
+ u1(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:))
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#ifdef MHD
! update the solution for the magnetic variables
!
pblock%u(ibx:ibz,:,:,:) = 0.5d0 * (pblock%u(ibx:ibz,:,:,:) &
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
+ u1(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:))
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#ifdef GLM
! update the solution for the scalar potential Psi
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
!
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
pblock%u(iph,:,:,:) = 0.5d0 * (pblock%u(iph,:,:,:) &
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
+ u1(iph,:,:,:) + ch2 * dt * du(iph,:,:,:))
GLM-MHD: implement Psi decay due to a source term. - the scalar potential Psi evolution is controlled by a dissipative source term; include this update using a simple analytical solution;
2010-12-01 11:20:25 -02:00
! evolve Psi due to the source term
!
decay = exp(- alpha_p * cmax * dt / dx_min)
pblock%u(iph,:,:,:) = decay * pblock%u(iph,:,:,:)
GLM-MHD: update global solution. - update the magnetic field components and scalar potential in the Euler and RK2 methods, evolve_euler() and evolve_rk2() subroutines, respectively;
2010-12-01 10:53:21 -02:00
#endif /* GLM */
#endif /* MHD */
Initial support for the MHD equations. VARIABLES - add indices for the magnetic field components, both face and cell centered SOLVER, MHD - add support for the magnetohydrodynamic (MHD) equations to the subroutines cons2prim(), prim2cons() - add MHD flux and the fastest speed calculation in the subroutine fluxspeed() - include magnetosonic speed in the calculation of the maximum speed in the system required for estimation of the new time step - extend the HLL solver in subroutine hll() to support MHD - calculate the magnetic field update according to a CT scheme in the subroutine update() INTERPOLATION - add subroutine magtocen() to interpolate cell centered magnetic field EVOLUTION - add evolution of the magnetic field components in the evolve_euler() and evolve_rk2() time integration subroutines - also call the subroutine magtocen() in the right places BOUNDARY CONDITIONS - support for magnetic field boundary update only in the case of blocks with the same level so far; later we need to include proper restriction and prolongation for the magnetic field to keep its divergence equal zero PROBLEMS, BLAST - extend the blast problem to include the initial magnetic field IO, HDF5 - write down in a HDF5 file magnetic field components
2009-10-28 00:12:18 -02:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!-------------------------------------------------------------------------------
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
end subroutine evolve_rk2
Runge-Kutta 2nd order time integration implemented. In addition, I've done some fixes to the problem initialization, and I defined new variables igrids, jgrids, kgrids, which specify the dimensions of the block.
2008-12-08 16:21:59 -06:00
#endif /* RK2 */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#ifdef RK3
!
!===============================================================================
!
! evolve_rk3: subroutine evolves the current block using the 3rd order
! Runge-Kutta method
!
!===============================================================================
!
subroutine evolve_rk3(pblock)
use blocks , only : block_data
use config , only : im, jm, km
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
use forcing , only : real_forcing
#endif /* FORCE */
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
use mesh , only : adxi, adyi, adzi
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#ifdef SHAPE
use problem , only : update_shapes
#endif /* SHAPE */
use scheme , only : update, cmax
use variables, only : nqt, nfl
#ifdef MHD
use variables, only : ibx, ibz
#ifdef GLM
use config , only : alpha_p
use mesh , only : dx_min
use variables, only : iph
#endif /* GLM */
#endif /* MHD */
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
use variables, only : idn, imx, imy, imz
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
implicit none
! input arguments
!
type(block_data), intent(inout) :: pblock
! local variables
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: dxi, dyi, dzi, ch2
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#if defined MHD && defined GLM
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
real :: decay
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#endif /* MHD & GLM */
! local arrays
!
real, dimension(nqt,im,jm,km) :: u1, du
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
real, dimension( 3,im,jm,km) :: f
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
! parameters
!
real, parameter :: f4 = 1.0d0 / 4.0d0, f3 = 1.0d0 / 3.0d0
!
!-------------------------------------------------------------------------------
!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
! prepare dxi, dyi, and dzi
!
dxi = adxi(pblock%meta%level)
dyi = adyi(pblock%meta%level)
dzi = adzi(pblock%meta%level)
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
! obtain the forcing terms in real space
!
call real_forcing(pblock%meta%level, pblock%meta%xmin, pblock%meta%ymin &
, pblock%meta%zmin, f(:,:,:,:))
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#if defined MHD && defined GLM
! calculate c_h^2
!
ch2 = cmax * cmax
#endif /* MHD & GLM */
!! 1st step of integration
!!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update(pblock%u(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + pblock%u(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + pblock%u(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + pblock%u(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#ifdef SHAPE
! restrict update in a defined shape
!
call update_shapes(pblock, du(:,:,:,:))
#endif /* SHAPE */
! update the solution for the fluid variables
!
u1(1:nfl,:,:,:) = pblock%u(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:)
#ifdef MHD
! update the solution for the magnetic variables
!
u1(ibx:ibz,:,:,:) = pblock%u(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:)
#ifdef GLM
! update the solution for the scalar potential Psi
!
u1(iph,:,:,:) = pblock%u(iph,:,:,:) + ch2 * dt * du(iph,:,:,:)
#endif /* GLM */
#endif /* MHD */
!! 2nd step of integration
!!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update(u1(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + u1(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + u1(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + u1(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#ifdef SHAPE
! restrict update in a defined shape
!
call update_shapes(pblock, du(:,:,:,:))
#endif /* SHAPE */
! update the solution for the fluid variables
!
u1(1:nfl,:,:,:) = f4 * (3.0d0 * pblock%u(1:nfl,:,:,:) &
+ u1(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:))
#ifdef MHD
! update the solution for the magnetic variables
!
u1(ibx:ibz,:,:,:) = f4 * (3.0d0 * pblock%u(ibx:ibz,:,:,:) &
+ u1(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:))
#ifdef GLM
! update the solution for the scalar potential Psi
!
u1(iph,:,:,:) = f4 * (3.0d0 * pblock%u(iph,:,:,:) &
+ u1(iph,:,:,:) + ch2 * dt * du(iph,:,:,:))
#endif /* GLM */
#endif /* MHD */
!! 3rd step of integration
!!
Revert "INTERPOLATION: pass the spacial increment to reconstruct()." This reverts commit d92ae5d3a62743b66e97c42be4aa5f31ef5993d1.
2010-12-06 16:20:49 -02:00
call update(u1(:,:,:,:), du(:,:,:,:), dxi, dyi, dzi)
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
EVOLUTION: include forcing terms in the RK3 integration.
2010-12-09 17:54:59 -02:00
#ifdef FORCE
! update du due to forcing terms
!
du(imx,:,:,:) = du(imx,:,:,:) + u1(idn,:,:,:) * f(1,:,:,:)
du(imy,:,:,:) = du(imy,:,:,:) + u1(idn,:,:,:) * f(2,:,:,:)
du(imz,:,:,:) = du(imz,:,:,:) + u1(idn,:,:,:) * f(3,:,:,:)
#endif /* FORCE */
EVOLUTION: implement the 3rd order RK method. - implement the 3rd order Runge-Kutta time integration; - rewrite slightly the 2nd order Runge-Kutta method;
2010-12-03 15:38:48 -02:00
#ifdef SHAPE
! restrict update in a defined shape
!
call update_shapes(pblock, du(:,:,:,:))
#endif /* SHAPE */
! update the solution for the fluid variables
!
pblock%u(1:nfl,:,:,:) = f3 * (pblock%u(1:nfl,:,:,:) &
+ 2.0d0 * (u1(1:nfl,:,:,:) + dt * du(1:nfl,:,:,:)))
#ifdef MHD
! update the solution for the magnetic variables
!
pblock%u(ibx:ibz,:,:,:) = f3 * (pblock%u(ibx:ibz,:,:,:) &
+ 2.0d0 * (u1(ibx:ibz,:,:,:) + dt * du(ibx:ibz,:,:,:)))
#ifdef GLM
! update the solution for the scalar potential Psi
!
pblock%u(iph,:,:,:) = f3 * (pblock%u(iph,:,:,:) &
+ 2.0d0 * (u1(iph,:,:,:) + ch2 * dt * du(iph,:,:,:)))
! evolve analytically Psi due to the source term
!
decay = exp(- alpha_p * cmax * dt / dx_min)
pblock%u(iph,:,:,:) = decay * pblock%u(iph,:,:,:)
#endif /* GLM */
#endif /* MHD */
!
!-------------------------------------------------------------------------------
!
end subroutine evolve_rk3
#endif /* RK3 */
Implement FLUXCT integration of the induction equation. SCHEME - implement Flux-CT scheme for the staggered magnetic field integration; BLOCK STRUCTURE - use more space efficient storage of the variables, which means storing only staggered components of magnetic field; cell-centered components are calculated only when necessary; EVOLUTION - remove loops in the field updates; operations are performed on the arrays; BOUNDARY CONDITIONS - remove loops in the bnd_copy; operations are calculated on the whole array now; INTERPOLATION - subroutine magtocen() has been rewritten to avoid problems with the array allocation; now as an argument we enter the array of all variables; subroutine uses indices for the face-centered and cell-centered magnetic field components internally; MAKE - add flag defining Flux-CT scheme; PROBLEM - use predefined array variables instead of allocated;
2010-02-28 18:35:57 -03:00
!
Updated comments in the evolution module.
2008-12-08 21:07:10 -06:00
!===============================================================================
New module 'evolution' for time integration. A new module for the time integration has been added. This module contains a set of subroutines to perform one step time integration of each leaf block using 2nd order Runge-Kutta method. More methods can be added later. Time 't', timestep 'dt' and iteration 'n' have been moved to this module as well.
2008-12-07 18:57:08 -06:00
!
end module
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