-
Notifications
You must be signed in to change notification settings - Fork 2
drreynolds/rmhd3d_share
Folders and files
| Name | Name | Last commit message | Last commit date | |
|---|---|---|---|---|
Repository files navigation
Building and Running RMHD2D:
1. Edit one of the machine-dependent Makefiles,
e.g. Make.reynolds-linux, to set up the various compilers, compiler
flags, libraries, and Fortran-to-C translation directives.
2. Link this machine-dependent Makefile to Make.machine: e.g.
ln -s Make.reynolds-linux Make.machine
3. To set the problem size and parallelism topology, do either of the
following two steps:
3a. Edit the file include/make_uparms_static.h to set the problem
size (nx, ny and nz give the total problem dimensions) along
with the parallelism topology information (xprocs, yprocs and
zprocs give the number of processors in each cartesian
dimension).
3b. Edit Make.config to ensure that -DDYNAMIC is set. Then copy
the input parameter file ./inputs/mesh.inp to the
runtime-directory. Edit this file with the same information as
in 4a.
NOTE: this option allows runs of differing dimension without
re-compiling the executable.
4. Edit one of the problem configuration makefiles,
e.g. Make.config-KH, to set up the appropriate dimensionality (2D
vs 2.5D), boundary conditions, flux discretization choices,
parallelism, and preconditioning for the type of problem that you
wish to run.
5. Link this problem-dependent Makefile to Make.config: e.g.
ln -s Make.config-KH Make.config
6. Type 'make <target>', where <target> specifies the type of executable
(problem type and time integration algorithm) that you wish to
build. Typing 'make' alone will bring up a list of possible
targets.
7. Copy problem-specific input files to the run-time directory from
the ./inputs directory. You will need the files mhd.inp and
prop.inp for all problems (remove the problem specifier suffix from
the file name). For some problems, you will also need the
problem-specific input parameter files provided in this directory,
e.g. the Kelvin-Helmholtz problem requires kh_init.inp. If the
time-integration algorithm is KINSOL, you will also need
kincontrol.inp; if it is CVODE, you will need cvcontrol.inp.
8. Edit the input files to your tastes and run your executable.
About
Shared version of 3D Cartesian geometry, finite volume, implicit viscoresistive MHD research code.
Resources
Stars
Watchers
Forks
Releases
No releases published
Packages 0
No packages published