Welcome! Here is my Julia code to simulate 2D convection in a Cartesian box. Theory and methods used can be found in Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation.
- Julia (version 1.6)
convect-jl
docs/
src/
convect_linear.jl
convect_nonlinear.jl
critical_ra.jl
data_utils.jl
postprocess.jl
routines.jl
LICENSE.md
README.md
-
Open
src/convect_linear.jl
-
Specify input parameters
# Inputs
nz = 101 # no. of vertical gridpoints
nn = 30 # no. of horizontal Fourier modes (excluding zeroth mode)
a = 5 # L/D aspect ratio
Ra = 2700 # Rayleigh number
Pr = 0.5 # Prandtl number
nt = 1e5 # no. of timesteps
nout = 1e3 # output every nout timesteps
zeroth = 0 # include zeroth order temperature in plot?
initOn = 1
saveDir = "/Users/wongj/Documents/convect-out/linear/2021-09-03"
-
Run script from terminal using
julia <working directory>/convect-jl/src/convect_linear.jl
(or from julia REPL usinginclude("<working directory>/convect-jl/src/convect_linear.jl")
) -
Admire the output:
-
Open
src/convect_nonlinear.jl
-
Specify input parameters
# Inputs
nz = 101 # no. of vertical gridpoints
nn = 50 # no. of Fourier modes (excluding zeroth mode)
a = 3 # L/D aspect ratio
Ra = 1e6 # Rayleigh number
Pr = 0.5 # Prandtl number
dt = 3e-6 # timestep size
nt = 1e4 # no. of timesteps
nout = 1e2 # save output every nout timesteps
initOn = 1 # initialise run, otherwise load existing data
saveDir = "/Users/wongj/Documents/convect-out/2021-09-03" # save directory
-
Run script from terminal using
julia <working directory>/convect-jl/src/convect_nonlinear.jl
(or from julia REPL usinginclude("<working directory>/convect-jl/src/convect_nonlinear.jl")
) -
Postprocess and visualise the data using
julia <working directory>/convect-jl/src/postprocess.jl
(or from julia REPL usinginclude("<working directory>/convect-jl/src/postprocess.jl")
) with the following input parameters
# Inputs
saveDir = "/Users/wongj/Documents/convect-out/2021-09-03" # save directory
nStart = 1
nEnd = 500
zeroth= 1 # plot zeroth mode?
- Admire the output:
- Jenny Wong - Institut des Sciences de la Terre
This project is licensed under the MIT License - see the LICENSE.md file for details
🎉