fargo2python/fargo2python.py at main · charango/fargo2python · GitHub

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# ===================================================================
# FARGO to PYTHON
# code written by Clement Baruteau (CB), with contributions from
# Pablo Benitez-Llambay and Gaylor Wafflard-Fernandez
# ===================================================================
#
# program can run with either Python 2.X or Python 3.X.
#
# NB: logarithmic color scale requires matplotblib version > 3.0 to
# display color bar properly
#
# ===================================================================

# =========================================
# TO DO LIST
# =========================================
# - think of a better handling of 3D case? Right now I can only plot the primitive fields in a
# vertical plane, not the fields built upon primitive ones (like the vorticity etc.).
# - show RH around planet
# - axifield (minor): add 1D visc evolving profiles, add planet position via dashed line
# =========================================

# Plotting parameters
importmatplotlib
matplotlib.rcParams.update({'font.size': 24})
matplotlib.rc('font', family='Arial')

# =====================
# 1. IMPORT GLOBAL VARIABLES
# =====================
importpar
ifpar.allfluids=='Yes':
matplotlib.rcParams.update({'font.size': 20})

# =====================
# 2. DISPLAY 2D FIELDS
# =====================
ifpar.onedprofile=='No'andpar.plot_field==True:
fromplot_twodfieldimport*
plottwodfield()

# =====================
# 3. DISPLAY AZIMUTHALLY-AVERAGED RADIAL 1D PROFILES
# =====================
ifpar.onedprofile!='No'andpar.plot_field==True:
ifpar.onedspacetime=='Yes':
fromplot_spacetimediagramimport*
plotspacetimediagram()

else:
fromplot_onedprofileimport*
plotonedprofile()

# =====================
# 4. DISPLAY TIME EVOLUTION OF DISC TORQUE OR POWER ON PLANET(s)
# =====================
ifpar.plot_tqwk!='No':
fromplot_tqwkimport*
plottqwk()

# =====================
# 5. DISPLAY TIME EVOLUTION OF PLANET ORBITAL ELEMENTS
# =====================
ifpar.plot_planet!='No':
fromplot_planetimport*
plotplanet()

# =====================
# 6. DISPLAY STUFF FOR DUST PARTICLES (only for Dusty-FARGO ADSG)
# =====================
ifpar.plot_dust!='No'andpar.fargo3d=='No':
fromplot_dustimport*
plotdust()

# =====================
# 7. DISC'S CENTER OF MASS
# =====================
if ( ('plot_disccom'inopen('paramsf2p.dat').read()) and (par.plot_disccom!='No') ):
fromplot_disccomimport*
plotdisccom()

# =====================
# 8. DISC MASS (time)
# =====================
if ( ('plot_discmass'inopen('paramsf2p.dat').read()) and (par.plot_discmass!='No') ):
fromplot_discmassimport*
plotdiscmass()

# =====================
# 9. ratio of orbit-crossing and librating inverse vortensities (time)
# =====================
if ( ('plot_libcross'inopen('paramsf2p.dat').read()) and (par.plot_libcross!='No') ):
fromplot_libcrossimport*
plotlibcross()

# =====================
# 10. disc turbulent properties
# =====================
if ( ('plot_turb'inopen('paramsf2p.dat').read()) and (par.plot_turb!='No') ):
fromplot_turbimport*
ifpar.plot_turb=='power_spectrum':
plotpowerspectrum()
ifpar.plot_turb=='auto_correlation':
plotautocorrelationtimescale()
ifpar.plot_turb=='alphas':
plot_alphas()
ifpar.plot_turb=='histo_field':
plot_histofield()
ifpar.plot_turb=='histo_torque':
plot_histotorque()
ifpar.plot_turb=='time_alphareynolds':
plot_time_alphaRey()
ifpar.plot_turb=='time_alphagrav':
plot_time_alphaGrav()
ifpar.plot_turb=='time_alphagrav_ext':
plot_time_alphaGrav_external()

# =====================
# 11. DISC'S ECCENTRICITY OR PERICENTRE ARGUMENT
# =====================
if ( ('plot_discecc'inopen('paramsf2p.dat').read()) and (par.plot_discecc!='No') ):
fromplot_discbinaryimport*
plotdiscecc()
if ( ('plot_discperarg'inopen('paramsf2p.dat').read()) and (par.plot_discperarg!='No') ):
fromplot_discbinaryimport*
plotdiscperarg()

# =====================
# 12. FOURIER ANALYSIS
# =====================
if ( ('plot_fourier'inopen('paramsf2p.dat').read()) and (par.plot_fourier!='No') ):
fromplot_fourierimport*
if (par.plot_fourier=='naodens'orpar.plot_fourier=='rossby'):
plotmaxnaodens_orminrossby()
else:
plotfourier()