Merge branch 'master' into no_unnecessary_loop_in_pair

README

@@ -28,6 +28,7 @@ Valid options are:
   -G          Run with self-gravity
   -n    {int} Execute a fixed number of time steps. When unset use the time_end parameter to stop. 
   -s          Run with SPH
+  -S          Run with stars
   -t    {int} The number of threads to use on each MPI rank. Defaults to 1 if not specified.
   -v     [12] Increase the level of verbosity
   	      1: MPI-rank 0 writes

doc/Doxyfile.in

@@ -762,6 +762,7 @@ WARN_LOGFILE           =
 INPUT                  =  @top_srcdir@ @top_srcdir@/src @top_srcdir@/tests @top_srcdir@/examples
 INPUT		       += @top_srcdir@/src/hydro/Minimal
 INPUT		       += @top_srcdir@/src/gravity/Default
+INPUT		       += @top_srcdir@/src/stars/Default
 INPUT		       += @top_srcdir@/src/riemann
 INPUT		       += @top_srcdir@/src/potential/point_mass
 INPUT		       += @top_srcdir@/src/cooling/const_du

examples/EAGLE_100/README

+ICs extracted from the EAGLE suite of simulations. 
+
+WARNING: The ICs are 217GB in size. They contain ~3.4G DM particles,
+~3.2G gas particles and ~170M star particles
+
+The particle distribution here is the snapshot 27 (z=0.1) of the 100Mpc
+Ref-model. h- and a- factors from the original Gadget code have been
+corrected for. Variables not used in a pure hydro & gravity code have
+been removed. 
+Everything is ready to be run without cosmological integration. 
+
+The particle load of the main EAGLE simulation can be reproduced by
+running these ICs on 4096 cores.
+
+MD5 checksum of the ICs:
+2301ea73e14207b541bbb04163c5269e  EAGLE_ICs_100.hdf5

examples/Feedback/feedback.yml → examples/EAGLE_100/eagle_100.yml

 # Define the system of units to use internally. 
 InternalUnitSystem:
-  UnitMass_in_cgs:     1   # Grams
-  UnitLength_in_cgs:   1   # Centimeters
-  UnitVelocity_in_cgs: 1   # Centimeters per second
-  UnitCurrent_in_cgs:  1   # Amperes
-  UnitTemp_in_cgs:     1   # Kelvin
+  UnitMass_in_cgs:     1.989e43      # 10^10 M_sun in grams
+  UnitLength_in_cgs:   3.085678e24   # Mpc in centimeters
+  UnitVelocity_in_cgs: 1e5           # km/s in centimeters per second
+  UnitCurrent_in_cgs:  1             # Amperes
+  UnitTemp_in_cgs:     1             # Kelvin
 
 # Parameters governing the time integration
 TimeIntegration:
   time_begin: 0.    # The starting time of the simulation (in internal units).
-  time_end:   5e-2  # The end time of the simulation (in internal units).
-  dt_min:     1e-7  # The minimal time-step size of the simulation (in internal units).
+  time_end:   1e-2  # The end time of the simulation (in internal units).
+  dt_min:     1e-10 # The minimal time-step size of the simulation (in internal units).
   dt_max:     1e-4  # The maximal time-step size of the simulation (in internal units).
 
 # Parameters governing the snapshots
 Snapshots:
-  basename:            Feedback # Common part of the name of output files
-  time_first:          0.       # Time of the first output (in internal units)
-  delta_time:          1e-2     # Time difference between consecutive outputs (in internal units)
+  basename:            eagle # Common part of the name of output files
+  time_first:          0.    # Time of the first output (in internal units)
+  delta_time:          1e-3  # Time difference between consecutive outputs (in internal units)
 
 # Parameters governing the conserved quantities statistics
 Statistics:
-  delta_time:          1e-3 # Time between statistics output
+  delta_time:          1e-2 # Time between statistics output
 
 # Parameters for the hydrodynamics scheme
 SPH:
@@ -31,13 +31,5 @@ SPH:
 
 # Parameters related to the initial conditions
 InitialConditions:
-  file_name:  ./Feedback.hdf5          # The file to read
+  file_name:  ./EAGLE_ICs_100.hdf5     # The file to read
 
-# Parameters for feedback
-
-SN:
-  time:    0.001 # time the SN explodes (internal units)
-  energy:  1.0   # energy of the explosion (internal units)
-  x:       0.5   # x-position of explostion (internal units)
-  y:       0.5   # y-position of explostion (internal units)
-  z:       0.5   # z-position of explostion (internal units)

examples/EAGLE_100/getIC.sh

+#!/bin/bash
+wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/ICs/EAGLE_ICs_100.hdf5

examples/EAGLE_100/run.sh

+#!/bin/bash
+
+ # Generate the initial conditions if they are not present.
+if [ ! -e EAGLE_ICs_100.hdf5 ]
+then
+    echo "Fetching initial conditions for the EAGLE 100Mpc example..."
+    ./getIC.sh
+fi
+
+../swift -s -t 16 eagle_100.yml 2>&1 | tee output.log
+

examples/ExternalPointMass/energy_plot.py

+import matplotlib
+matplotlib.use("Agg")
+from pylab import *
+import h5py
+
+# Plot parameters
+params = {'axes.labelsize': 10,
+'axes.titlesize': 10,
+'font.size': 12,
+'legend.fontsize': 12,
+'xtick.labelsize': 10,
+'ytick.labelsize': 10,
+'text.usetex': True,
+ 'figure.figsize' : (3.15,3.15),
+'figure.subplot.left'    : 0.145,
+'figure.subplot.right'   : 0.99,
+'figure.subplot.bottom'  : 0.11,
+'figure.subplot.top'     : 0.99,
+'figure.subplot.wspace'  : 0.15,
+'figure.subplot.hspace'  : 0.12,
+'lines.markersize' : 6,
+'lines.linewidth' : 3.,
+'text.latex.unicode': True
+}
+rcParams.update(params)
+rc('font',**{'family':'sans-serif','sans-serif':['Times']})
+
+
+import numpy as np
+import h5py as h5
+import sys
+
+# File containing the total energy
+stats_filename = "./energy.txt"
+
+# First snapshot
+snap_filename = "pointMass_000.hdf5"
+f = h5.File(snap_filename,'r')
+
+# Read the units parameters from the snapshot
+units = f["InternalCodeUnits"]
+unit_mass = units.attrs["Unit mass in cgs (U_M)"]
+unit_length = units.attrs["Unit length in cgs (U_L)"]
+unit_time = units.attrs["Unit time in cgs (U_t)"]
+
+G = 6.67408e-8 * unit_mass * unit_time**2 / unit_length**3
+
+# Read the header
+header = f["Header"]
+box_size = float(header.attrs["BoxSize"][0])
+
+# Read the properties of the potential
+parameters = f["Parameters"]
+mass = float(parameters.attrs["PointMassPotential:mass"])
+centre = [box_size/2, box_size/2, box_size/2]
+f.close()
+
+# Read the statistics summary
+file_energy = np.loadtxt("energy.txt")
+time_stats = file_energy[:,0]
+E_kin_stats = file_energy[:,3]
+E_pot_stats = file_energy[:,5]
+E_tot_stats = E_kin_stats + E_pot_stats
+
+# Read the snapshots
+time_snap = np.zeros(402)
+E_kin_snap = np.zeros(402)
+E_pot_snap = np.zeros(402)
+E_tot_snap = np.zeros(402)
+Lz_snap = np.zeros(402)
+
+# Read all the particles from the snapshots
+for i in range(402):
+    snap_filename = "pointMass_%0.3d.hdf5"%i
+    f = h5.File(snap_filename,'r')
+
+    pos_x = f["PartType1/Coordinates"][:,0]
+    pos_y = f["PartType1/Coordinates"][:,1]
+    pos_z = f["PartType1/Coordinates"][:,2]
+    vel_x = f["PartType1/Velocities"][:,0]
+    vel_y = f["PartType1/Velocities"][:,1]
+    vel_z = f["PartType1/Velocities"][:,2]
+    m = f["/PartType1/Masses"][:]
+    
+    r = np.sqrt((pos_x[:] - centre[0])**2 + (pos_y[:] - centre[1])**2 + (pos_z[:] - centre[2])**2)
+    Lz = (pos_x[:] - centre[0]) * vel_y[:] - (pos_y[:] - centre[1]) * vel_x[:]
+
+    time_snap[i] = f["Header"].attrs["Time"]
+    E_kin_snap[i] = np.sum(0.5 * m * (vel_x[:]**2 + vel_y[:]**2 + vel_z[:]**2))
+    E_pot_snap[i] = np.sum(-mass * m * G / r)
+    E_tot_snap[i] = E_kin_snap[i] + E_pot_snap[i]
+    Lz_snap[i] = np.sum(Lz)
+
+# Plot energy evolution
+figure()
+plot(time_stats, E_kin_stats, "r-", lw=0.5, label="Kinetic energy")
+plot(time_stats, E_pot_stats, "g-", lw=0.5, label="Potential energy")
+plot(time_stats, E_tot_stats, "k-", lw=0.5, label="Total energy")
+
+plot(time_snap[::10], E_kin_snap[::10], "rD", lw=0.5, ms=2)
+plot(time_snap[::10], E_pot_snap[::10], "gD", lw=0.5, ms=2)
+plot(time_snap[::10], E_tot_snap[::10], "kD", lw=0.5, ms=2)
+
+legend(loc="center right", fontsize=8, frameon=False, handlelength=3, ncol=1)
+xlabel("${\\rm{Time}}$", labelpad=0)
+ylabel("${\\rm{Energy}}$",labelpad=0)
+xlim(0, 8)
+
+savefig("energy.png", dpi=200)
+
+# Plot angular momentum evolution
+figure()
+plot(time_snap, Lz_snap, "k-", lw=0.5, ms=2)
+
+xlabel("${\\rm{Time}}$", labelpad=0)
+ylabel("${\\rm{Angular~momentum}}$",labelpad=0)
+xlim(0, 8)
+
+savefig("angular_momentum.png", dpi=200)
+
+

examples/ExternalPointMass/externalPointMass.yml

@@ -9,7 +9,7 @@ InternalUnitSystem:
 # Parameters governing the time integration
 TimeIntegration:
   time_begin: 0.    # The starting time of the simulation (in internal units).
-  time_end:   1.    # The end time of the simulation (in internal units).
+  time_end:   8.    # The end time of the simulation (in internal units).
   dt_min:     1e-6  # The minimal time-step size of the simulation (in internal units).
   dt_max:     1e-3  # The maximal time-step size of the simulation (in internal units).
 
@@ -31,7 +31,7 @@ SPH:
 
 # Parameters related to the initial conditions
 InitialConditions:
-  file_name:  Sphere.hdf5           # The file to read
+  file_name:  PointMass.hdf5        # The file to read
   shift_x:    50.                   # A shift to apply to all particles read from the ICs (in internal units).
   shift_y:    50.
   shift_z:    50.

examples/ExternalPointMass/makeIC.py

@@ -24,10 +24,10 @@ import numpy
 import math
 import random
 
-# Generates a random distriution of particles, for motion in an external potnetial centred at (0,0,0)
+# Generates a random distriution of particles, for motion in an external potential centred at (0,0,0)
 
 # physical constants in cgs
-NEWTON_GRAVITY_CGS  = 6.672e-8
+NEWTON_GRAVITY_CGS  = 6.67408e-8
 SOLAR_MASS_IN_CGS   = 1.9885e33
 PARSEC_IN_CGS       = 3.0856776e18
 
@@ -39,34 +39,28 @@ const_unit_velocity_in_cgs =   (1e5)
 print "UnitMass_in_cgs:     ", const_unit_mass_in_cgs 
 print "UnitLength_in_cgs:   ", const_unit_length_in_cgs
 print "UnitVelocity_in_cgs: ", const_unit_velocity_in_cgs
+print "UnitTime_in_cgs:     ", const_unit_length_in_cgs / const_unit_velocity_in_cgs
 
 # derived units
 const_unit_time_in_cgs = (const_unit_length_in_cgs / const_unit_velocity_in_cgs)
 const_G                = ((NEWTON_GRAVITY_CGS*const_unit_mass_in_cgs*const_unit_time_in_cgs*const_unit_time_in_cgs/(const_unit_length_in_cgs*const_unit_length_in_cgs*const_unit_length_in_cgs)))
-print 'G=', const_G
+print '---------------------'
+print 'G in internal units: ', const_G
 
 
 # Parameters
-periodic= 1            # 1 For periodic box
-boxSize = 100.         # 
-Radius  = boxSize / 4. # maximum radius of particles
-G       = const_G 
-Mass    = 1e10         
+periodic   = 1            # 1 For periodic box
+boxSize    = 100.         # 
+max_radius = boxSize / 4. # maximum radius of particles
+Mass       = 1e10         
+print "Mass at the centre:  ", Mass
 
-N       = int(sys.argv[1])  # Number of particles
-L       = N**(1./3.)
+numPart = int(sys.argv[1])  # Number of particles
+mass    = 1.
 
-# these are not used but necessary for I/O
-rho = 2.              # Density
-P = 1.                # Pressure
-gamma = 5./3.         # Gas adiabatic index
-fileName = "Sphere.hdf5" 
+fileName = "PointMass.hdf5" 
 
 
-#---------------------------------------------------
-numPart        = N
-mass           = 1
-internalEnergy = P / ((gamma - 1.)*rho)
 
 #--------------------------------------------------
 
@@ -98,25 +92,26 @@ grp.attrs["Unit current in cgs (U_I)"] = 1.
 grp.attrs["Unit temperature in cgs (U_T)"] = 1.
 
 #Particle group
-#grp0 = file.create_group("/PartType0")
 grp1 = file.create_group("/PartType1")
+
 #generate particle positions
-radius = Radius * (numpy.random.rand(N))**(1./3.) 
-ctheta = -1. + 2 * numpy.random.rand(N)
-stheta = numpy.sqrt(1.-ctheta**2)
-phi    =  2 * math.pi * numpy.random.rand(N)
+radius = max_radius * (numpy.random.rand(numPart))**(1./3.)
+print '---------------------'
+print 'Radius: minimum = ',min(radius)
+print 'Radius: maximum = ',max(radius)
+radius = numpy.sort(radius)
 r      = numpy.zeros((numPart, 3))
-# r[:,0] = radius * stheta * numpy.cos(phi)
-# r[:,1] = radius * stheta * numpy.sin(phi)
-# r[:,2] = radius * ctheta
 r[:,0] = radius
-#
-speed  = numpy.sqrt(G * Mass / radius)
-v      = numpy.zeros((numPart, 3))
+
+#generate particle velocities
+speed  = numpy.sqrt(const_G * Mass / radius)
 omega  = speed / radius
 period = 2.*math.pi/omega
-print 'period = minimum = ',min(period), ' maximum = ',max(period)
+print '---------------------'
+print 'Period: minimum = ',min(period)
+print 'Period: maximum = ',max(period)
 
+v      = numpy.zeros((numPart, 3))
 v[:,0] = -omega * r[:,1]
 v[:,1] =  omega * r[:,0]
 
@@ -129,17 +124,6 @@ ds = grp1.create_dataset('Masses', (numPart,), 'f')
 ds[()] = m
 m = numpy.zeros(1)
 
-h = numpy.full((numPart, ), 1.1255 * boxSize / L)
-ds = grp1.create_dataset('SmoothingLength', (numPart,), 'f')
-ds[()] = h
-h = numpy.zeros(1)
-
-u = numpy.full((numPart, ), internalEnergy)
-ds = grp1.create_dataset('InternalEnergy', (numPart,), 'f')
-ds[()] = u
-u = numpy.zeros(1)
-
-
 ids = 1 + numpy.linspace(0, numPart, numPart, endpoint=False)
 ds = grp1.create_dataset('ParticleIDs', (numPart, ), 'L')
 ds[()] = ids

examples/ExternalPointMass/run.sh

 #!/bin/bash
 
 # Generate the initial conditions if they are not present.
-if [ ! -e Sphere.hdf5 ]
+if [ ! -e PointMass.hdf5 ]
 then
     echo "Generating initial conditions for the point mass potential box example..."
     python makeIC.py 10000
 fi
 
+rm -rf pointMass_*.hdf5
 ../swift -g -t 1 externalPointMass.yml 2>&1 | tee output.log
+
+python energy_plot.py

examples/ExternalPointMass/test.pro

-;
-;  test energy / angular momentum conservation of test problem
-;
-@physunits
-
-indir    = '/gpfs/data/tt/Codes/Swift-git/swiftsim/examples/'
-basefile = 'output_'
-nfiles   = 657
-nfollow  = 100 ; number of particles to follow
-eout     = fltarr(nfollow, nfiles)
-ekin     = fltarr(nfollow, nfiles)
-epot     = fltarr(nfollow, nfiles)
-tout     = fltarr(nfiles)
-; set properties of potential
-uL  = 1e3 * phys.pc             ; unit of length
-uM  = phys.msun                 ; unit of mass
-uV  = 1d5                       ; unit of velocity
-
-; derived units
-constG   = 10.^(alog10(phys.g)+alog10(uM)-2d0*alog10(uV)-alog10(uL)) ;
-pcentre  = [50.,50.,50.] * 1d3 * pc / uL
-mextern  = 1d10 * msun / uM
-;
-;
-;
-ifile  = 0
-for ifile=0,nfiles-1 do begin
-;for ifile=0,3 do begin
-   inf    = indir + basefile + strtrim(string(ifile,'(i3.3)'),1) + '.hdf5'
-   time   = h5ra(inf, 'Header','Time')
-   p      = h5rd(inf,'PartType1/Coordinates')
-   v      = h5rd(inf,'PartType1/Velocities')
-   id     = h5rd(inf,'PartType1/ParticleIDs')
-   indx   = sort(id)
-;
-   id     = id[indx]
-   for ic=0,2 do begin
-      tmp = reform(p[ic,*]) & p[ic,*] = tmp[indx]
-      tmp = reform(v[ic,*]) & v[ic,*] = tmp[indx]
-   endfor
-; calculate energy
-   dd  = size(p,/dimen) & npart = dd[1]
-   ener = fltarr(npart)
-   dr   = fltarr(npart) & dv = dr
-   for ic=0,2 do dr[*] = dr[*] + (p[ic,*]-pcentre[ic])^2
-   for ic=0,2 do dv[*] = dv[*] + v[ic,*]^2
-   dr = sqrt(dr)
-;   print,'time = ',time,p[0,0],v[0,0],id[0]
-   ek   = 0.5 * dv
-   ep   = - constG * mextern / dr
-   ener = ek + ep
-   tout(ifile) = time
-   eout(*,ifile) = ener[0:nfollow-1]
-   ekin(*,ifile) = ek[0:nfollow-1]
-   epot(*,ifile) = ep[0:nfollow-1]
-endfor
-
-; calculate relative energy change
-de = 0.0 * eout
-for ifile=1, nfiles -1 do de[*,ifile] = (eout[*,ifile]-eout[*,0])/eout[*,0]
-
-
-end
-
-

examples/Feedback/feedback.pro

-base = 'Feedback'
-inf  = 'Feedback_005.hdf5'
-
-blast  = [5.650488e-01, 5.004371e-01, 5.010494e-01] ; location of blast
-pos    = h5rd(inf,'PartType0/Coordinates')
-vel    = h5rd(inf,'PartType0/Velocities')
-rho    = h5rd(inf,'PartType0/Density')
-utherm = h5rd(inf,'PartType0/InternalEnergy')
-
-; shift to centre
-for ic=0,2 do pos[ic,*] = pos[ic,*] - blast[ic]
-
-;; distance from centre
-dist = fltarr(n_elements(rho))
-for ic=0,2 do dist = dist + pos[ic,*]^2
-dist = sqrt(dist)
-
-; radial velocity
-vr = fltarr(n_elements(rho))
-for ic=0,2 do vr = vr + pos[ic,*]*vel[ic,*]
-vr = vr / dist
-
-; 
-end

examples/Feedback/makeIC.py

-###############################################################################
- # This file is part of SWIFT.
- # Copyright (c) 2013 Pedro Gonnet (pedro.gonnet@durham.ac.uk),
- #                    Matthieu Schaller (matthieu.schaller@durham.ac.uk)
- #               2016 Tom Theuns (tom.theuns@durham.ac.uk)
- # 
- # This program is free software: you can redistribute it and/or modify
- # it under the terms of the GNU Lesser General Public License as published
- # by the Free Software Foundation, either version 3 of the License, or
- # (at your option) any later version.
- # 
- # This program 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 Lesser General Public License
- # along with this program.  If not, see <http://www.gnu.org/licenses/>.
- # 
- ##############################################################################
-
-import h5py
-import sys
-from numpy import *
-
-# Generates a swift IC file containing a cartesian distribution of particles
-# at a constant density and pressure in a cubic box
-
-# Parameters
-periodic= 1           # 1 For periodic box
-boxSize = 1.
-L = int(sys.argv[1])  # Number of particles along one axis
-rho = 1.              # Density
-P = 1.e-6             # Pressure
-gamma = 5./3.         # Gas adiabatic index
-eta = 1.2349          # 48 ngbs with cubic spline kernel
-fileName = "Feedback.hdf5" 
-
-#---------------------------------------------------
-numPart = L**3
-mass = boxSize**3 * rho / numPart
-internalEnergy = P / ((gamma - 1.)*rho)
-
-#--------------------------------------------------
-
-#File
-file = h5py.File(fileName, 'w')
-
-# Header
-grp = file.create_group("/Header")
-grp.attrs["BoxSize"] = boxSize
-grp.attrs["NumPart_Total"] =  [numPart, 0, 0, 0, 0, 0]
-grp.attrs["NumPart_Total_HighWord"] = [0, 0, 0, 0, 0, 0]
-grp.attrs["NumPart_ThisFile"] = [numPart, 0, 0, 0, 0, 0]
-grp.attrs["Time"] = 0.0
-grp.attrs["NumFilesPerSnapshot"] = 1
-grp.attrs["MassTable"] = [0.0, 0.0, 0.0, 0.0, 0.0, 0.0]
-grp.attrs["Flag_Entropy_ICs"] = 0
-
-#Runtime parameters
-grp = file.create_group("/RuntimePars")
-grp.attrs["PeriodicBoundariesOn"] = periodic
-
-#Units
-grp = file.create_group("/Units")
-grp.attrs["Unit length in cgs (U_L)"] = 1.
-grp.attrs["Unit mass in cgs (U_M)"] = 1.
-grp.attrs["Unit time in cgs (U_t)"] = 1.
-grp.attrs["Unit current in cgs (U_I)"] = 1.
-grp.attrs["Unit temperature in cgs (U_T)"] = 1.
-
-#Particle group
-grp = file.create_group("/PartType0")
-
-v  = zeros((numPart, 3))
-ds = grp.create_dataset('Velocities', (numPart, 3), 'f')
-ds[()] = v
-v = zeros(1)
-
-m = full((numPart, 1), mass)
-ds = grp.create_dataset('Masses', (numPart,1), 'f')
-ds[()] = m
-m = zeros(1)
-
-h = full((numPart, 1), eta * boxSize / L)
-ds = grp.create_dataset('SmoothingLength', (numPart,1), 'f')
-ds[()] = h
-h = zeros(1)
-
-u = full((numPart, 1), internalEnergy)
-ds = grp.create_dataset('InternalEnergy', (numPart,1), 'f')
-ds[()] = u
-u = zeros(1)
-
-
-ids = linspace(0, numPart, numPart, endpoint=False).reshape((numPart,1))
-ds = grp.create_dataset('ParticleIDs', (numPart, 1), 'L')
-ds[()] = ids + 1
-x      = ids % L;
-y      = ((ids - x) / L) % L;
-z      = (ids - x - L * y) / L**2;
-coords = zeros((numPart, 3))
-coords[:,0] = z[:,0] * boxSize / L + boxSize / (2*L)
-coords[:,1] = y[:,0] * boxSize / L + boxSize / (2*L)
-coords[:,2] = x[:,0] * boxSize / L + boxSize / (2*L)
-ds = grp.create_dataset('Coordinates', (numPart, 3), 'd')
-ds[()] = coords
-
-file.close()

examples/IsothermalPotential/energy_plot.py

+import matplotlib
+matplotlib.use("Agg")
+from pylab import *
+import h5py
+
+# Plot parameters
+params = {'axes.labelsize': 10,
+'axes.titlesize': 10,
+'font.size': 12,
+'legend.fontsize': 12,
+'xtick.labelsize': 10,
+'ytick.labelsize': 10,
+'text.usetex': True,
+ 'figure.figsize' : (3.15,3.15),
+'figure.subplot.left'    : 0.145,
+'figure.subplot.right'   : 0.99,
+'figure.subplot.bottom'  : 0.11,