def _plot_time_range(times, figname):
for i, t in enumerate(times):
vlab.clf()
cotr = Cotr(t)
vlab.plot_blue_marble(r=1.0, rotate=t, crd_system=crd_system,
nphi=256, ntheta=128, res=4, lines=True)
vlab.plot_earth_3d(radius=1.005, crd_system=crd_system,
night_only=True, opacity=0.5)
mag_north = cotr.transform('sm', crd_system, [0, 0, 1.0])
vlab.mlab.points3d(*mag_north, scale_factor=0.05, mode='sphere',
color=(0.992, 0.455, 0.0), resolution=32)
vlab.orientation_axes(line_width=4.0)
vlab.mlab.text(0.325, 0.95, viscid.format_datetime(t))
vlab.view(azimuth=0.0, elevation=90.0, distance=5.0,
focalpoint=[0, 0, 0])
vlab.savefig("{0}_eq_{1:06d}.png".format(figname, i))
vlab.view(azimuth=0.0, elevation=0.0, distance=5.0,
focalpoint=[0, 0, 0])
vlab.savefig("{0}_pole_{1:06d}.png".format(figname, i))
def _main():
try:
# raise ImportError
from viscid.plot import vlab
_HAS_MVI = True
except ImportError:
_HAS_MVI = False
def _test(_p1, _p2, r1=None, r2=None, color=(0.8, 0.8, 0.8)):
if r1 is not None:
_p1 = r1 * np.asarray(_p1) / np.linalg.norm(_p1)
if r2 is not None:
_p2 = r2 * np.asarray(_p2) / np.linalg.norm(_p2)
circ = great_circle(_p1, _p2)
if not np.all(np.isclose(circ[:, 0], _p1)):
print("!! great circle error P1:", _p1, ", P2:", _p2)
print(" first_point:", circ[:, 0], "!= P1")
if not np.all(np.isclose(circ[:, -1], _p2)):
print("!! great circle error P1:", _p1, ", P2:", _p2)
print(" last_point:", circ[:, -1], "!= P2")
if _HAS_MVI:
vlab.plot_lines([circ], tube_radius=0.02, color=color)
print("TEST 1")
_test([1, 0, 0], [0, 1, 0], r1=1.0, r2=1.0, color=(0.8, 0.8, 0.2))
print("TEST 2")
_test([1, 0, 0], [-1, 0, 0], r1=1.0, r2=1.0, color=(0.2, 0.8, 0.8))
print("TEST 3")
_test([1, 1, 0.01], [-1, -1, 0.01], r1=1.0, r2=1.5, color=(0.8, 0.2, 0.8))
print("TEST 4")
_test([-0.9947146, 1.3571029, 2.6095123],
[-0.3371437, -1.5566425, 2.6634643],
color=(0.8, 0.2, 0.2))
print("TEST 5")
_test([0.9775307, -1.3741084, 2.6030273],
[0.3273931, 1.5570284, 2.6652965],
color=(0.2, 0.2, 0.8))
if _HAS_MVI:
vlab.plot_blue_marble(r=1.0, lines=False, ntheta=64, nphi=128)
vlab.plot_earth_3d(radius=1.01, night_only=True, opacity=0.5)
vlab.show()
return 0
def _main():
try:
# raise ImportError
from viscid.plot import vlab
_HAS_MVI = True
except ImportError:
_HAS_MVI = False
def _test(_p1, _p2, r1=None, r2=None, color=(0.8, 0.8, 0.8)):
if r1 is not None:
_p1 = r1 * np.asarray(_p1) / np.linalg.norm(_p1)
if r2 is not None:
_p2 = r2 * np.asarray(_p2) / np.linalg.norm(_p2)
circ = great_circle(_p1, _p2)
if not np.all(np.isclose(circ[:, 0], _p1)):
print("!! great circle error P1:", _p1, ", P2:", _p2)
print(" first_point:", circ[:, 0], "!= P1")
if not np.all(np.isclose(circ[:, -1], _p2)):
print("!! great circle error P1:", _p1, ", P2:", _p2)
print(" last_point:", circ[:, -1], "!= P2")
if _HAS_MVI:
vlab.plot_lines([circ], tube_radius=0.02, color=color)
print("TEST 1")
_test([1, 0, 0], [0, 1, 0], r1=1.0, r2=1.0, color=(0.8, 0.8, 0.2))
print("TEST 2")
_test([1, 0, 0], [-1, 0, 0], r1=1.0, r2=1.0, color=(0.2, 0.8, 0.8))
print("TEST 3")
_test([1, 1, 0.01], [-1, -1, 0.01], r1=1.0, r2=1.5, color=(0.8, 0.2, 0.8))
print("TEST 4")
_test([-0.9947146, 1.3571029, 2.6095123], [-0.3371437, -1.5566425, 2.6634643],
color=(0.8, 0.2, 0.2))
print("TEST 5")
_test([0.9775307, -1.3741084, 2.6030273], [0.3273931, 1.5570284, 2.6652965],
color=(0.2, 0.2, 0.8))
if _HAS_MVI:
vlab.plot_blue_marble(r=1.0, lines=False, ntheta=64, nphi=128)
vlab.plot_earth_3d(radius=1.01, night_only=True, opacity=0.5)
vlab.show()
return 0
def _plot_time_range(times, figname):
for i, t in enumerate(times):
vlab.clf()
cotr = Cotr(t)
vlab.plot_blue_marble(r=1.0,
rotate=t,
crd_system=crd_system,
nphi=256,
ntheta=128,
res=4,
lines=True)
vlab.plot_earth_3d(radius=1.005,
crd_system=crd_system,
night_only=True,
opacity=0.5)
mag_north = cotr.transform('sm', crd_system, [0, 0, 1.0])
vlab.mlab.points3d(*mag_north,
scale_factor=0.05,
mode='sphere',
color=(0.992, 0.455, 0.0),
resolution=32)
vlab.orientation_axes(line_width=4.0)
vlab.mlab.text(0.325, 0.95, viscid.format_datetime(t))
vlab.view(azimuth=0.0,
elevation=90.0,
distance=5.0,
focalpoint=[0, 0, 0])
vlab.savefig("{0}_eq_{1:06d}.png".format(figname, i))
vlab.view(azimuth=0.0,
elevation=0.0,
distance=5.0,
focalpoint=[0, 0, 0])
vlab.savefig("{0}_pole_{1:06d}.png".format(figname, i))
def _main():
parser = argparse.ArgumentParser(description=__doc__)
parser.add_argument("--notwo", dest='notwo', action="store_true")
parser.add_argument("--nothree", dest='nothree', action="store_true")
parser.add_argument("--show", "--plot", action="store_true")
args = viscid.vutil.common_argparse(parser, default_verb=0)
plot2d = not args.notwo
plot3d = not args.nothree
# plot2d = True
# plot3d = True
# args.show = True
img = np.load(os.path.join(sample_dir, "logo.npy"))
x = np.linspace(-1, 1, img.shape[0])
y = np.linspace(-1, 1, img.shape[1])
z = np.linspace(-1, 1, img.shape[2])
logo = viscid.arrays2field([x, y, z], img)
if 1:
viscid.logger.info('Testing Point with custom local coordinates...')
pts = np.vstack([[-1, -0.5, 0, 0.5, 1],
[-1, -0.5, 0, 0.5, 1],
[ 0, 0.5, 1, 1.5, 2]])
local_crds = viscid.asarray_datetime64([0, 60, 120, 180, 240],
conservative=True)
seeds = viscid.Point(pts, local_crds=local_crds)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Line...')
seeds = viscid.Line([-1, -1, 0], [1, 1, 2], n=5)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Plane...')
seeds = viscid.Plane([0.0, 0.0, 0.0], [1, 1, 1], [1, 0, 0], 2, 2,
nl=160, nm=170, NL_are_vectors=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Volume...')
seeds = viscid.Volume([-0.8, -0.8, -0.8], [0.8, 0.8, 0.8],
n=[64, 64, 3])
# note: can't make a 2d plot of the volume w/o a slice
run_test(logo, seeds, plot2d=False, plot3d=plot3d, add_title="3d",
show=args.show)
if 1:
viscid.logger.info('Testing Volume (with ignorable dim)...')
seeds = viscid.Volume([-0.8, -0.8, 0.0], [0.8, 0.8, 0.0],
n=[64, 64, 1])
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="2d",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (phi, theta)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (theta, phi)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (phi, theta)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (theta, phi)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Patch...')
seeds = viscid.SphericalPatch(p0=[0, 0, 0], p1=[0, -0, -1],
max_alpha=30.0, max_beta=59.9,
nalpha=65, nbeta=80, r=0.5, roll=45.0)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
# this spline test is very custom
viscid.logger.info('Testing Spline...')
try:
import scipy.interpolate as interpolate
except ImportError:
msg = "XFail: ImportError (is scipy installed?)"
if plot2d:
try:
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
plt.clf()
plt.annotate(msg, xy=(0.3, 0.4), xycoords='axes fraction')
plt.savefig(next_plot_fname(__file__, series='2d'))
plt.savefig(next_plot_fname(__file__, series='2d'))
plt.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
plt.show()
except ImportError:
pass
else:
knots = np.array([[ 0.2, 0.5, 0.0], [-0.2, 0.5, 0.2],
[-0.2, 0.0, 0.4], [ 0.2, 0.0, 0.2],
[ 0.2, -0.5, 0.0], [-0.2, -0.5, 0.2]]).T
seed_name = "Spline"
fld = logo
seeds = viscid.Spline(knots)
seed_pts = seeds.get_points()
interp_fld = viscid.interp_trilin(fld, seeds)
if plot2d:
try:
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
plt.clf()
vlt.plot(interp_fld)
plt.title(seed_name)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
plt.show()
plt.clf()
from matplotlib import rcParams
_ms = rcParams['lines.markersize']
plt.gca().scatter(knots[0, :], knots[1, :],
s=(2 * _ms)**2, marker='^', color='y')
plt.gca().scatter(seed_pts[0, :], seed_pts[1, :],
s=(1.5 * _ms)**2, marker='o', color='k')
vlt.plot2d_line(seed_pts, scalars=interp_fld.flat_data,
symdir='z')
plt.title(seed_name)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
plt.show()
except ImportError:
pass
if plot3d:
try:
from viscid.plot import vlab
_ = get_mvi_fig(offscreen=not args.show)
vlab.points3d(knots[0], knots[1], knots[2],
color=(1.0, 1.0, 0), scale_mode='none',
scale_factor=0.04)
p = vlab.points3d(seed_pts[0], seed_pts[1], seed_pts[2],
color=(0, 0, 0), scale_mode='none',
scale_factor=0.03)
vlab.plot_line(seed_pts, scalars=interp_fld.flat_data,
tube_radius=0.01)
vlab.axes(p)
vlab.title(seed_name)
vlab.mlab.roll(-90.0)
vlab.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
vlab.show(stop=True)
except ImportError:
pass
if 1:
viscid.logger.info('Testing RectilinearMeshPoints...')
f = viscid.load_file(os.path.join(sample_dir, 'sample_xdmf.3d.[-1].xdmf'))
slc = 'x=-40j:12j, y=-10j:10j, z=-10j:10j'
b = f['b'][slc]
z = b.get_crd('z')
sheet_iz = np.argmin(b['x']**2, axis=2)
sheet_pts = b['z=0:1'].get_points()
sheet_pts[2, :] = z[sheet_iz].reshape(-1)
isphere_mask = np.sum(sheet_pts[:2, :]**2, axis=0) < 5**2
day_mask = sheet_pts[0:1, :] > -1.0
sheet_pts[2, :] = np.choose(isphere_mask, [sheet_pts[2, :], 0])
sheet_pts[2, :] = np.choose(day_mask, [sheet_pts[2, :], 0])
nx, ny, _ = b.sshape
sheet_seed = viscid.RectilinearMeshPoints(sheet_pts.reshape(3, nx, ny))
vx_sheet = viscid.interp_nearest(f['vx'], sheet_seed)
try:
if not plot2d:
raise ImportError
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
vlt.clf()
vlt.plot(vx_sheet, symmetric=True)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
vlt.show()
except ImportError:
pass
try:
if not plot3d:
raise ImportError
from viscid.plot import vlab
_ = get_mvi_fig(offscreen=not args.show)
mesh = vlab.mesh_from_seeds(sheet_seed, scalars=vx_sheet,
clim=(-400, 400))
vlab.plot_earth_3d(crd_system=b)
vlab.view(azimuth=+90.0 + 45.0, elevation=90.0 - 25.0,
distance=30.0, focalpoint=(-10.0, +1.0, +1.0))
vlab.title("RectilinearMeshPoints")
vlab.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
vlab.show(stop=True)
except ImportError:
pass
# prevent weird xorg bad-instructions on tear down
if 'figure' in _global_ns and _global_ns['figure'] is not None:
from viscid.plot import vlab
vlab.mlab.close(_global_ns['figure'])
return 0
def _main():
parser = argparse.ArgumentParser(description=__doc__)
parser.add_argument("--show", "--plot", action="store_true")
parser.add_argument("--interact", "-i", action="store_true")
args = vutil.common_argparse(parser)
f3d = viscid.load_file(os.path.join(sample_dir, 'sample_xdmf.3d.[0].xdmf'))
f_iono = viscid.load_file(os.path.join(sample_dir, "sample_xdmf.iof.[0].xdmf"))
b = f3d["b"]
v = f3d["v"]
pp = f3d["pp"]
e = f3d["e_cc"]
vlab.figure(size=(1280, 800), offscreen=not args.show)
##########################################################
# make b a dipole inside 3.1Re and set e = 0 inside 4.0Re
cotr = viscid.Cotr(time='1990-03-21T14:48', dip_tilt=0.0) # pylint: disable=not-callable
moment = cotr.get_dipole_moment(crd_system=b)
isphere_mask = viscid.make_spherical_mask(b, rmax=3.1)
viscid.fill_dipole(b, m=moment, mask=isphere_mask)
e_mask = viscid.make_spherical_mask(b, rmax=4.0)
viscid.set_in_region(e, 0.0, alpha=0.0, mask=e_mask, out=e)
######################################
# plot a scalar cut plane of pressure
pp_src = vlab.field2source(pp, center='node')
scp = vlab.scalar_cut_plane(pp_src, plane_orientation='z_axes', opacity=0.5,
transparent=True, view_controls=False,
cmap="inferno", logscale=True)
scp.implicit_plane.normal = [0, 0, -1]
scp.implicit_plane.origin = [0, 0, 0]
scp.enable_contours = True
scp.contour.filled_contours = True
scp.contour.number_of_contours = 64
cbar = vlab.colorbar(scp, title=pp.name, orientation='vertical')
cbar.scalar_bar_representation.position = (0.01, 0.13)
cbar.scalar_bar_representation.position2 = (0.08, 0.76)
######################################
# plot a vector cut plane of the flow
vcp = vlab.vector_cut_plane(v, scalars=pp_src, plane_orientation='z_axes',
view_controls=False, mode='arrow',
cmap='Greens_r')
vcp.implicit_plane.normal = [0, 0, -1]
vcp.implicit_plane.origin = [0, 0, 0]
##############################
# plot very faint isosurfaces
vx_src = vlab.field2source(v['x'], center='node')
iso = vlab.iso_surface(vx_src, contours=[0.0], opacity=0.008, cmap='Pastel1')
##############################################################
# calculate B field lines && topology in Viscid and plot them
seedsA = viscid.SphericalPatch([0, 0, 0], [2, 0, 1], 30, 15, r=5.0,
nalpha=5, nbeta=5)
seedsB = viscid.SphericalPatch([0, 0, 0], [1.9, 0, -20], 30, 15, r=5.0,
nalpha=1, nbeta=5)
seeds = np.concatenate([seedsA, seedsB], axis=1)
b_lines, topo = viscid.calc_streamlines(b, seeds, ibound=3.5,
obound0=[-25, -20, -20],
obound1=[15, 20, 20], wrap=True)
vlab.plot_lines(b_lines, scalars=viscid.topology2color(topo))
######################################################################
# plot a random circle at geosynchronus orbit with scalars colored
# by the Matplotlib viridis color map, just because we can; this is
# a useful toy for debugging
circle = viscid.Circle(p0=[0, 0, 0], r=6.618, n=128, endpoint=True)
scalar = np.sin(circle.as_local_coordinates().get_crd('phi'))
surf = vlab.plot_line(circle.get_points(), scalars=scalar, clim=0.8,
cmap="Spectral_r")
######################################################################
# Use Mayavi (VTK) to calculate field lines using an interactive seed
# These field lines are colored by E parallel
epar = viscid.project(e, b)
epar.name = "Epar"
bsl2 = vlab.streamline(b, epar, seedtype='plane', seed_resolution=4,
integration_direction='both', clim=(-0.05, 0.05))
# now tweak the VTK streamlines
bsl2.stream_tracer.maximum_propagation = 20.
bsl2.seed.widget.origin = [-11, -5.0, -2.0]
bsl2.seed.widget.point1 = [-11, 5.0, -2.0]
bsl2.seed.widget.point2 = [-11.0, -5.0, 2.0]
bsl2.streamline_type = 'tube'
bsl2.tube_filter.radius = 0.03
bsl2.stop() # this stop/start was a hack to get something to update
bsl2.start()
bsl2.seed.widget.enabled = False
cbar = vlab.colorbar(bsl2, title=epar.name, label_fmt='%.3f',
orientation='horizontal')
cbar.scalar_bar_representation.position = (0.15, 0.01)
cbar.scalar_bar_representation.position2 = (0.72, 0.10)
###############################################################
# Make a contour at the open-closed boundary in the ionosphere
seeds_iono = viscid.Sphere(r=1.063, pole=-moment, ntheta=256, nphi=256,
thetalim=(0, 180), philim=(0, 360), crd_system=b)
_, topo_iono = viscid.calc_streamlines(b, seeds_iono, ibound=1.0,
nr_procs='all',
output=viscid.OUTPUT_TOPOLOGY)
topo_iono = np.log2(topo_iono)
m = vlab.mesh_from_seeds(seeds_iono, scalars=topo_iono, opacity=1.0,
clim=(0, 3), color=(0.992, 0.445, 0.0))
m.enable_contours = True
m.actor.property.line_width = 4.0
m.contour.number_of_contours = 4
####################################################################
# Plot the ionosphere, note that the sample data has the ionosphere
# at a different time, so the open-closed boundary found above
# will not be consistant with the field aligned currents
fac_tot = 1e9 * f_iono['fac_tot']
m = vlab.plot_ionosphere(fac_tot, bounding_lat=30.0, vmin=-300, vmax=300,
opacity=0.75, rotate=cotr, crd_system=b)
m.actor.property.backface_culling = True
########################################################################
# Add some markers for earth, i.e., real earth, and dayside / nightside
# representation
vlab.plot_blue_marble(r=1.0, lines=False, ntheta=64, nphi=128,
rotate=cotr, crd_system=b)
# now shade the night side with a transparent black hemisphere
vlab.plot_earth_3d(radius=1.01, night_only=True, opacity=0.5, crd_system=b)
####################
# Finishing Touches
# vlab.axes(pp_src, nb_labels=5)
oa = vlab.orientation_axes()
oa.marker.set_viewport(0.75, 0.75, 1.0, 1.0)
# note that resize won't work if the current figure has the
# off_screen_rendering flag set
# vlab.resize([1200, 800])
vlab.view(azimuth=45, elevation=70, distance=35.0, focalpoint=[-2, 0, 0])
##############
# Save Figure
# print("saving png")
# vlab.savefig('mayavi_msphere_sample.png')
# print("saving x3d")
# # x3d files can be turned into COLLADA files with meshlab, and
# # COLLADA (.dae) files can be opened in OS X's preview
# #
# # IMPORTANT: for some reason, using bounding_lat in vlab.plot_ionosphere
# # causes a segfault when saving x3d files
# #
# vlab.savefig('mayavi_msphere_sample.x3d')
# print("done")
vlab.savefig(next_plot_fname(__file__))
###########################
# Interact Programatically
if args.interact:
vlab.interact()
#######################
# Interact Graphically
if args.show:
vlab.show()
try:
vlab.mlab.close()
except AttributeError:
pass
return 0
def _main():
global offscreen_vlab
parser = argparse.ArgumentParser(description=__doc__)
parser.add_argument("--notwo", dest='notwo', action="store_true")
parser.add_argument("--nothree", dest='nothree', action="store_true")
parser.add_argument("--show", "--plot", action="store_true")
args = viscid.vutil.common_argparse(parser, default_verb=0)
plot2d = not args.notwo
plot3d = not args.nothree
# plot2d = True
# plot3d = True
# args.show = True
offscreen_vlab = not args.show
img = np.load(os.path.join(sample_dir, "logo.npy"))
x = np.linspace(-1, 1, img.shape[0])
y = np.linspace(-1, 1, img.shape[1])
z = np.linspace(-1, 1, img.shape[2])
logo = viscid.arrays2field([x, y, z], img)
if 1:
viscid.logger.info('Testing Point with custom local coordinates...')
pts = np.vstack([[-1, -0.5, 0, 0.5, 1],
[-1, -0.5, 0, 0.5, 1],
[ 0, 0.5, 1, 1.5, 2]])
local_crds = viscid.asarray_datetime64([0, 60, 120, 180, 240],
conservative=True)
seeds = viscid.Point(pts, local_crds=local_crds)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Line...')
seeds = viscid.Line([-1, -1, 0], [1, 1, 2], n=5)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Plane...')
seeds = viscid.Plane([0.0, 0.0, 0.0], [1, 1, 1], [1, 0, 0], 2, 2,
nl=160, nm=170, NL_are_vectors=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Volume...')
seeds = viscid.Volume([-0.8, -0.8, -0.8], [0.8, 0.8, 0.8],
n=[64, 64, 3])
# note: can't make a 2d plot of the volume w/o a slice
run_test(logo, seeds, plot2d=False, plot3d=plot3d, add_title="3d",
show=args.show)
if 1:
viscid.logger.info('Testing Volume (with ignorable dim)...')
seeds = viscid.Volume([-0.8, -0.8, 0.0], [0.8, 0.8, 0.0],
n=[64, 64, 1])
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="2d",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (phi, theta)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (theta, phi)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (phi, theta)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (theta, phi)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Patch...')
seeds = viscid.SphericalPatch(p0=[0, 0, 0], p1=[0, -0, -1],
max_alpha=30.0, max_beta=59.9,
nalpha=65, nbeta=80, r=0.5, roll=45.0)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
# this spline test is very custom
viscid.logger.info('Testing Spline...')
try:
import scipy.interpolate as interpolate
except ImportError:
msg = "XFail: ImportError (is scipy installed?)"
if plot2d:
try:
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
plt.clf()
plt.annotate(msg, xy=(0.3, 0.4), xycoords='axes fraction')
plt.savefig(next_plot_fname(__file__, series='2d'))
plt.savefig(next_plot_fname(__file__, series='2d'))
plt.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
plt.show()
except ImportError:
pass
else:
knots = np.array([[ 0.2, 0.5, 0.0], [-0.2, 0.5, 0.2],
[-0.2, 0.0, 0.4], [ 0.2, 0.0, 0.2],
[ 0.2, -0.5, 0.0], [-0.2, -0.5, 0.2]]).T
seed_name = "Spline"
fld = logo
seeds = viscid.Spline(knots)
seed_pts = seeds.get_points()
interp_fld = viscid.interp_trilin(fld, seeds)
if plot2d:
try:
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
plt.clf()
vlt.plot(interp_fld)
plt.title(seed_name)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
plt.show()
plt.clf()
from matplotlib import rcParams
_ms = rcParams['lines.markersize']
plt.gca().scatter(knots[0, :], knots[1, :],
s=(2 * _ms)**2, marker='^', color='y')
plt.gca().scatter(seed_pts[0, :], seed_pts[1, :],
s=(1.5 * _ms)**2, marker='o', color='k')
vlt.plot2d_line(seed_pts, scalars=interp_fld.flat_data,
symdir='z')
plt.title(seed_name)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
plt.show()
except ImportError:
pass
if plot3d:
try:
vlab, _ = get_mvi_fig()
vlab.points3d(knots[0], knots[1], knots[2],
color=(1.0, 1.0, 0), scale_mode='none',
scale_factor=0.04)
p = vlab.points3d(seed_pts[0], seed_pts[1], seed_pts[2],
color=(0, 0, 0), scale_mode='none',
scale_factor=0.03)
vlab.plot_line(seed_pts, scalars=interp_fld.flat_data,
tube_radius=0.01)
vlab.axes(p)
vlab.title(seed_name)
vlab.mlab.roll(-90.0)
vlab.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
vlab.show(stop=True)
except ImportError:
pass
if 1:
viscid.logger.info('Testing RectilinearMeshPoints...')
f = viscid.load_file(os.path.join(sample_dir, 'sample_xdmf.3d.[-1].xdmf'))
slc = 'x=-40j:12j, y=-10j:10j, z=-10j:10j'
b = f['b'][slc]
z = b.get_crd('z')
sheet_iz = np.argmin(b['x']**2, axis=2)
sheet_pts = b['z=0:1'].get_points()
sheet_pts[2, :] = z[sheet_iz].reshape(-1)
isphere_mask = np.sum(sheet_pts[:2, :]**2, axis=0) < 5**2
day_mask = sheet_pts[0:1, :] > -1.0
sheet_pts[2, :] = np.choose(isphere_mask, [sheet_pts[2, :], 0])
sheet_pts[2, :] = np.choose(day_mask, [sheet_pts[2, :], 0])
nx, ny, _ = b.sshape
sheet_seed = viscid.RectilinearMeshPoints(sheet_pts.reshape(3, nx, ny))
vx_sheet = viscid.interp_nearest(f['vx'], sheet_seed)
try:
if not plot2d:
raise ImportError
from viscid.plot import vpyplot as vlt
from matplotlib import pyplot as plt
vlt.clf()
vlt.plot(vx_sheet, symmetric=True)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
vlt.show()
except ImportError:
pass
try:
if not plot3d:
raise ImportError
vlab, _ = get_mvi_fig()
mesh = vlab.mesh_from_seeds(sheet_seed, scalars=vx_sheet,
clim=(-400, 400))
vlab.plot_earth_3d(crd_system=b)
vlab.view(azimuth=+90.0 + 45.0, elevation=90.0 - 25.0,
distance=30.0, focalpoint=(-10.0, +1.0, +1.0))
vlab.title("RectilinearMeshPoints")
vlab.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
vlab.show(stop=True)
except ImportError:
pass
# prevent weird xorg bad-instructions on tear down
if 'figure' in _global_ns and _global_ns['figure'] is not None:
from viscid.plot import vlab
vlab.mlab.close(_global_ns['figure'])
return 0
def trace_separator(grid,
b_slcstr="x=-25f:15f, y=-30f:30f, z=-15f:15f",
r=1.0,
plot=False,
trace_opts=None,
cache=True,
cache_dir=None):
"""Trace a separator line from most dawnward null
**Still in testing** Uses the bisection algorithm.
Args:
grid (Grid): A grid that has a "b" field
b_slcstr (str): Some valid slice for B field
r (float): spatial step of separator line
plot (bool): make debugging plots
trace_opts (dict): passed to streamline function
cache (bool, str): Save to and load from cache, if "force",
then don't load from cache if it exists, but do save a
cache at the end
cache_dir (str): Directory for cache, if None, same directory
as that file to which the grid belongs
Raises:
IOError: Description
Returns:
tuple: (separator_lines, nulls)
- **separator_lines** (list): list of M 3xN ndarrays that
represent M separator lines with N points
- **nulls** (ndarray): 3xN array of N null points
"""
if not cache_dir:
cache_dir = grid.find_info("_viscid_dirname", "./")
run_name = grid.find_info("run")
sep_fname = "{0}/{1}.sep.{2:06.0f}".format(cache_dir, run_name, grid.time)
try:
if isinstance(cache,
string_types) and cache.strip().lower() == "force":
raise IOError()
with np.load(sep_fname + ".npz") as dat:
sep_iter = (f for f in dat.files if f.startswith("arr_"))
_it = sorted(sep_iter, key=lambda s: int(s[len("arr_"):]))
seps = [dat[n] for n in _it]
nulls = dat['nulls']
except IOError:
_b = grid['b'][b_slcstr]
_, nulls = viscid.find_nulls(_b['x=-30f:15f'], ibound=5.0)
# get most dawnward null, nulls2 is all nulls except p0
nullind = np.argmin(nulls[1, :])
p0 = nulls[:, nullind]
nulls2 = np.concatenate([nulls[:, :nullind], nulls[:, (nullind + 1):]],
axis=1)
if plot:
from viscid.plot import vlab
vlab.plot_earth_3d(crd_system='gse')
vlab.points3d(nulls2[0],
nulls2[1],
nulls2[2],
color=(0, 0, 0),
scale_factor=1.0)
vlab.points3d(nulls[0, nullind],
nulls[1, nullind],
nulls[2, nullind],
color=(1, 1, 1),
scale_factor=1.0)
seed = viscid.Sphere(p0=p0,
r=r,
ntheta=30,
nphi=60,
theta_endpoint=True,
phi_endpoint=True)
p1 = viscid.get_sep_pts_bisect(_b,
seed,
max_depth=12,
plot=plot,
trace_opts=trace_opts)
# print("p1 shape", p1.shape)
# if p1.shape[1] > 2:
# raise RuntimeError("Invalid B field, should be no branch @ null")
seps = []
sep_stubs = []
for i in range(p1.shape[1]):
sep_stubs.append([p0, p1[:, i]])
# print("??", sep_stubs)
while sep_stubs:
sep = sep_stubs.pop(0)
# print("!!! new stub")
for i in count():
# print("::", i)
seed = viscid.SphericalPatch(p0=sep[-1],
p1=sep[-1] - sep[-2],
r=r,
nalpha=240,
nbeta=240)
pn = viscid.get_sep_pts_bisect(_b,
seed,
max_depth=8,
plot=plot,
trace_opts=trace_opts)
if pn.shape[1] == 0:
# print("END: pn.shape[1] == 0")
break
# print("++", nulls2.shape, pn.shape)
closest_null_dist = np.min(
np.linalg.norm(nulls2 - pn[:, :1], axis=0))
# print("closest_null_dist:", closest_null_dist)
if closest_null_dist < 1.01 * r:
# print("END: within 1.01 of a null")
break
# print("??", pn)
for j in range(1, pn.shape[1]):
# print("inserting new stub")
sep_stubs.insert(0, [sep[-1], pn[:, j]])
sep.append(pn[:, 0])
# print("sep", sep)
seps.append(np.stack(sep, axis=1))
if cache:
np.savez_compressed(sep_fname, *seps, nulls=nulls)
return seps, nulls
def main():
mhd_type = "C"
make_plots = 1
mhd_type = mhd_type.upper()
if mhd_type.startswith("C"):
if mhd_type in ("C",):
f = viscid.load_file("$WORK/tmedium/*.3d.[-1].xdmf")
elif mhd_type in ("C2", "C3"):
f = viscid.load_file("$WORK/tmedium2/*.3d.[-1].xdmf")
else:
raise ValueError()
catol = 1e-8
rtol = 2e-6
elif mhd_type in ("F", "FORTRAN"):
f = viscid.load_file("$WORK/tmedium3/*.3df.[-1]")
catol = 1e-8
rtol = 7e-2
else:
raise ValueError()
do_fill_dipole = True
gslc = "x=-21.2j:12j, y=-11j:11j, z=-11j:11j"
b = f['b_cc'][gslc]
b1 = f['b_fc'][gslc]
e_cc = f['e_cc'][gslc]
e_ec = f['e_ec'][gslc]
if do_fill_dipole:
mask = viscid.make_spherical_mask(b, rmax=3.5)
viscid.fill_dipole(b, mask=mask)
mask = viscid.make_spherical_mask(b1, rmax=3.5)
viscid.fill_dipole(b1, mask=mask)
mask = None
# seeds = viscid.SphericalCap(r=1.02, ntheta=64, nphi=32, angle0=17, angle=20,
# philim=(100, 260), roll=-180.0)
# seeds = viscid.SphericalCap(r=1.02, ntheta=64, nphi=32, angle0=17, angle=20,
# philim=(0, 10), roll=0.0)
seedsN = viscid.Sphere(r=1.02, ntheta=16, nphi=16, thetalim=(15, 25),
philim=(0, 300), crd_system=b)
seedsS = viscid.Sphere(r=1.02, ntheta=16, nphi=16, thetalim=(155, 165),
philim=(0, 300), crd_system=b)
bl_kwargs = dict(ibound=0.9, obound0=(-20, -10, -10), obound1=(11, 10, 10))
# blines_cc, topo_cc = viscid.streamlines(b, seeds, **bl_kwargs)
blinesN_fc, topoN_fc = viscid.streamlines(b1, seedsN, **bl_kwargs)
_, topoS_fc = viscid.streamlines(b1, seedsS, output=viscid.OUTPUT_TOPOLOGY,
**bl_kwargs)
if True:
from viscid.plot import vlab
mesh = vlab.mesh_from_seeds(seedsN, scalars=topoN_fc)
mesh.actor.property.backface_culling = True
# vlab.plot_lines(blines_cc, scalars="#000000", tube_radius=0.03)
vlab.plot_lines(blinesN_fc, scalars=viscid.topology2color(topoN_fc),
opacity=0.7)
vlab.plot_blue_marble(r=1.0)
vlab.plot_earth_3d(radius=1.01, crd_system=b, night_only=True,
opacity=0.5)
vlab.show()
if True:
vlt.subplot(121, projection='polar')
vlt.plot(topoN_fc)
vlt.subplot(122, projection='polar')
vlt.plot(topoS_fc)
vlt.show()
return 0
def _main():
f = viscid.load_file('~/dev/work/xi_fte_001/*.3d.*.xdmf')
time_slice = ':'
times = np.array([grid.time for grid in f.iter_times(time_slice)])
# XYZ coordinates of virtual satelites in warped "plasma sheet coords"
x_sat_psc = np.linspace(-30, 0, 31) # X (GSE == PSC)
y_sat_psc = np.linspace(-10, 10, 21) # Y (GSE == PSC)
z_sat_psc = np.linspace(-2, 2, 5) # Z in PSC (z=0 is the plasma sheet)
# the GSE z location of the virtual satelites in the warped plasma sheet
# coordinates, so sat_z_gse_ts['x=5j, y=1j, z=0j'] would give the
# plasma sheet location at x=5.0, y=1.0
# These fields depend on time because the plasma sheet moves in time
sat_z_gse_ts = viscid.zeros([times, x_sat_psc, y_sat_psc, z_sat_psc],
crd_names='txyz', center='node',
name='PlasmaSheetZ_GSE')
vx_ts = viscid.zeros_like(sat_z_gse_ts)
bz_ts = viscid.zeros_like(sat_z_gse_ts)
for itime, grid in enumerate(f.iter_times(time_slice)):
print("Processing time slice", itime, grid.time)
gse_slice = 'x=-35j:0j, y=-15j:15j, z=-6j:6j'
bx = grid['bx'][gse_slice]
bx_argmin = np.argmin(bx**2, axis=2)
z_gse = bx.get_crd('z')
# ps_zloc_gse is the plasma sheet z location along the GGCM grid x/y
ps_z_gse = viscid.zeros_like(bx[:, :, 0:1])
ps_z_gse[...] = z_gse[bx_argmin]
# Note: Here you could apply a gaussian filter to
# ps_z_gse[:, :, 0].data in order to smooth the surface
# if desired. Scipy / Scikit-Image have some functions
# that do this
# ok, we found the plasma sheet z GSE location on the actual GGCM
# grid, but we just want a subset of that grid for our virtual
# satelites, so just interpolate the ps z location to our subset
ps_z_gse_subset = viscid.interp_trilin(ps_z_gse,
sat_z_gse_ts[itime, :, :, 0:1],
wrap=True)
# now we know the plasma sheet z location in GSE, and how far
# apart we want the satelites in z, so put those two things together
# to get a bunch of satelite locations
sat_z_gse_ts[itime] = ps_z_gse_subset.data + z_sat_psc.reshape(1, 1, -1)
# make a seed generator that we can use to fill the vx and bz
# time series for this instant in time
sat_loc_gse = sat_z_gse_ts[itime].get_points()
sat_loc_gse[2, :] = sat_z_gse_ts[itime].data.reshape(-1)
# slicing the field before doing the interpolation makes this
# faster for hdf5 data, but probably for other data too
vx_ts[itime] = viscid.interp_trilin(grid['vx'][gse_slice],
sat_loc_gse,
wrap=False
).reshape(vx_ts.shape[1:])
bz_ts[itime] = viscid.interp_trilin(grid['bz'][gse_slice],
sat_loc_gse,
wrap=False
).reshape(bz_ts.shape[1:])
# 2d plots of the plasma sheet z location to make sure we did the
# interpolation correctly
if False: # pylint: disable=using-constant-test
from viscid.plot import vpyplot as vlt
fig, (ax0, ax1) = vlt.subplots(2, 1) # pylint: disable=unused-variable
vlt.plot(ps_z_gse, ax=ax0, clim=(-5, 5))
vlt.plot(ps_z_gse_subset, ax=ax1, clim=(-5, 5))
vlt.auto_adjust_subplots()
vlt.show()
# make a 3d plot of the plasma sheet surface to verify that it
# makes sense
if True: # pylint: disable=using-constant-test
from viscid.plot import vlab
fig = vlab.figure(size=(1280, 800), bgcolor=(1, 1, 1),
fgcolor=(0, 0, 0))
vlab.clf()
# plot the plasma sheet coloured by vx
# Note: points closer to x = 0 are unsightly since the plasma
# sheet criteria starts to fall apart on the flanks, so
# just remove the first few rows
ps_z_gse_tail = ps_z_gse['x=:-2.25j']
ps_mesh_shape = [3, ps_z_gse_tail.shape[0], ps_z_gse_tail.shape[1]]
ps_pts = ps_z_gse_tail.get_points().reshape(ps_mesh_shape)
ps_pts[2, :, :] = ps_z_gse_tail[:, :, 0]
plasma_sheet = viscid.RectilinearMeshPoints(ps_pts)
ps_vx = viscid.interp_trilin(grid['vx'][gse_slice], plasma_sheet)
_ = vlab.mesh_from_seeds(plasma_sheet, scalars=ps_vx)
vx_clim = (-1400, 1400)
vx_cmap = 'viridis'
vlab.colorbar(title='Vx', clim=vx_clim, cmap=vx_cmap,
nb_labels=5)
# plot satelite locations as dots colored by Vx with the same
# limits and color as the plasma sheet mesh
sat3d = vlab.points3d(sat_loc_gse[0], sat_loc_gse[1], sat_loc_gse[2],
vx_ts[itime].data.reshape(-1),
scale_mode='none', scale_factor=0.2)
vlab.apply_cmap(sat3d, clim=vx_clim, cmap=vx_cmap)
# plot Earth for reference
cotr = viscid.Cotr(dip_tilt=0.0) # pylint: disable=not-callable
vlab.plot_blue_marble(r=1.0, lines=False, ntheta=64, nphi=128,
rotate=cotr, crd_system='mhd')
vlab.plot_earth_3d(radius=1.01, night_only=True, opacity=0.5,
crd_system='gse')
vlab.view(azimuth=45, elevation=70, distance=35.0,
focalpoint=[-9, 3, -1])
vlab.savefig('plasma_sheet_3d_{0:02d}.png'.format(itime))
vlab.show()
try:
vlab.mlab.close(fig)
except TypeError:
pass # this happens if the figure is already closed
# now do what we will with the time series... this is not a good
# presentation of this data, but you get the idea
from viscid.plot import vpyplot as vlt
fig, axes = vlt.subplots(4, 4, figsize=(12, 12))
for ax_row, yloc in zip(axes, np.linspace(-5, 5, len(axes))[::-1]):
for ax, xloc in zip(ax_row, np.linspace(4, 7, len(ax_row))):
vlt.plot(vx_ts['x={0}j, y={1}j, z=0j'.format(xloc, yloc)], ax=ax)
ax.set_ylabel('')
vlt.plt.title('x = {0:g}, y = {1:g}'.format(xloc, yloc))
vlt.plt.suptitle('Vx [km/s]')
vlt.auto_adjust_subplots()
vlt.show()
return 0
def _main():
parser = argparse.ArgumentParser(description=__doc__)
parser.add_argument("--notwo", dest='notwo', action="store_true")
parser.add_argument("--nothree", dest='nothree', action="store_true")
parser.add_argument("--show", "--plot", action="store_true")
args = viscid.vutil.common_argparse(parser, default_verb=0)
plot2d = not args.notwo
plot3d = not args.nothree
# plot2d = True
# plot3d = True
# args.show = True
img = np.load(os.path.join(sample_dir, "logo.npy"))
x = np.linspace(-1, 1, img.shape[0])
y = np.linspace(-1, 1, img.shape[1])
z = np.linspace(-1, 1, img.shape[2])
logo = viscid.arrays2field([x, y, z], img)
if 1:
viscid.logger.info('Testing Line...')
seeds = viscid.Line([-1, -1, 0], [1, 1, 2], n=5)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Plane...')
seeds = viscid.Plane([0.0, 0.0, 0.0], [1, 1, 1], [1, 0, 0], 2, 2,
nl=160, nm=170, NL_are_vectors=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing Volume...')
seeds = viscid.Volume([-0.8, -0.8, -0.8], [0.8, 0.8, 0.8],
n=[64, 64, 3])
# note: can't make a 2d plot of the volume w/o a slice
run_test(logo, seeds, plot2d=False, plot3d=plot3d, add_title="3d",
show=args.show)
if 1:
viscid.logger.info('Testing Volume (with ignorable dim)...')
seeds = viscid.Volume([-0.8, -0.8, 0.0], [0.8, 0.8, 0.0],
n=[64, 64, 1])
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="2d",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (phi, theta)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Sphere (theta, phi)...')
seeds = viscid.Sphere([0, 0, 0], r=1.0, ntheta=160, nphi=170,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (phi, theta)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=False)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="PT",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Cap (theta, phi)...')
seeds = viscid.SphericalCap(p0=[0, 0, 0], r=1.0, ntheta=64, nphi=80,
pole=[-1, -1, -1], theta_phi=True)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, add_title="TP",
view_kwargs=dict(azimuth=180, elevation=180), show=args.show)
if 1:
viscid.logger.info('Testing Spherical Patch...')
seeds = viscid.SphericalPatch(p0=[0, 0, 0], p1=[0, -0, -1],
max_alpha=30.0, max_beta=59.9,
nalpha=65, nbeta=80, r=0.5, roll=45.0)
run_test(logo, seeds, plot2d=plot2d, plot3d=plot3d, show=args.show)
if 1:
viscid.logger.info('Testing RectilinearMeshPoints...')
f = viscid.load_file(os.path.join(sample_dir, 'sample_xdmf.3d.[-1].xdmf'))
slc = 'x=-40f:12f, y=-10f:10f, z=-10f:10f'
b = f['b'][slc]
z = b.get_crd('z')
sheet_iz = np.argmin(b['x']**2, axis=2)
sheet_pts = b['z=0:1'].get_points()
sheet_pts[2, :] = z[sheet_iz].reshape(-1)
isphere_mask = np.sum(sheet_pts[:2, :]**2, axis=0) < 5**2
day_mask = sheet_pts[0:1, :] > -1.0
sheet_pts[2, :] = np.choose(isphere_mask, [sheet_pts[2, :], 0])
sheet_pts[2, :] = np.choose(day_mask, [sheet_pts[2, :], 0])
nx, ny, _ = b.sshape
sheet_seed = viscid.RectilinearMeshPoints(sheet_pts.reshape(3, nx, ny))
vx_sheet = viscid.interp_nearest(f['vx'], sheet_seed)
try:
if not plot2d:
raise ImportError
from matplotlib import pyplot as plt
from viscid.plot import vpyplot as vlt
vlt.clf()
vlt.plot(vx_sheet, symmetric=True)
plt.savefig(next_plot_fname(__file__, series='2d'))
if args.show:
vlt.show()
except ImportError:
pass
try:
if not plot3d:
raise ImportError
from viscid.plot import vlab
vlab.clf()
mesh = vlab.mesh_from_seeds(sheet_seed, scalars=vx_sheet,
clim=(-400, 400))
vlab.plot_earth_3d(crd_system=b)
vlab.view(azimuth=+90.0 + 45.0, elevation=90.0 - 25.0,
distance=30.0, focalpoint=(-10.0, +1.0, +1.0))
vlab.title("RectilinearMeshPoints")
vlab.savefig(next_plot_fname(__file__, series='3d'))
if args.show:
vlab.show()
except ImportError:
pass
# prevent weird xorg bad-instructions on tear down
if 'figure' in _global_ns and _global_ns['figure'] is not None:
from viscid.plot import vlab
vlab.mlab.close(_global_ns['figure'])
return 0
def _main():
parser = argparse.ArgumentParser(description=__doc__)
parser.add_argument("--show", "--plot", action="store_true")
parser.add_argument("--interact", "-i", action="store_true")
args = vutil.common_argparse(parser)
f3d = viscid.load_file(os.path.join(sample_dir, 'sample_xdmf.3d.[0].xdmf'))
f_iono = viscid.load_file(
os.path.join(sample_dir, "sample_xdmf.iof.[0].xdmf"))
b = f3d["b"]
v = f3d["v"]
pp = f3d["pp"]
e = f3d["e_cc"]
vlab.mlab.options.offscreen = not args.show
vlab.figure(size=(1280, 800))
##########################################################
# make b a dipole inside 3.1Re and set e = 0 inside 4.0Re
cotr = viscid.Cotr(time='1990-03-21T14:48', dip_tilt=0.0) # pylint: disable=not-callable
moment = cotr.get_dipole_moment(crd_system=b)
isphere_mask = viscid.make_spherical_mask(b, rmax=3.1)
viscid.fill_dipole(b, m=moment, mask=isphere_mask)
e_mask = viscid.make_spherical_mask(b, rmax=4.0)
viscid.set_in_region(e, 0.0, alpha=0.0, mask=e_mask, out=e)
######################################
# plot a scalar cut plane of pressure
pp_src = vlab.field2source(pp, center='node')
scp = vlab.scalar_cut_plane(pp_src,
plane_orientation='z_axes',
opacity=0.5,
transparent=True,
view_controls=False,
cmap="inferno",
logscale=True)
scp.implicit_plane.normal = [0, 0, -1]
scp.implicit_plane.origin = [0, 0, 0]
scp.enable_contours = True
scp.contour.filled_contours = True
scp.contour.number_of_contours = 64
cbar = vlab.colorbar(scp, title=pp.name, orientation='vertical')
cbar.scalar_bar_representation.position = (0.01, 0.13)
cbar.scalar_bar_representation.position2 = (0.08, 0.76)
######################################
# plot a vector cut plane of the flow
vcp = vlab.vector_cut_plane(v,
scalars=pp_src,
plane_orientation='z_axes',
view_controls=False,
mode='arrow',
cmap='Greens_r')
vcp.implicit_plane.normal = [0, 0, -1]
vcp.implicit_plane.origin = [0, 0, 0]
##############################
# plot very faint isosurfaces
vx_src = vlab.field2source(v['x'], center='node')
iso = vlab.iso_surface(vx_src,
contours=[0.0],
opacity=0.008,
cmap='Pastel1')
##############################################################
# calculate B field lines && topology in Viscid and plot them
seedsA = viscid.SphericalPatch([0, 0, 0], [2, 0, 1],
30,
15,
r=5.0,
nalpha=5,
nbeta=5)
seedsB = viscid.SphericalPatch([0, 0, 0], [1.9, 0, -20],
30,
15,
r=5.0,
nalpha=1,
nbeta=5)
seeds = np.concatenate([seedsA, seedsB], axis=1)
b_lines, topo = viscid.calc_streamlines(b,
seeds,
ibound=3.5,
obound0=[-25, -20, -20],
obound1=[15, 20, 20],
wrap=True)
vlab.plot_lines(b_lines, scalars=viscid.topology2color(topo))
######################################################################
# plot a random circle at geosynchronus orbit with scalars colored
# by the Matplotlib viridis color map, just because we can; this is
# a useful toy for debugging
circle = viscid.Circle(p0=[0, 0, 0], r=6.618, n=128, endpoint=True)
scalar = np.sin(circle.as_local_coordinates().get_crd('phi'))
surf = vlab.plot_line(circle.get_points(),
scalars=scalar,
clim=0.8,
cmap="Spectral_r")
######################################################################
# Use Mayavi (VTK) to calculate field lines using an interactive seed
# These field lines are colored by E parallel
epar = viscid.project(e, b)
epar.name = "Epar"
bsl2 = vlab.streamline(b,
epar,
seedtype='plane',
seed_resolution=4,
integration_direction='both',
clim=(-0.05, 0.05))
# now tweak the VTK streamlines
bsl2.stream_tracer.maximum_propagation = 20.
bsl2.seed.widget.origin = [-11, -5.0, -2.0]
bsl2.seed.widget.point1 = [-11, 5.0, -2.0]
bsl2.seed.widget.point2 = [-11.0, -5.0, 2.0]
bsl2.streamline_type = 'tube'
bsl2.tube_filter.radius = 0.03
bsl2.stop() # this stop/start was a hack to get something to update
bsl2.start()
bsl2.seed.widget.enabled = False
cbar = vlab.colorbar(bsl2,
title=epar.name,
label_fmt='%.3f',
orientation='horizontal')
cbar.scalar_bar_representation.position = (0.15, 0.01)
cbar.scalar_bar_representation.position2 = (0.72, 0.10)
###############################################################
# Make a contour at the open-closed boundary in the ionosphere
seeds_iono = viscid.Sphere(r=1.063,
pole=-moment,
ntheta=256,
nphi=256,
thetalim=(0, 180),
philim=(0, 360),
crd_system=b)
_, topo_iono = viscid.calc_streamlines(b,
seeds_iono,
ibound=1.0,
nr_procs='all',
output=viscid.OUTPUT_TOPOLOGY)
topo_iono = np.log2(topo_iono)
m = vlab.mesh_from_seeds(seeds_iono,
scalars=topo_iono,
opacity=1.0,
clim=(0, 3),
color=(0.992, 0.445, 0.0))
m.enable_contours = True
m.actor.property.line_width = 4.0
m.contour.number_of_contours = 4
####################################################################
# Plot the ionosphere, note that the sample data has the ionosphere
# at a different time, so the open-closed boundary found above
# will not be consistant with the field aligned currents
fac_tot = 1e9 * f_iono['fac_tot']
m = vlab.plot_ionosphere(fac_tot,
bounding_lat=30.0,
vmin=-300,
vmax=300,
opacity=0.75,
rotate=cotr,
crd_system=b)
m.actor.property.backface_culling = True
########################################################################
# Add some markers for earth, i.e., real earth, and dayside / nightside
# representation
vlab.plot_blue_marble(r=1.0,
lines=False,
ntheta=64,
nphi=128,
rotate=cotr,
crd_system=b)
# now shade the night side with a transparent black hemisphere
vlab.plot_earth_3d(radius=1.01, night_only=True, opacity=0.5, crd_system=b)
####################
# Finishing Touches
# vlab.axes(pp_src, nb_labels=5)
oa = vlab.orientation_axes()
oa.marker.set_viewport(0.75, 0.75, 1.0, 1.0)
# note that resize won't work if the current figure has the
# off_screen_rendering flag set
# vlab.resize([1200, 800])
vlab.view(azimuth=45, elevation=70, distance=35.0, focalpoint=[-2, 0, 0])
##############
# Save Figure
# print("saving png")
# vlab.savefig('mayavi_msphere_sample.png')
# print("saving x3d")
# # x3d files can be turned into COLLADA files with meshlab, and
# # COLLADA (.dae) files can be opened in OS X's preview
# #
# # IMPORTANT: for some reason, using bounding_lat in vlab.plot_ionosphere
# # causes a segfault when saving x3d files
# #
# vlab.savefig('mayavi_msphere_sample.x3d')
# print("done")
vlab.savefig(next_plot_fname(__file__))
###########################
# Interact Programatically
if args.interact:
vlab.interact()
#######################
# Interact Graphically
if args.show:
vlab.show()
try:
vlab.mlab.close()
except AttributeError:
pass
return 0
def main():
mhd_type = "C"
make_plots = 1
mhd_type = mhd_type.upper()
if mhd_type.startswith("C"):
if mhd_type in ("C", ):
f = viscid.load_file("$WORK/tmedium/*.3d.[-1].xdmf")
elif mhd_type in ("C2", "C3"):
f = viscid.load_file("$WORK/tmedium2/*.3d.[-1].xdmf")
else:
raise ValueError()
catol = 1e-8
rtol = 2e-6
elif mhd_type in ("F", "FORTRAN"):
f = viscid.load_file("$WORK/tmedium3/*.3df.[-1]")
catol = 1e-8
rtol = 7e-2
else:
raise ValueError()
do_fill_dipole = True
gslc = "x=-21.2j:12j, y=-11j:11j, z=-11j:11j"
b = f['b_cc'][gslc]
b1 = f['b_fc'][gslc]
e_cc = f['e_cc'][gslc]
e_ec = f['e_ec'][gslc]
if do_fill_dipole:
mask = viscid.make_spherical_mask(b, rmax=3.5)
viscid.fill_dipole(b, mask=mask)
mask = viscid.make_spherical_mask(b1, rmax=3.5)
viscid.fill_dipole(b1, mask=mask)
mask = None
# seeds = viscid.SphericalCap(r=1.02, ntheta=64, nphi=32, angle0=17, angle=20,
# philim=(100, 260), roll=-180.0)
# seeds = viscid.SphericalCap(r=1.02, ntheta=64, nphi=32, angle0=17, angle=20,
# philim=(0, 10), roll=0.0)
seedsN = viscid.Sphere(r=1.02,
ntheta=16,
nphi=16,
thetalim=(15, 25),
philim=(0, 300),
crd_system=b)
seedsS = viscid.Sphere(r=1.02,
ntheta=16,
nphi=16,
thetalim=(155, 165),
philim=(0, 300),
crd_system=b)
bl_kwargs = dict(ibound=0.9, obound0=(-20, -10, -10), obound1=(11, 10, 10))
# blines_cc, topo_cc = viscid.streamlines(b, seeds, **bl_kwargs)
blinesN_fc, topoN_fc = viscid.streamlines(b1, seedsN, **bl_kwargs)
_, topoS_fc = viscid.streamlines(b1,
seedsS,
output=viscid.OUTPUT_TOPOLOGY,
**bl_kwargs)
if True:
from viscid.plot import vlab
mesh = vlab.mesh_from_seeds(seedsN, scalars=topoN_fc)
mesh.actor.property.backface_culling = True
# vlab.plot_lines(blines_cc, scalars="#000000", tube_radius=0.03)
vlab.plot_lines(blinesN_fc,
scalars=viscid.topology2color(topoN_fc),
opacity=0.7)
vlab.plot_blue_marble(r=1.0)
vlab.plot_earth_3d(radius=1.01,
crd_system=b,
night_only=True,
opacity=0.5)
vlab.show()
if True:
vlt.subplot(121, projection='polar')
vlt.plot(topoN_fc)
vlt.subplot(122, projection='polar')
vlt.plot(topoS_fc)
vlt.show()
return 0
def trace_separator(grid, b_slcstr="x=-25j:15j, y=-30j:30j, z=-15j:15j",
r=1.0, plot=False, trace_opts=None, cache=True,
cache_dir=None):
"""Trace a separator line from most dawnward null
**Still in testing** Uses the bisection algorithm.
Args:
grid (Grid): A grid that has a "b" field
b_slcstr (str): Some valid slice for B field
r (float): spatial step of separator line
plot (bool): make debugging plots
trace_opts (dict): passed to streamline function
cache (bool, str): Save to and load from cache, if "force",
then don't load from cache if it exists, but do save a
cache at the end
cache_dir (str): Directory for cache, if None, same directory
as that file to which the grid belongs
Raises:
IOError: Description
Returns:
tuple: (separator_lines, nulls)
- **separator_lines** (list): list of M 3xN ndarrays that
represent M separator lines with N points
- **nulls** (ndarray): 3xN array of N null points
"""
if not cache_dir:
cache_dir = grid.find_info("_viscid_dirname", "./")
run_name = grid.find_info("run")
sep_fname = "{0}/{1}.sep.{2:06.0f}".format(cache_dir, run_name, grid.time)
try:
if isinstance(cache, string_types) and cache.strip().lower() == "force":
raise IOError()
with np.load(sep_fname + ".npz") as dat:
sep_iter = (f for f in dat.files if f.startswith("arr_"))
_it = sorted(sep_iter, key=lambda s: int(s[len("arr_"):]))
seps = [dat[n] for n in _it]
nulls = dat['nulls']
except IOError:
_b = grid['b'][b_slcstr]
_, nulls = viscid.find_nulls(_b['x=-30j:15j'], ibound=5.0)
# get most dawnward null, nulls2 is all nulls except p0
nullind = np.argmin(nulls[1, :])
p0 = nulls[:, nullind]
nulls2 = np.concatenate([nulls[:, :nullind], nulls[:, (nullind + 1):]],
axis=1)
if plot:
from viscid.plot import vlab
vlab.plot_earth_3d(crd_system='gse')
vlab.points3d(nulls2[0], nulls2[1], nulls2[2],
color=(0, 0, 0), scale_factor=1.0)
vlab.points3d(nulls[0, nullind], nulls[1, nullind], nulls[2, nullind],
color=(1, 1, 1), scale_factor=1.0)
seed = viscid.Sphere(p0=p0, r=r, ntheta=30, nphi=60,
theta_endpoint=True, phi_endpoint=True)
p1 = viscid.get_sep_pts_bisect(_b, seed, max_depth=12, plot=plot,
trace_opts=trace_opts)
# print("p1 shape", p1.shape)
# if p1.shape[1] > 2:
# raise RuntimeError("Invalid B field, should be no branch @ null")
seps = []
sep_stubs = []
for i in range(p1.shape[1]):
sep_stubs.append([p0, p1[:, i]])
# print("??", sep_stubs)
while sep_stubs:
sep = sep_stubs.pop(0)
# print("!!! new stub")
for i in count():
# print("::", i)
seed = viscid.SphericalPatch(p0=sep[-1], p1=sep[-1] - sep[-2],
r=r, nalpha=240, nbeta=240)
pn = viscid.get_sep_pts_bisect(_b, seed, max_depth=8, plot=plot,
trace_opts=trace_opts)
if pn.shape[1] == 0:
# print("END: pn.shape[1] == 0")
break
# print("++", nulls2.shape, pn.shape)
closest_null_dist = np.min(np.linalg.norm(nulls2 - pn[:, :1], axis=0))
# print("closest_null_dist:", closest_null_dist)
if closest_null_dist < 1.01 * r:
# print("END: within 1.01 of a null")
break
# print("??", pn)
for j in range(1, pn.shape[1]):
# print("inserting new stub")
sep_stubs.insert(0, [sep[-1], pn[:, j]])
sep.append(pn[:, 0])
# print("sep", sep)
seps.append(np.stack(sep, axis=1))
if cache:
np.savez_compressed(sep_fname, *seps, nulls=nulls)
return seps, nulls
