def test_no_element_setter(self):
species = Species(elements.carbon, 3, self.get_maxwellian())
with self.assertRaises(
AttributeError,
msg=
'It must not be possible to change the element of a species!'):
species.element = elements.fluorine
def test_no_ionisation_setter(self):
species = Species(elements.carbon, 3, self.get_maxwellian())
with self.assertRaises(
AttributeError,
msg=
'It must not be possible to change the ionisation of a species!'
):
species.ionisation = 5
def test_no_distribution_setter(self):
species = Species(elements.carbon, 3, self.get_maxwellian())
with self.assertRaises(
AttributeError,
msg=
'It must not be possible to change the distribution of a species!'
):
species.distribution = Maxwellian(
lambda x, y, z: 2e20, lambda x, y, z: 3e3,
lambda x, y, z: Vector3D(1.6e5, 0, 0), 4.1 * atomic_mass)
def test_negative_ionisation(self):
distribution = self.get_maxwellian()
with self.assertRaises(
ValueError,
msg='The ionisation of a species must not be negative!'):
Species(elements.carbon, -2, distribution)
def test_too_big_ionisation(self):
distribution = self.get_maxwellian()
with self.assertRaises(
ValueError,
msg=
'The ionisation of a species must not be superior than the atomic number of the element!'
):
Species(elements.carbon, 7, distribution)
d_density = GaussianVolume(0.94 * ion_density, sigma) he2_density = GaussianVolume(0.04 * ion_density, sigma) c6_density = GaussianVolume(0.01 * ion_density, sigma) ne10_density = GaussianVolume(0.01 * ion_density, sigma) e_density = GaussianVolume((0.94 + 0.04*2 + 0.01*6 + 0.01*10) * ion_density, sigma) temperature = 1000 + GaussianVolume(4000, sigma) bulk_velocity = ConstantVector3D(Vector3D(200e3, 0, 0)) d_distribution = Maxwellian(d_density, temperature, bulk_velocity, elements.deuterium.atomic_weight * atomic_mass) he2_distribution = Maxwellian(he2_density, temperature, bulk_velocity, elements.helium.atomic_weight * atomic_mass) c6_distribution = Maxwellian(c6_density, temperature, bulk_velocity, elements.carbon.atomic_weight * atomic_mass) ne10_distribution = Maxwellian(ne10_density, temperature, bulk_velocity, elements.neon.atomic_weight * atomic_mass) e_distribution = Maxwellian(e_density, temperature, bulk_velocity, electron_mass) d_species = Species(elements.deuterium, 1, d_distribution) he2_species = Species(elements.helium, 2, he2_distribution) c6_species = Species(elements.carbon, 6, c6_distribution) ne10_species = Species(elements.neon, 10, ne10_distribution) # define species plasma.b_field = ConstantVector3D(Vector3D(1.0, 1.0, 1.0)) plasma.electron_distribution = e_distribution plasma.composition = [d_species, he2_species, c6_species, ne10_species] # BEAM ------------------------------------------------------------------------ beam = Beam(parent=world, transform=translate(1.0, 0.0, 0) * rotate(90, 0, 0)) beam.plasma = plasma beam.atomic_data = adas beam.energy = 60000 beam.power = 3e6
d_density = GaussianVolume(0.5 * ion_density, sigma * 10000)
n_density = d_density * 0.01
e_density = GaussianVolume(ion_density, sigma * 10000)
temperature = 1 + GaussianVolume(79, sigma)
bulk_velocity = ConstantVector3D(Vector3D(-1e6, 0, 0))
deuterium_mass = deuterium.atomic_weight * atomic_mass
d_distribution = Maxwellian(d_density, temperature, bulk_velocity,
deuterium_mass)
nitrogen_mass = nitrogen.atomic_weight * atomic_mass
n_distribution = Maxwellian(n_density, temperature, bulk_velocity,
nitrogen_mass)
e_distribution = Maxwellian(e_density, temperature, bulk_velocity,
electron_mass)
d0_species = Species(deuterium, 0, d_distribution)
d1_species = Species(deuterium, 1, d_distribution)
n1_species = Species(nitrogen, 1, n_distribution)
# define species
plasma.b_field = ConstantVector3D(Vector3D(1.0, 1.0, 1.0))
plasma.electron_distribution = e_distribution
plasma.composition = [d0_species, d1_species, n1_species]
# setup the Balmer lines
hydrogen_I_410 = Line(deuterium, 0, (6, 2)) # n = 6->2: 410.12nm
hydrogen_I_396 = Line(deuterium, 0, (7, 2)) # n = 7->2: 396.95nm
# setup the Nitrgon II line with multiplet splitting instructions
nitrogen_II_404 = Line(nitrogen, 1,
("2s2 2p1 4f1 3G13.0", "2s2 2p1 3d1 3F10.0"))
def create_plasma(self, parent=None, transform=None, name=None):
"""
Make a CHERAB plasma object from this SOLEGE2D simulation.
:param Node parent: The plasma's parent node in the scenegraph, e.g. a World object.
:param AffineMatrix3D transform: Affine matrix describing the location and orientation
of the plasma in the world.
:param str name: User friendly name for this plasma (default = "SOLEDGE2D Plasma").
:rtype: Plasma
"""
mesh = self.mesh
name = name or "SOLEDGE2D Plasma"
plasma = Plasma(parent=parent, transform=transform, name=name)
radius = mesh.mesh_extent['maxr']
height = mesh.mesh_extent['maxz'] - mesh.mesh_extent['minz']
plasma.geometry = Cylinder(radius, height)
plasma.geometry_transform = translate(0, 0, mesh.mesh_extent['minz'])
tri_index_lookup = self.mesh.triangle_index_lookup
tri_to_grid = self.mesh.triangle_to_grid_map
if isinstance(self._b_field_vectors, np.ndarray):
plasma.b_field = SOLEDGE2DVectorFunction3D(
tri_index_lookup, tri_to_grid, self._b_field_vectors_cartesian)
else:
print(
'Warning! No magnetic field data available for this simulation.'
)
# Create electron species
triangle_data = _map_data_onto_triangles(self._electron_temperature)
electron_te_interp = Discrete2DMesh(mesh.vertex_coords,
mesh.triangles,
triangle_data,
limit=False)
electron_temp = AxisymmetricMapper(electron_te_interp)
triangle_data = _map_data_onto_triangles(self._electron_density)
electron_ne_interp = Discrete2DMesh.instance(electron_te_interp,
triangle_data)
electron_dens = AxisymmetricMapper(electron_ne_interp)
electron_velocity = lambda x, y, z: Vector3D(0, 0, 0)
plasma.electron_distribution = Maxwellian(electron_dens, electron_temp,
electron_velocity,
electron_mass)
if not isinstance(self.velocities_cartesian, np.ndarray):
print(
'Warning! No velocity field data available for this simulation.'
)
b2_neutral_i = 0 # counter for B2 neutrals
for k, sp in enumerate(self.species_list):
# Identify the species based on its symbol
symbol, charge = re.match(_SPECIES_REGEX, sp).groups()
charge = int(charge)
species_type = _species_symbol_map[symbol]
# If neutral and B" atomic density available, use B2 density, otherwise use fluid species density.
if isinstance(self.b2_neutral_densities,
np.ndarray) and charge == 0:
species_dens_data = self.b2_neutral_densities[:, :,
b2_neutral_i]
b2_neutral_i += 1
else:
species_dens_data = self.species_density[:, :, k]
triangle_data = _map_data_onto_triangles(species_dens_data)
dens = AxisymmetricMapper(
Discrete2DMesh.instance(electron_te_interp, triangle_data))
# dens = SOLPSFunction3D(tri_index_lookup, tri_to_grid, species_dens_data)
# Create the velocity vector lookup function
if isinstance(self.velocities_cartesian, np.ndarray):
velocity = SOLEDGE2DVectorFunction3D(
tri_index_lookup, tri_to_grid,
self.velocities_cartesian[:, :, k, :])
else:
velocity = lambda x, y, z: Vector3D(0, 0, 0)
distribution = Maxwellian(dens, electron_temp, velocity,
species_type.atomic_weight * atomic_mass)
plasma.composition.add(Species(species_type, charge, distribution))
return plasma
vy_profile = IonFunction(1E5, 0, pedestal_top=pedestal_top)
def vectorfunction3d(x, y, z):
vy = vy_profile(x, y, z)
return Vector3D(0, vy, 0)
velocity_profile = PythonVectorFunction3D(vectorfunction3d)
# define neutral species distribution
h0_density = NeutralFunction(peak_density, 0.1, pedestal_top=pedestal_top)
h0_temperature = Constant3D(neutral_temperature)
h0_distribution = Maxwellian(h0_density, h0_temperature, velocity_profile,
hydrogen.atomic_weight * atomic_mass)
species.append(Species(hydrogen, 0, h0_distribution))
# define hydrogen ion species distribution
h1_density = IonFunction(peak_density, 0, pedestal_top=pedestal_top)
h1_temperature = IonFunction(peak_temperature, 0, pedestal_top=pedestal_top)
h1_distribution = Maxwellian(h1_density, h1_temperature, velocity_profile,
hydrogen.atomic_weight * atomic_mass)
species.append(Species(hydrogen, 1, h1_distribution))
# add impurities
if impurities:
for impurity, ionisation, concentration in impurities:
imp_density = IonFunction(peak_density * concentration,
0,
pedestal_top=pedestal_top)
imp_temperature = IonFunction(peak_temperature,
density_c6_data = sal.get(
DATA_PATH.format(PULSE_PLASMA, user, 'PRFL', 'C6', sequence)).data[mask]
density_c6_psi = Interpolate1DCubic(psi_coord, density_c6_data)
density_c6 = AxisymmetricMapper(
Blend2D(Constant2D(0.0), IsoMapper2D(psin_2d, density_c6_psi),
inside_lcfs))
density_d = lambda x, y, z: electron_density(x, y, z) - 6 * density_c6(x, y, z)
d_distribution = Maxwellian(density_d, ion_temperature, flow_velocity,
deuterium.atomic_weight * atomic_mass)
c6_distribution = Maxwellian(density_c6, ion_temperature, flow_velocity,
carbon.atomic_weight * atomic_mass)
e_distribution = Maxwellian(electron_density, ion_temperature, flow_velocity,
electron_mass)
d_species = Species(deuterium, 1, d_distribution)
c6_species = Species(carbon, 6, c6_distribution)
plasma.electron_distribution = e_distribution
plasma.composition = [d_species, c6_species]
# ########################### NBI CONFIGURATION ############################# #
print('Loading JET PINI configuration...')
attenuation_instructions = (SingleRayAttenuator, {'clamp_to_zero': True})
beam_emission_instructions = [(BeamCXLine, {'line': Line(carbon, 5, (8, 7))})]
pini_8_1 = load_pini_from_ppf(PULSE, '8.1', plasma, adas,
attenuation_instructions,
plasma.geometry = Sphere(sigma * 5.0)
plasma.geometry_transform = None
plasma.integrator = NumericalIntegrator(step=sigma / 5.0)
# define basic distributions
d_density = GaussianVolume(0.5 * ion_density, sigma * 10000)
e_density = GaussianVolume(ion_density, sigma * 10000)
temperature = 1 + GaussianVolume(79, sigma)
bulk_velocity = ConstantVector3D(Vector3D(-1e5, 0, 0))
d_mass = elements.deuterium.atomic_weight * atomic_mass
d_distribution = Maxwellian(d_density, temperature, bulk_velocity, d_mass)
e_distribution = Maxwellian(e_density, temperature, bulk_velocity,
electron_mass)
d0_species = Species(elements.deuterium, 0, d_distribution)
d1_species = Species(elements.deuterium, 1, d_distribution)
# define species
plasma.b_field = ConstantVector3D(Vector3D(1.0, 1.0, 1.0))
plasma.electron_distribution = e_distribution
plasma.composition = [d0_species, d1_species]
# Setup elements.deuterium lines
d_alpha = Line(elements.deuterium, 0, (3, 2))
d_beta = Line(elements.deuterium, 0, (4, 2))
d_gamma = Line(elements.deuterium, 0, (5, 2))
d_delta = Line(elements.deuterium, 0, (6, 2))
d_epsilon = Line(elements.deuterium, 0, (7, 2))
plasma.models = [
plt.title('c6 density')
plt.figure()
plt.imshow(d)
plt.colorbar()
plt.title('deuterium density in poloidal plane')
#define distributions
d_distribution = Maxwellian(density_d, ion_temperature, flow_velocity,
deuterium.atomic_weight * atomic_mass)
c6_distribution = Maxwellian(density_c6, ion_temperature, flow_velocity,
carbon.atomic_weight * atomic_mass)
e_distribution = Maxwellian(electron_density, ion_temperature, flow_velocity,
electron_mass)
d1_species = Species(elements.deuterium, 1, d_distribution)
c6_species = Species(carbon, 6, c6_distribution)
#define plasma parameters - electron distribution, impurity composition and B field from EFIT
plasma.electron_distribution = e_distribution
plasma.composition = [d1_species, c6_species]
plasma.b_field = VectorAxisymmetricMapper(equil_time_slice.b_field)
sigma = 0.25
integration_step = 0.02
#define the plasma geometry
plasma.integrator.step = integration_step
plasma.integrator.min_samples = 1000
plasma.atomic_data = adas
plasma.geometry = Cylinder(sigma * 2, sigma * 10.0)
# plasma creation #
plasma = Plasma(parent=world)
plasma.atomic_data = OpenADAS(permit_extrapolation=True)
plasma.geometry = Cylinder(3.5, 2.2, transform=translate(0, 0, -1.1))
plasma.geometry_transform = translate(0, 0, -1.1)
# No net velocity for any species
zero_velocity = ConstantVector3D(Vector3D(0, 0, 0))
# define neutral species distribution
d0_density = NeutralFunction(peak_density, 0.1, magnetic_axis)
d0_temperature = Constant3D(0.5) # constant 0.5eV temperature for all neutrals
d0_distribution = Maxwellian(d0_density, d0_temperature, zero_velocity,
deuterium.atomic_weight * atomic_mass)
d0_species = Species(deuterium, 0, d0_distribution)
# define deuterium ion species distribution
d1_density = IonFunction(peak_density, 0, magnetic_axis)
d1_temperature = IonFunction(peak_temperature, 0, magnetic_axis)
d1_distribution = Maxwellian(d1_density, d1_temperature, zero_velocity,
deuterium.atomic_weight * atomic_mass)
d1_species = Species(deuterium, 1, d1_distribution)
# define the electron distribution
e_density = IonFunction(peak_density, 0, magnetic_axis)
e_temperature = IonFunction(peak_temperature, 0, magnetic_axis)
e_distribution = Maxwellian(e_density, e_temperature, zero_velocity, electron_mass)
# define species
plasma.b_field = ConstantVector3D(Vector3D(1.0, 1.0, 1.0))
