コード例 #1
0
ファイル: beam.py プロジェクト: cherab/core
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
beam.element = elements.deuterium
beam.sigma = 0.025
beam.divergence_x = 0.5
beam.divergence_y = 0.5
beam.length = 3.0
beam.attenuator = SingleRayAttenuator(clamp_to_zero=True)
コード例 #2
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        imp_temperature = IonFunction(peak_temperature,
                                      0,
                                      pedestal_top=pedestal_top)
        imp_distribution = Maxwellian(imp_density, imp_temperature,
                                      velocity_profile,
                                      impurity.atomic_weight * atomic_mass)
        species.append(Species(impurity, ionisation, imp_distribution))

# define the electron distribution
e_density = IonFunction(peak_density, 0, pedestal_top=pedestal_top)
e_temperature = IonFunction(peak_temperature, 0, pedestal_top=pedestal_top)
e_distribution = Maxwellian(e_density, e_temperature, velocity_profile,
                            electron_mass)

# define species
plasma.b_field = ConstantVector3D(Vector3D(0, 0, 0))
plasma.electron_distribution = e_distribution
plasma.composition = species

####################
# Visualise Plasma #

h0 = plasma.composition.get(hydrogen, 0)
h1 = plasma.composition.get(hydrogen, 1)
c6 = plasma.composition.get(carbon, 6)

# Run some plots to check the distribution functions and emission profile are as expected
h1_temp = h1.distribution.effective_temperature
r, _, z, t_samples = sample3d(h1_temp, (-1, 2, 200), (0, 0, 1), (-1, 1, 200))
plt.imshow(np.transpose(np.squeeze(t_samples)), extent=[-1, 2, -1, 1])
plt.colorbar()
コード例 #3
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    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
コード例 #4
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# ########################### PLASMA EQUILIBRIUM ############################ #
print('Plasma equilibrium')

equilibrium = JETEquilibrium(PULSE)
equil_time_slice = equilibrium.time(TIME)
psin_2d = equil_time_slice.psi_normalised
psin_3d = AxisymmetricMapper(equil_time_slice.psi_normalised)
inside_lcfs = equil_time_slice.inside_lcfs

# ########################### PLASMA CONFIGURATION ########################## #
print('Plasma configuration')

plasma = Plasma(parent=world)
plasma.atomic_data = adas
plasma.b_field = VectorAxisymmetricMapper(equil_time_slice.b_field)

DATA_PATH = '/pulse/{}/ppf/signal/{}/{}/{}:{}'
user = '******'
sequence = 0

psi_coord = sal.get(
    DATA_PATH.format(PULSE_PLASMA, user, 'PRFL', 'C6',
                     sequence)).dimensions[0].data
mask = psi_coord <= 1.0
psi_coord = psi_coord[mask]

flow_velocity_tor_data = sal.get(
    DATA_PATH.format(PULSE_PLASMA, user, 'PRFL', 'VT', sequence)).data[mask]
flow_velocity_tor_psi = Interpolate1DCubic(psi_coord, flow_velocity_tor_data)
flow_velocity_tor = AxisymmetricMapper(