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# # Electromagnetic scattering from a wire with scattering boundary conditions
#
# Copyright (C) 2022 Michele Castriotta, Igor Baratta, Jørgen S. Dokken
#
# This demo is implemented in two files: one for the mesh generation
# with gmsh, and one for the variational forms and the solver. It
# illustrates how to:
#
# - Use complex quantities in FEniCSx
# - Setup and solve Maxwell's equations
# - Implement Scattering Boundary Conditions
#
# ## Equations, problem definition and implementation
#
# First of all, let's import the modules that will be used:

# +
import sys

from mpi4py import MPI

from analytical_efficiencies_wire import calculate_analytical_efficiencies
from mesh_wire import generate_mesh_wire

import ufl
from basix.ufl import element
from dolfinx import default_scalar_type, fem, io, plot
from dolfinx.fem.petsc import LinearProblem

try:
    import gmsh
except ModuleNotFoundError:
    print("This demo requires gmsh to be installed")
    sys.exit(0)
import numpy as np

try:
    import pyvista

    have_pyvista = True
except ModuleNotFoundError:
    print("pyvista and pyvistaqt are required to visualise the solution")
    have_pyvista = False

# -

# Since we want to solve time-harmonic Maxwell's equation, we need to
# solve a complex-valued PDE, and therefore need to use PETSc compiled
# with complex numbers.

if not np.issubdtype(default_scalar_type, np.complexfloating):
    print("Demo should only be executed with DOLFINx complex mode")
    exit(0)


# Now, let's consider an infinite metallic wire immersed in a background
# medium (e.g. vacuum or water). Let's now consider the plane cutting
# the wire perpendicularly to its axis at a generic point. Such plane
# $\Omega=\Omega_{m} \cup\Omega_{b}$ is formed by the cross-section of
# the wire $\Omega_m$ and the background medium $\Omega_{b}$ surrounding
# the wire. Let's consider just the portion of this plane delimited by
# an external circular boundary $\partial \Omega$. We want to calculate
# the electric field $\mathbf{E}_s$ scattered by the wire when a
# background wave $\mathbf{E}_b$ impinges on it. We will consider a
# background plane wave at $\lambda_0$ wavelength, that can be written
# analytically as:
#
# $$
# \mathbf{E}_b = \exp(\mathbf{k}\cdot\mathbf{r})\hat{\mathbf{u}}_p
# $$
#
# with $\mathbf{k} = \frac{2\pi}{\lambda_0}n_b\hat{\mathbf{u}}_k$ being
# the wavevector of the plane wave, pointing along the propagation
# direction, with $\hat{\mathbf{u}}_p$ being the polarization direction,
# and with $\mathbf{r}$ being a point in $\Omega$. We will only consider
# $\hat{\mathbf{u}}_k$ and $\hat{\mathbf{u}}_p$ with components
# belonging to the $\Omega$ domain and perpendicular to each other, i.e.
# $\hat{\mathbf{u}}_k \perp \hat{\mathbf{u}}_p$ (transversality
# condition of plane waves). Using a Cartesian coordinate system for
# $\Omega$, and by defining $k_x = n_bk_0\cos\theta$ and $k_y =
# n_bk_0\sin\theta$, with $\theta$ being the angle defined by the
# propagation direction $\hat{\mathbf{u}}_k$ and the horizontal axis
# $\hat{\mathbf{u}}_x$, we have:
#
# $$
# \mathbf{E}_b = -\sin\theta e^{j (k_xx+k_yy)}\hat{\mathbf{u}}_x
# + \cos\theta e^{j (k_xx+k_yy)}\hat{\mathbf{u}}_y
# $$
#
# The following class implements this functions. The inputs to the
# function are the angle $\theta$, the background refractive index $n_b$
# and the vacuum wavevector $k_0$.

# +


class BackgroundElectricField:
    def __init__(self, theta: float, n_bkg: float, k0: complex):
        self.theta = theta  # incident angle
        self.k0 = k0  # vacuum wavevector
        self.n_bkg = n_bkg  # background refractive index

    def eval(
        self, x: np.typing.NDArray[np.float64]
    ) -> tuple[np.typing.NDArray[np.complex128], np.typing.NDArray[np.complex128]]:
        kx = self.n_bkg * self.k0 * np.cos(self.theta)
        ky = self.n_bkg * self.k0 * np.sin(self.theta)
        phi = kx * x[0] + ky * x[1]
        ax, ay = np.sin(self.theta), np.cos(self.theta)
        return (-ax * np.exp(1j * phi), ay * np.exp(1j * phi))


# -

# The Maxwell's equation for scattering problems takes the following
# form:
#
# $$
# -\nabla \times \nabla \times \mathbf{E}_s+\varepsilon_{r} k_{0}^{2}
# \mathbf{E}_s
# +k_{0}^{2}\left(\varepsilon_{r}-\varepsilon_{b}\right)
# \mathbf{E}_{\mathrm{b}}=0 \textrm{ in } \Omega,
# $$
#
# where $k_0 = 2\pi/\lambda_0$ is the vacuum wavevector of the
# background field, $\varepsilon_b$ is the background relative
# permittivity and $\varepsilon_r$ is the relative permittivity as a
# function of space, i.e.:
#
# $$
# \varepsilon_r = \begin{cases}
# \varepsilon_m & \textrm{on }\Omega_m \\
# \varepsilon_b & \textrm{on }\Omega_b
# \end{cases}
# $$
#
# with $\varepsilon_m$ being the relative permittivity of the metallic
# wire. As reference values, we will consider $\lambda_0 =
# 400\textrm{nm}$ (violet light), $\varepsilon_b = 1.33^2$ (relative
# permittivity of water), and $\varepsilon_m = -1.0782 +
# 5.8089\textrm{j}$ (relative permittivity of gold at $400\textrm{nm}$).
#
# To form a well-determined system, we add boundary conditions on
# $\partial \Omega$. It is common to use scattering boundary conditions
# (ref), which make the boundary transparent for $\mathbf{E}_s$,
# allowing us to restrict the computational boundary to a finite
# $\Omega$ domain. The first-order boundary conditions in the 2D case
# take the following form:
#
# $$\mathbf{n} \times
# \nabla \times \mathbf{E}_s+\left(j k_{0}n_b + \frac{1}{2r}
# \right) \mathbf{n} \times \mathbf{E}_s
# \times \mathbf{n}=0\quad \textrm{ on } \partial \Omega,
# $$
#
#
# with $n_b = \sqrt{\varepsilon_b}$ being the background refractive
# index, $\mathbf{n}$ being the normal vector to $\partial \Omega$, and
# $r = \sqrt{(x-x_s)^2 + (y-y_s)^2}$ being the distance of the $(x, y)$
# point on $\partial\Omega$ from the wire centered in $(x_s, y_s)$. We
# consider a wired centered at the origin, i.e. $r =\sqrt{x^2 + y^2}$.
#
# The radial distance function $r(x)$ and $\nabla \times$ operator for a
# 2D vector (in UFL syntax) is defined below.
#


# +
def radial_distance(x: ufl.SpatialCoordinate):
    """Returns the radial distance from the origin"""
    return ufl.sqrt(x[0] ** 2 + x[1] ** 2)


def curl_2d(f: fem.Function):
    """Returns the curl of two 2D vectors as a 3D vector"""
    return ufl.as_vector((0, 0, f[1].dx(0) - f[0].dx(1)))


# -

# Next we define some mesh specific parameters. Please notice that the
# length units are normalized with respect to $1\mu m$.


# +
pi = np.pi
epsilon_0 = 8.8541878128 * 10**-12
mu_0 = 4 * pi * 10**-7

# Radius of the wire and of the boundary of the domain
radius_wire = 0.050
radius_dom = 1

# The smaller the mesh_factor, the finer is the mesh
mesh_factor = 1.2

# Mesh size inside the wire
in_wire_size = mesh_factor * 7.0e-3

# Mesh size at the boundary of the wire
on_wire_size = mesh_factor * 3.0e-3

# Mesh size in the background
bkg_size = mesh_factor * 60.0e-3

# Mesh size at the boundary
boundary_size = mesh_factor * 30.0e-3

# Tags for the subdomains
au_tag = 1  # gold wire
bkg_tag = 2  # background
boundary_tag = 3  # boundary
# -

# We generate the mesh using GMSH and convert it to a
# `dolfinx.mesh.Mesh`.

# +
model = None
gmsh.initialize(sys.argv)
if MPI.COMM_WORLD.rank == 0:
    model = generate_mesh_wire(
        radius_wire,
        radius_dom,
        in_wire_size,
        on_wire_size,
        bkg_size,
        boundary_size,
        au_tag,
        bkg_tag,
        boundary_tag,
    )

model = MPI.COMM_WORLD.bcast(model, root=0)
domain, cell_tags, facet_tags = io.gmshio.model_to_mesh(model, MPI.COMM_WORLD, 0, gdim=2)

gmsh.finalize()
MPI.COMM_WORLD.barrier()
# -

# The mesh is visualized with [PyVista](https://docs.pyvista.org/)

if have_pyvista:
    topology, cell_types, geometry = plot.vtk_mesh(domain, 2)
    grid = pyvista.UnstructuredGrid(topology, cell_types, geometry)
    plotter = pyvista.Plotter()
    num_local_cells = domain.topology.index_map(domain.topology.dim).size_local
    grid.cell_data["Marker"] = cell_tags.values[cell_tags.indices < num_local_cells]
    grid.set_active_scalars("Marker")
    plotter.add_mesh(grid, show_edges=True)
    plotter.view_xy()
    if not pyvista.OFF_SCREEN:
        plotter.show()
    else:
        pyvista.start_xvfb()
        figure = plotter.screenshot("wire_mesh.png", window_size=[8000, 8000])

# Now we define some other problem specific parameters:

wl0 = 0.4  # Wavelength of the background field
n_bkg = 1.33  # Background refractive index
eps_bkg = n_bkg**2  # Background relative permittivity
k0 = 2 * np.pi / wl0  # Wavevector of the background field
theta = np.pi / 4  # Angle of incidence of the background field

# We use a function space consisting of degree 3 [Nedelec (first
# kind)](https://defelement.com/elements/nedelec1.html) elements to
# represent the electric field

degree = 3
curl_el = element("N1curl", domain.basix_cell(), degree)
V = fem.functionspace(domain, curl_el)

# Next, we can interpolate $\mathbf{E}_b$ into the function space $V$:

# +
f = BackgroundElectricField(theta, n_bkg, k0)
Eb = fem.Function(V)
Eb.interpolate(f.eval)

x = ufl.SpatialCoordinate(domain)
r = radial_distance(x)

# Create test and trial functions
Es = ufl.TrialFunction(V)
v = ufl.TestFunction(V)

# Definition of 3d fields for cross and curl operations
Es_3d = ufl.as_vector((Es[0], Es[1], 0))
v_3d = ufl.as_vector((v[0], v[1], 0))

# Measures for subdomains
dx = ufl.Measure("dx", domain, subdomain_data=cell_tags)
ds = ufl.Measure("ds", domain, subdomain_data=facet_tags)
dDom = dx((au_tag, bkg_tag))
dsbc = ds(boundary_tag)

# Normal to the boundary
n = ufl.FacetNormal(domain)
n_3d = ufl.as_vector((n[0], n[1], 0))
# -

# We turn our focus to the permittivity $\varepsilon$. First, we define
# the relative permittivity $\varepsilon_m$ of the gold wire at $400nm$.
# This data can be found in [*Olmon et al.
# 2012*](https://doi.org/10.1103/PhysRevB.86.235147) or at
# [refractiveindex.info](
# https://refractiveindex.info/?shelf=main&book=Au&page=Olmon-sc)):

eps_au = -1.0782 + 1j * 5.8089

# We define a permittivity function $\varepsilon$ that takes the value
# of the gold permittivity $\varepsilon_m$ for cells inside the wire,
# while it takes the value of the background permittivity otherwise:

D = fem.functionspace(domain, ("DG", 0))
eps = fem.Function(D)
au_cells = cell_tags.find(au_tag)
bkg_cells = cell_tags.find(bkg_tag)
eps.x.array[au_cells] = np.full_like(au_cells, eps_au, dtype=eps.x.array.dtype)
eps.x.array[bkg_cells] = np.full_like(bkg_cells, eps_bkg, dtype=eps.x.array.dtype)
eps.x.scatter_forward()

# Next we derive the weak formulation of the Maxwell's equation plus
# with scattering boundary conditions. First, we take the inner products
# of the equations with a complex test function $\mathbf{v}$, and
# integrate the terms over the corresponding domains:
#
# $$
# \begin{align}
# & \int_{\Omega}-\nabla \times( \nabla \times \mathbf{E}_s) \cdot
# \bar{\mathbf{v}}+\varepsilon_{r} k_{0}^{2} \mathbf{E}_s \cdot
# \bar{\mathbf{v}}+k_{0}^{2}\left(\varepsilon_{r}-\varepsilon_b\right)
# \mathbf{E}_b \cdot \bar{\mathbf{v}}~\mathrm{d}x \\
# +& \int_{\partial \Omega}
# (\mathbf{n} \times \nabla \times \mathbf{E}_s) \cdot \bar{\mathbf{v}}
# +\left(j n_bk_{0}+\frac{1}{2r}\right) (\mathbf{n} \times \mathbf{E}_s
# \times \mathbf{n}) \cdot \bar{\mathbf{v}}~\mathrm{d}s=0
# \end{align}
# $$
#
# By using $(\nabla \times \mathbf{A}) \cdot \mathbf{B}=\mathbf{A}
# \cdot(\nabla \times \mathbf{B})+\nabla \cdot(\mathbf{A} \times
# \mathbf{B}),$ we can change the first term into:
#
# $$
# \begin{align}
# & \int_{\Omega}-\nabla \cdot(\nabla\times\mathbf{E}_s \times
# \bar{\mathbf{v}})-\nabla \times \mathbf{E}_s \cdot \nabla
# \times\bar{\mathbf{v}}+\varepsilon_{r} k_{0}^{2} \mathbf{E}_s
# \cdot \bar{\mathbf{v}}+k_{0}^{2}\left(\varepsilon_{r}-\varepsilon_b\right)
# \mathbf{E}_b \cdot \bar{\mathbf{v}}~\mathrm{dx} \\
# +&\int_{\partial \Omega}
# (\mathbf{n} \times \nabla \times \mathbf{E}_s) \cdot \bar{\mathbf{v}}
# +\left(j n_bk_{0}+\frac{1}{2r}\right) (\mathbf{n} \times \mathbf{E}_s
# \times \mathbf{n}) \cdot \bar{\mathbf{v}}~\mathrm{d}s=0,
# \end{align}
# $$
#
# using the divergence theorem
# $\int_\Omega\nabla\cdot\mathbf{F}~\mathrm{d}x = \int_{\partial\Omega}
# \mathbf{F}\cdot\mathbf{n}~\mathrm{d}s$, we can write:
#
# $$
# \begin{align}
# & \int_{\Omega}-(\nabla \times \mathbf{E}_s) \cdot (\nabla \times
# \bar{\mathbf{v}})+\varepsilon_{r} k_{0}^{2} \mathbf{E}_s \cdot
# \bar{\mathbf{v}}+k_{0}^{2}\left(\varepsilon_{r}-\varepsilon_b\right)
# \mathbf{E}_b \cdot \bar{\mathbf{v}}~\mathrm{d}x \\
# +&\int_{\partial \Omega}
# -(\nabla\times\mathbf{E}_s \times \bar{\mathbf{v}})\cdot\mathbf{n}
# + (\mathbf{n} \times \nabla \times \mathbf{E}_s) \cdot \bar{\mathbf{v}}
# +\left(j n_bk_{0}+\frac{1}{2r}\right) (\mathbf{n} \times \mathbf{E}_s
# \times \mathbf{n}) \cdot \bar{\mathbf{v}}~\mathrm{d}s=0.
# \end{align}
# $$
#
# Cancelling $-(\nabla\times\mathbf{E}_s \times \bar{\mathbf{V}})
# \cdot\mathbf{n}$  and $\mathbf{n} \times \nabla \times \mathbf{E}_s
# \cdot \bar{\mathbf{V}}$ and rearrange $\left((\mathbf{n} \times \mathbf{E}_s)
# \times \mathbf{n}\right) \cdot \bar{\mathbf{v}}$ to $ (\mathbf{E}_s \times\mathbf{n})
# \cdot (\bar{\mathbf{v}} \times \mathbf{n})$ using the triple product rule $\mathbf{A}
# \cdot(\mathbf{B} \times \mathbf{C})=\mathbf{B} \cdot(\mathbf{C} \times
# \mathbf{A})=\mathbf{C} \cdot(\mathbf{A} \times \mathbf{B})$, we get:
#
# $$
# \begin{align}
# & \int_{\Omega}-(\nabla \times \mathbf{E}_s) \cdot (\nabla \times
# \bar{\mathbf{v}})+\varepsilon_{r} k_{0}^{2} \mathbf{E}_s \cdot
# \bar{\mathbf{v}}+k_{0}^{2}\left(\varepsilon_{r}-\varepsilon_b\right)
# \mathbf{E}_b \cdot \bar{\mathbf{v}}~\mathrm{d}x \\
# +&\int_{\partial \Omega}
# \left(j n_bk_{0}+\frac{1}{2r}\right)( \mathbf{n} \times \mathbf{E}_s \times
# \mathbf{n}) \cdot \bar{\mathbf{v}} ~\mathrm{d} s = 0.
# \end{align}
# $$
#
# We use the [UFL](https://github.com/FEniCS/ufl/) to implement the
# residual

# Weak form
F = (
    -ufl.inner(ufl.curl(Es), ufl.curl(v)) * dDom
    + eps * (k0**2) * ufl.inner(Es, v) * dDom
    + (k0**2) * (eps - eps_bkg) * ufl.inner(Eb, v) * dDom
    + (1j * k0 * n_bkg + 1 / (2 * r))
    * ufl.inner(ufl.cross(Es_3d, n_3d), ufl.cross(v_3d, n_3d))
    * dsbc
)

# We split the residual into a sesquilinear (lhs) and linear (rhs) form
# and solve the problem. We store the scattered field $\mathbf{E}_s$ as
# `Esh`:

a, L = ufl.lhs(F), ufl.rhs(F)
problem = LinearProblem(a, L, bcs=[], petsc_options={"ksp_type": "preonly", "pc_type": "lu"})
Esh = problem.solve()

# We save the solution as an [ADIOS2
# bp](https://adios2.readthedocs.io/en/latest/ecosystem/visualization.html)
# folder. In order to do so, we need to interpolate our solution
# discretized with Nedelec elements into a suitable discontinuous
# Lagrange space.

# +
gdim = domain.geometry.dim
V_dg = fem.functionspace(domain, ("Discontinuous Lagrange", degree, (gdim,)))
Esh_dg = fem.Function(V_dg)
Esh_dg.interpolate(Esh)

if hasattr(io,"VTXWriter"):
    with io.VTXWriter(domain.comm, "Esh.bp", Esh_dg) as vtx:
        vtx.write(0.0)
else:
    print("Cannot write Esh.bp: VTXWriter (adios2) is not available")
# -

# We visualize the solution using PyVista. For more information about
# saving and visualizing vector fields discretized with Nedelec
# elements, check [this](
# https://docs.fenicsproject.org/dolfinx/main/python/demos/demo_interpolation-io.html)
# DOLFINx demo.

if have_pyvista:
    V_cells, V_types, V_x = plot.vtk_mesh(V_dg)
    V_grid = pyvista.UnstructuredGrid(V_cells, V_types, V_x)
    Esh_values = np.zeros((V_x.shape[0], 3), dtype=np.float64)
    Esh_values[:, : domain.topology.dim] = Esh_dg.x.array.reshape(
        V_x.shape[0], domain.topology.dim
    ).real

    V_grid.point_data["u"] = Esh_values

    plotter = pyvista.Plotter()
    plotter.add_text("magnitude", font_size=12, color="black")
    plotter.add_mesh(V_grid.copy(), show_edges=True)
    plotter.view_xy()
    plotter.link_views()
    if not pyvista.OFF_SCREEN:
        plotter.show()
    else:
        pyvista.start_xvfb()
        plotter.screenshot("Esh.png", window_size=[800, 800])

# Next we can calculate the total electric field
# $\mathbf{E}=\mathbf{E}_s+\mathbf{E}_b$ and save it.

# +
E = fem.Function(V)
E.x.array[:] = Eb.x.array[:] + Esh.x.array[:]
E_dg = fem.Function(V_dg)
E_dg.interpolate(E)
if hasattr(io,"VTXWriter"):
    with io.VTXWriter(domain.comm, "E.bp", E_dg) as vtx:
        vtx.write(0.0)
else:
    print("Cannot write E.bp: VTXWriter (adios2) is not available")
# -

# We validate our numerical solution by computing the absorption,
# scattering and extinction efficiencies, which are quantities that
# define how much light is absorbed and scattered by the wire. First of
# all, we calculate the analytical efficiencies with the
# `calculate_analytical_efficiencies` function defined in a separate
# file:

# Calculation of analytical efficiencies
q_abs_analyt, q_sca_analyt, q_ext_analyt = calculate_analytical_efficiencies(
    eps_au, n_bkg, wl0, radius_wire
)

# Now we can calculate the numerical efficiencies. The formula for the
# absorption, scattering and extinction are:
#
# $$
# \begin{align}
# & Q_{abs} = \operatorname{Re}\left(\int_{\Omega_{m}} \frac{1}{2}
#   \frac{\operatorname{Im}(\varepsilon_m)k_0}{Z_0n_b}
#   \mathbf{E}\cdot\hat{\mathbf{E}}dx\right) \\
# & Q_{sca} = \operatorname{Re}\left(\int_{\partial\Omega} \frac{1}{2}
#   \left(\mathbf{E}_s\times\bar{\mathbf{H}}_s\right)
#   \cdot\mathbf{n}ds\right)\\ \\
# & Q_{ext} = Q_{abs} + Q_{sca},
# \end{align}
# $$
#
# with $Z_0 = \sqrt{\frac{\mu_0}{\varepsilon_0}}$ being the vacuum
# impedance, and $\mathbf{H}_s =
# -j\frac{1}{Z_0k_0n_b}\nabla\times\mathbf{E}_s$ being the scattered
# magnetic field. We can then normalize these values over the intensity
# of the electromagnetic field $I_0$ and the geometrical cross section
# of the wire, $\sigma_{gcs} = 2r_w$:
#
# $$
# \begin{align}
# & q_{abs} = \frac{Q_{abs}}{I_0\sigma_{gcs}} \\
# & q_{sca} = \frac{Q_{sca}}{I_0\sigma_{gcs}} \\
# & q_{ext} = q_{abs} + q_{sca}.
# \end{align}
# $$
#
# We can calculate these values in the following way:

# +
# Vacuum impedance
Z0 = np.sqrt(mu_0 / epsilon_0)

# Magnetic field H
Hsh_3d = -1j * curl_2d(Esh) / (Z0 * k0 * n_bkg)

Esh_3d = ufl.as_vector((Esh[0], Esh[1], 0))
E_3d = ufl.as_vector((E[0], E[1], 0))

# Intensity of the electromagnetic fields I0 = 0.5*E0**2/Z0 E0 =
# np.sqrt(ax**2 + ay**2) = 1, see background_electric_field
I0 = 0.5 / Z0

# Geometrical cross section of the wire
gcs = 2 * radius_wire

# Quantities for the calculation of efficiencies
P = 0.5 * ufl.inner(ufl.cross(Esh_3d, ufl.conj(Hsh_3d)), n_3d)
Q = 0.5 * np.imag(eps_au) * k0 * (ufl.inner(E_3d, E_3d)) / Z0 / n_bkg

# Define integration domain for the wire
dAu = dx(au_tag)

# Normalized absorption efficiency
q_abs_fenics_proc = (fem.assemble_scalar(fem.form(Q * dAu)) / gcs / I0).real
q_abs_fenics = domain.comm.allreduce(q_abs_fenics_proc, op=MPI.SUM)

# Normalized scattering efficiency
q_sca_fenics_proc = (fem.assemble_scalar(fem.form(P * dsbc)) / gcs / I0).real
q_sca_fenics = domain.comm.allreduce(q_sca_fenics_proc, op=MPI.SUM)

# Extinction efficiency
q_ext_fenics = q_abs_fenics + q_sca_fenics

# Error calculation
err_abs = np.abs(q_abs_analyt - q_abs_fenics) / q_abs_analyt
err_sca = np.abs(q_sca_analyt - q_sca_fenics) / q_sca_analyt
err_ext = np.abs(q_ext_analyt - q_ext_fenics) / q_ext_analyt

# Check if errors are smaller than 1%
assert err_abs < 0.01
assert err_sca < 0.01
assert err_ext < 0.01

if domain.comm.rank == 0:
    print()
    print(f"The analytical absorption efficiency is {q_abs_analyt}")
    print(f"The numerical absorption efficiency is {q_abs_fenics}")
    print(f"The error is {err_abs * 100}%")
    print()
    print(f"The analytical scattering efficiency is {q_sca_analyt}")
    print(f"The numerical scattering efficiency is {q_sca_fenics}")
    print(f"The error is {err_sca * 100}%")
    print()
    print(f"The analytical extinction efficiency is {q_ext_analyt}")
    print(f"The numerical extinction efficiency is {q_ext_fenics}")
    print(f"The error is {err_ext * 100}%")
