Scattering cross-section calculation#

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This tutorial will show you how to compute the radar cross section (RCS) for a dielectric sphere by sampling scattered near fields on a closed surface surrounding the sphere, and transforming them to observation points far away.

This example demonstrates the usefulness of the near field to far field transformation for reducing the simulation size needed for structures involving lots of empty space.

To obtain the scattered field, we will run two simulations: * one with the sphere to compute the total near field on a closed surface around the sphere, and * one without the sphere, to compute just the incident field and subtract it from the above to get the scattered field.

Note that in the future, this process will be simplified with the introduction of a total-field/scattered-field source, requiring only one simulation. Stay tuned!

Then, we’ll show how to use a near-field to far-field transformation in Tidy3D to compute the RCS for the sphere either on the cloud during the simulation run, or on your local machine afterwards.

[1]:
# standard python imports
import numpy as np
import matplotlib.pyplot as plt

# tidy3d imports
import tidy3d as td
import tidy3d.web as web

[23:02:08] WARNING  This version of Tidy3D was pip installed from the 'tidy3d-beta' repository on   __init__.py:102
                    PyPI. Future releases will be uploaded to the 'tidy3d' repository. From now on,                
                    please use 'pip install tidy3d' instead.                                                       
           INFO     Using client version: 1.8.2                                                     __init__.py:120

Define Simulation Parameters#

We first need to define our simulation parameters and the structure.

[2]:
# radius and location of the sphere
radius = 0.5
center = [0, 0, 0]

# permittivity of the sphere
epsr = 4

# free space central wavelength
wavelength = (2.0 * radius) / 2.0
f0 = td.C_0 / wavelength

# distance between the surface of the sphere and the start of the PML layers along each cartesian direction
buffer_PML = 3 * wavelength

# distance between the sphere and the near field monitor along each cartesian direction
buffer_mon = 1 * wavelength

# Define material properties
air = td.Medium(permittivity=1)
diel = td.Medium(permittivity=epsr)

# resolution control
min_steps_per_wvl = 24

# create the sphere
sphere = td.Structure(geometry=td.Sphere(center=center, radius=radius), medium=diel)
geometry = [sphere]

# define PML layers on all sides
boundary_spec = td.BoundarySpec.all_sides(boundary=td.PML())

# set the domain size in x, y, and z
domain_size = buffer_PML + 2 * radius + buffer_PML

# construct simulation size array
sim_size = (domain_size, domain_size, domain_size)

Create Source#

For our incident field, we create a plane wave incident from below the sphere polarized in the x direction.

[3]:
# Bandwidth in Hz
fwidth = f0 / 10.0

# Gaussian source offset; the source peak is at time t = offset/fwidth
offset = 4.0

# time dependence of source
gaussian = td.GaussianPulse(freq0=f0, fwidth=fwidth, offset=offset)

# place the source below the sphere, propagating in the +z direction
source = td.PlaneWave(
    center=(0, 0, -(radius + 3 * buffer_PML / 4)),
    size=(td.inf, td.inf, 0),
    source_time=gaussian,
    direction="+",
    pol_angle=0,
)

# Simulation run time past the source decay (around t=2*offset/fwidth)
run_time = 100 / fwidth

Create Monitors#

Next, we define the monitors that will capture the near field data.

First, we create a FieldMonitor completely enclosing the sphere, using the .surfaces() method to extract the 6 planar surfaces surrounding the volume. This cuts down on the data required vs computing the full volume because only the fields on the enclosing surface are required to get the far field information.

The near fields will be captured on these surfaces; after the simulation, they will be used to compute far fields on your local machine.

[4]:
# create a set of surface monitors around the sphere for local computation of far fields
mon_size = 2 * radius + 2 * buffer_mon
monitors_near = td.FieldMonitor.surfaces(
    center=center, size=[mon_size, mon_size, mon_size], freqs=[f0], name="near_field"
)

Next, we’ll make a FieldProjectionAngleMonitor which is used for computing far-fields directly on the server during the simulation run with Tidy3D’s full hardware optimization, making it extremely fast. Note that in this case, surfaces() must not be used because the solver already knows to use only surface tangential fields to compute the far fields.

With this approach, the near-field data associated with the monitor is used to compute the far fields, and only the far field data is downloaded and returned to the user. Then, we’ll show how to easily and quickly retrieve various quantities such as power and radar cross section from the computed far fields.

Note that for server-side calculation of far fields, this is the only monitor required. The monitor’s size and center fields specify the location where near fields will be sampled, while its theta and phi fields specify the far-field observation angles. Therefore, all the information needed is contained within FieldProjectionAngleMonitor (one can also use FieldProjectionCartesianMonitor or FieldProjectionKSpaceMonitor to specify the far-field observation grid in different coordinate systems).

[5]:
# set the far-field observation angles of interest
num_theta = 300
num_phi = 2
thetas = np.linspace(0, np.pi, num_theta)
phis = np.linspace(0, np.pi / 2, num_phi)

# create the far field monitor for server-side computation of far fields
monitor_far = td.FieldProjectionAngleMonitor(
    center=center,
    size=[mon_size, mon_size, mon_size],
    freqs=[f0],
    name="far_field",
    custom_origin=center,
    phi=list(phis),
    theta=list(thetas),
    far_field_approx=True,  # we leave this to its default value of 'True' because we are interested in fields sufficiently
    # far away that the far field approximations can be invoked to speed up the calculation
)

Let’s also create another near-field monitor where the fields are automatically downsampled based on given sampling rates. The rationale is that we may be able to approximate the far fields fairly well even if the resolution of near-fields is not very fine. This downsampled is achieved by supplying the interval_space field in the FieldMonitor, and can be useful for further reducing the amount of data that needs to be downloaded from the server, while still leading to accurate far fields, as shown below.

Here, we downsample by a factor of 2 along the x and y dimensions, and a factor of 3 along z.

Note that the downsampling feature can be useful if downloading near fields to compute far fields on your local machine, but is unnecessary if you choose to use server-side far field computations.

[6]:
# create a set of surface monitors around the sphere
monitors_downsampled = td.FieldMonitor.surfaces(
    center=center,
    size=[mon_size, mon_size, mon_size],
    freqs=[f0],
    name="near_field_downsampled",
    interval_space=(
        2,
        2,
        3,
    ),  # these are the (x, y, z) factors by which fields are downsampled
)

Create Simulation#

Now we can put everything together and define the two simulation classes: with the sphere to get the total field, and without the sphere to get the incident field. A uniform grid with a fixed grid size is used in both simulations to allow easily subtracting the incident field in the empty simulation from the total field in the actual simulation. We will also apply symmetries which reduce the computational complexity of the problem.

[7]:
monitors = monitors_near + [monitor_far] + monitors_downsampled

sim = td.Simulation(
    size=sim_size,
    grid_spec=td.GridSpec.auto(min_steps_per_wvl=min_steps_per_wvl),
    structures=geometry,
    sources=[source],
    monitors=monitors,
    run_time=run_time,
    boundary_spec=boundary_spec,
    symmetry=(-1, 1, 0),
)

# Here, we add the sphere as an override structure for the messhing such
# that the grids of the two simulations match.
sim_empty = td.Simulation(
    size=sim_size,
    grid_spec=td.GridSpec.auto(
        min_steps_per_wvl=min_steps_per_wvl,
        override_structures=geometry,
    ),
    structures=[],
    sources=[source],
    monitors=monitors,
    run_time=run_time,
    boundary_spec=boundary_spec,
    symmetry=(-1, 1, 0),
)

Visualize Geometry#

Let’s take a look and make sure everything is defined properly in both simulations.

[8]:
fig, (ax1, ax2) = plt.subplots(1, 2, figsize=(9, 3))
sim.plot(y=0, ax=ax1)
sim_empty.plot(y=0, ax=ax2)

           INFO     Auto meshing using wavelength 0.5000 defined from sources.                     grid_spec.py:510
           INFO     Auto meshing using wavelength 0.5000 defined from sources.                     grid_spec.py:510
[8]:
<AxesSubplot: title={'center': 'cross section at y=0.00'}, xlabel='x', ylabel='z'>
../_images/notebooks_Near2FarSphereRCS_15_3.png

Run Simulations#

Now we can run both simulations over time and measure the results

[9]:
# Run simulation
import tidy3d.web as web

sim_data = web.run(sim, task_name="sphereRCS", path="data/sphereRCS.hdf5")
sim_empty_data = web.run(
    sim_empty, task_name="sphereRCS_empty", path="data/sphereRCS_empty.hdf5"
)

           INFO     Using Tidy3D credentials from stored file.                                           auth.py:70
[23:02:12] INFO     Authentication successful.                                                           auth.py:30
[23:02:13] INFO     Created task 'sphereRCS' with task_id 'db541248-d795-4c2f-95de-a0f8f6b76173'.     webapi.py:120
[23:02:16] INFO     Maximum FlexUnit cost: 0.125                                                      webapi.py:252
           INFO     status = queued                                                                   webapi.py:261
[23:02:18] INFO     status = preprocess                                                               webapi.py:273
[23:02:22] INFO     starting up solver                                                                webapi.py:277
[23:02:33] INFO     running solver                                                                    webapi.py:283
[23:03:23] INFO     early shutoff detected, exiting.                                                  webapi.py:294
           INFO     status = postprocess                                                              webapi.py:300
[23:03:33] INFO     status = success                                                                  webapi.py:306
           INFO     Billed FlexUnit cost: 0.075                                                       webapi.py:310
           INFO     downloading file "output/monitor_data.hdf5" to "data/sphereRCS.hdf5"              webapi.py:592
[23:03:35] INFO     loading SimulationData from data/sphereRCS.hdf5                                   webapi.py:414
[23:03:36] INFO     Created task 'sphereRCS_empty' with task_id                                       webapi.py:120
                    'fd730b37-0095-49b7-8192-27e83c511de0'.                                                        
[23:03:39] INFO     Maximum FlexUnit cost: 0.125                                                      webapi.py:252
           INFO     status = queued                                                                   webapi.py:261
[23:03:42] INFO     status = preprocess                                                               webapi.py:273
[23:03:46] INFO     starting up solver                                                                webapi.py:277
[23:03:55] INFO     running solver                                                                    webapi.py:283
[23:03:57] INFO     early shutoff detected, exiting.                                                  webapi.py:294
           INFO     status = postprocess                                                              webapi.py:300
[23:04:05] INFO     status = success                                                                  webapi.py:306
[23:04:06] INFO     Billed FlexUnit cost: 0.025                                                       webapi.py:310
           INFO     downloading file "output/monitor_data.hdf5" to "data/sphereRCS_empty.hdf5"        webapi.py:592
[23:04:08] INFO     loading SimulationData from data/sphereRCS_empty.hdf5                             webapi.py:414

Setting Up the Local Near2Far Computation#

To set up the near-to-far transformation locally, we need to grab the fields on each surface of the near-field FieldMonitor objects.

So, we simply create a FieldProjector object and pass in the surface monitors as shown below. Note that we also need to pass the normal directions of each of the monitors in the list.

In addition to storing the near field data, this object will compute the surface currents and provide various methods for projecting the far field quantities.

We can optionally pass in the number of points per wavelength in the background medium with which to sample fields on the monitors. The default is 10 points per wavelength. This can reduce computation times significantly. By default, 10 points per wavelength are used.

One can also pass in coordinates for the local origin of the set of monitors; the far-field observation points will be defined with respect to this origin. By default, the local origin is set to the average of the centers of all surface monitors passed in.

To see the usefulness of downsampling the fields recorded on monitors, we’ll also run the near-to-far transformation with downsampled fields to compare the RCS.

Finally, to get a sense of performance, we’ll measure the time it takes to compute the far fields locally, and compare it to the time it took to compute them on the server.

[10]:
import time

# first, we construct the classes which compute far fields locally on your machine
n2f = td.FieldProjector.from_near_field_monitors(
    sim_data=sim_data,
    near_monitors=monitors_near,  # only supply the non-downsampled surface monitors as sources
    normal_dirs=["-", "+", "-", "+", "-", "+"],
    pts_per_wavelength=10,
)

# do the same for the downsampled monitors
n2f_downsampled = td.FieldProjector.from_near_field_monitors(
    sim_data=sim_data,
    near_monitors=monitors_downsampled,  # only supply the downsampled surface monitors as sources
    normal_dirs=["-", "+", "-", "+", "-", "+"],
    pts_per_wavelength=10,
)

# we'll also project the fields from the empty simulation into the far field to get the scattered far field
n2f_empty = td.FieldProjector.from_near_field_monitors(
    sim_data=sim_empty_data,
    near_monitors=monitors_near,  # only supply the non-downsampled surface monitors as sources
    normal_dirs=["-", "+", "-", "+", "-", "+"],
    pts_per_wavelength=10,
)

# now, we retrieve the far fields in all three cases by passing in our far field monitor from before
start = time.time()
far_fields = n2f.project_fields(monitor_far)
end = time.time()
n2f_time = end - start

start = time.time()
far_fields_downsampled = n2f_downsampled.project_fields(monitor_far)
end = time.time()
n2f_downsampled_time = end - start

start = time.time()
far_fields_empty = n2f_empty.project_fields(monitor_far)
end = time.time()
n2f_empty_time = end - start

Performance comparison#

We can see below that the local computation of far fields takes about the same time with and without downsampling, because the fields are anyway resampled on the near-field box prior to the computation. The real benefit of downsampling is reducing the amount of data that is stored and downloaded.

The server-side computation is extremely fast, as expected, and requires downloading no near-field data.

[11]:
# use the simulation log to find the time taken for server-side computations
n2f_server_time = float(
    sim_data.log.split("Field projection time (s):    ", 1)[1].split("\n", 1)[0]
)

print(f"Local near-to-far: {n2f_time} s")
print(f"Local near-to-far with downsampling: {n2f_downsampled_time} s")
print(f"Server-side near-to-far: {n2f_server_time} s")

Local near-to-far: 1.0027320384979248 s
Local near-to-far with downsampling: 0.7080271244049072 s
Server-side near-to-far: 0.0799 s

Get Far Field Data for the Server-Side Computations#

Recall that we also computed scattered far fields on the server; let’s extract that data too.

[12]:
far_fields_server = sim_data[monitor_far.name]
far_fields_empty_server = sim_empty_data[monitor_far.name]

Get Scattered Far Fields#

Now, for both client- and server-side fields, compute the scattered far fields by subtracting out the results of the empty simulation.

[13]:
# scattered fields for client-side projections
for field, field_empty in zip(
    far_fields.field_components.values(), far_fields_empty.field_components.values()
):
    field.values -= field_empty.values

# scattered fields for server-side projections
for field, field_empty in zip(
    far_fields_server.field_components.values(),
    far_fields_empty_server.field_components.values(),
):
    field.values -= field_empty.values

Compute the RCS#

Now that we have the far fields computed in three different ways (locally, locally with downsampling, and remotely on the server), various far field quantities can be extracted.

For this example, we use FieldProjectionAngleData.radar_cross_section to get the RCS at the previously-specified theta,phi points.

[14]:
# get the RCS for the local, local downsampled and server-side cases
RCS = far_fields.radar_cross_section.sel(f=f0).values
RCS_downsampled = far_fields_downsampled.radar_cross_section.sel(f=f0).values
RCS_server = far_fields_server.radar_cross_section.sel(f=f0).values

Plot Results#

Now we can plot the RCS and compare it to the analytical RCS computed via the Mie series.

The results match very well! As expected, there are minor deviations due to the FDTD discretization.

Notice that the downsampled monitors also yield fairly accurate results with less than an eighth of the data.

[15]:
def to_db(val):
    val = np.abs(val) / np.max(np.abs(val))
    return 10.0 * np.log10(val)


RCS_phi0 = RCS[0, :, 0]
RCS_phi90 = RCS[0, :, 1]

RCS_downsampled_phi0 = RCS_downsampled[0, :, 0]
RCS_downsampled_phi90 = RCS_downsampled[0, :, 1]

RCS_server_phi0 = RCS_server[0, :, 0]
RCS_server_phi90 = RCS_server[0, :, 1]

# ------ import analytical data from disk ------

mie_file_id = "2lambda_epsr4"
mie_filename_phi0 = "./data/mie_bRCS_phi0_" + mie_file_id + ".txt"
mie_filename_phi90 = "./data/mie_bRCS_phi90_" + mie_file_id + ".txt"

mie_data_phi0 = np.loadtxt(mie_filename_phi0, delimiter="\t", skiprows=2)
mie_theta_phi0 = np.squeeze(mie_data_phi0[:, [0]])
mie_phi0 = np.squeeze(mie_data_phi0[:, [1]])

mie_data_phi90 = np.loadtxt(mie_filename_phi90, delimiter="\t", skiprows=2)
mie_theta_phi90 = np.squeeze(mie_data_phi90[:, [0]])
mie_phi90 = np.squeeze(mie_data_phi90[:, [1]])

# ------ plot for phi = 0 ------

fig, ax = plt.subplots(figsize=(7.5, 5))

ax.plot(mie_theta_phi0, to_db(mie_phi0), "-k", label="$\\phi = 0$, Mie")
ax.plot(thetas, to_db(RCS_phi0), "--b", label="$\\phi = 0$, near2far local")
ax.plot(
    thetas,
    to_db(RCS_downsampled_phi0),
    "--r",
    label="$\\phi = 0$, near2far local downsampled",
)
ax.plot(thetas, to_db(RCS_server_phi0), "--g", label="$\\phi = 0$, near2far server")
ax.set(
    xlabel="$\\theta$ (degrees)",
    ylabel="Bistatic RCS (dBsm)",
    yscale="linear",
    xscale="linear",
)
ax.grid(visible=True, which="both", axis="both", linewidth=0.4)
plt.legend(loc="best", prop={"size": 14})
plt.tight_layout()

# ------ plot for phi = pi/2 ------

fig, ax = plt.subplots(figsize=(7.5, 5))

ax.plot(mie_theta_phi90, to_db(mie_phi90), "-k", label="$\\phi = \\pi/2$, Mie")
ax.plot(thetas, to_db(RCS_phi90), "--b", label="$\\phi = \\pi/2$, near2far local")
ax.plot(
    thetas,
    to_db(RCS_downsampled_phi90),
    "--r",
    label="$\\phi = \\pi/2$, near2far local downsampled",
)
ax.plot(
    thetas, to_db(RCS_server_phi90), "--g", label="$\\phi = \\pi/2$, near2far server"
)
ax.set(
    xlabel="$\\theta$ (degrees)",
    ylabel="Bistatic RCS (dBsm)",
    yscale="linear",
    xscale="linear",
)
ax.grid(visible=True, which="both", axis="both", linewidth=0.4)
plt.legend(loc="best", prop={"size": 14})
plt.tight_layout()

../_images/notebooks_Near2FarSphereRCS_29_0.png
../_images/notebooks_Near2FarSphereRCS_29_1.png
[ ]: