Near to Far Field Spectra

We demonstrate Meep's near-to-far field transformation feature using four different examples. There are three steps involved in this type of calculation. First, we need to define the "near" surface(s) as a set of surfaces capturing all outgoing radiation in the desired direction(s). Second, we run the simulation using a pulsed source (or alternatively, a CW source via the frequency-domain solver) to allow Meep to accumulate the Fourier transforms on the near surface(s). Third, we have Meep compute the far fields at any desired points with the option to save the far fields to an HDF5 file.

Radiation Pattern of an Antenna

In this example, we compute the radiation pattern of an antenna. This involves an electric-current point dipole emitter in vacuum. The source is placed at the center of a 2d cell surrounded by PML. The near fields are obtained on a bounding box defined along the edges of the non-PML region. The far fields are computed in two ways from closed surfaces: (1) sides of a square and (2) circumference of a circle, having a length/radius many times larger than the source wavelength and lying beyond the cell. From both the near and far fields, we will also compute the total outgoing Poynting flux and demonstrate that they are equivalent. Results will be shown for three orthogonal polarizations of the input source.

The simulation geometry is shown in the following schematic.

In the first part of the simulation, we define the cell and source as well as the near field and flux regions. Since we are using a pulsed source (with center wavelength of 1 μm), the fields are timestepped until they have sufficiently decayed away.

The simulation script is in examples/ The notebook is examples/antenna-radiation.ipynb.

import meep as mp
import math
import numpy as np
import matplotlib.pyplot as plt

resolution = 50  # pixels/um

sxy = 4
dpml = 1
cell = mp.Vector3(sxy+2*dpml,sxy+2*dpml,0)

pml_layers = [mp.PML(dpml)]

fcen = 1.0
df = 0.4
src_cmpt = mp.Ez
sources = [mp.Source(src=mp.GaussianSource(fcen,fwidth=df),

if src_cmpt == mp.Ex:
    symmetries = [mp.Mirror(mp.X,phase=-1),
elif src_cmpt == mp.Ey:
    symmetries = [mp.Mirror(mp.X,phase=+1),
elif src_cmpt == mp.Ez:
    symmetries = [mp.Mirror(mp.X,phase=+1),

sim = mp.Simulation(cell_size=cell,

nearfield_box = sim.add_near2far(fcen, 0, 1,
                                 mp.Near2FarRegion(mp.Vector3(y=0.5*sxy), size=mp.Vector3(sxy)),
                                 mp.Near2FarRegion(mp.Vector3(y=-0.5*sxy), size=mp.Vector3(sxy), weight=-1),
                                 mp.Near2FarRegion(mp.Vector3(0.5*sxy), size=mp.Vector3(y=sxy)),
                                 mp.Near2FarRegion(mp.Vector3(-0.5*sxy), size=mp.Vector3(y=sxy), weight=-1))

flux_box = sim.add_flux(fcen, 0, 1,
                        mp.FluxRegion(mp.Vector3(y=0.5*sxy), size=mp.Vector3(sxy)),
                        mp.FluxRegion(mp.Vector3(y=-0.5*sxy), size=mp.Vector3(sxy), weight=-1),
                        mp.FluxRegion(mp.Vector3(0.5*sxy), size=mp.Vector3(y=sxy)),
                        mp.FluxRegion(mp.Vector3(-0.5*sxy), size=mp.Vector3(y=sxy), weight=-1)), src_cmpt, mp.Vector3(), 1e-8))

After the time stepping, the flux of the near fields is computed using get_fluxes:

near_flux = mp.get_fluxes(flux_box)[0]

In the first of two cases, the flux of the far fields is computed using the flux routine for a square box of side length 2 mm which is 2000 times larger than the source wavelength. This requires computing the outgoing flux on each of the four sides of the box separately and summing the values. The resolution of the far fields is chosen arbitrarily as 1 point/μm. This means there are 2x106 points per side length.

r = 1000/fcen      # half side length of far-field square box OR radius of far-field circle
res_ff = 1         # resolution of far fields (points/μm)
far_flux_box = (nearfield_box.flux(mp.Y, mp.Volume(center=mp.Vector3(y=r), size=mp.Vector3(2*r)), res_ff)[0]
               - nearfield_box.flux(mp.Y, mp.Volume(center=mp.Vector3(y=-r), size=mp.Vector3(2*r)), res_ff)[0]
               + nearfield_box.flux(mp.X, mp.Volume(center=mp.Vector3(r), size=mp.Vector3(y=2*r)), res_ff)[0]
               - nearfield_box.flux(mp.X, mp.Volume(center=mp.Vector3(-r), size=mp.Vector3(y=2*r)), res_ff)[0])

For the second of two cases, we use the get_farfield routine to compute the far fields by looping over a set of 100 equally-spaced points along the circumference of a circle with radius of 1 mm. The six far field components (E, E, E, H, H, H) are stored as separate arrays of complex numbers. From the far fields at each point , we compute the outgoing or radial flux: , where P and P are the components of the Poynting vector . Note that is always 0 since this is a 2d simulation. The total flux is computed and the three flux values are displayed.

npts = 100         # number of points in [0,2*pi) range of angles
angles = 2*math.pi/npts*np.arange(npts)

E = np.zeros((npts,3),dtype=np.complex128)
H = np.zeros((npts,3),dtype=np.complex128)
for n in range(npts):
    ff = sim.get_farfield(nearfield_box,
    E[n,:] = [np.conj(ff[j]) for j in range(3)]
    H[n,:] = [ff[j+3] for j in range(3)]

Px = np.real(np.multiply(E[:,1],H[:,2])-np.multiply(E[:,2],H[:,1]))
Py = np.real(np.multiply(E[:,2],H[:,0])-np.multiply(E[:,0],H[:,2]))
Pr = np.sqrt(np.square(Px)+np.square(Py))

far_flux_circle = np.sum(Pr)*2*np.pi*r/len(Pr)

print("flux:, {:.6f}, {:.6f}, {:.6f}".format(near_flux,far_flux_box,far_flux_circle))

By Poynting's theorem, the total outgoing flux obtained by integrating around a closed surface should be the same whether it is calculated from the near or far fields (unless there are sources or absorbers in between). The flux of the near fields for the J source is 2.456196 and that for the far fields is 2.458030 (box) and 2.457249 (circle). The ratio of near- to far-field (circle) flux is 0.999571. Similarly, for the J source, the values are 1.227786 (near-field), 1.227651 (far-field box), and 1.227260 (far-field circle). The ratio of near- to far-field (circle) flux is 1.000429. The slight differences in the flux values are due to discretization effects and will decrease as the resolution is increased.

Finally, we plot the radial flux normalized by its maximum value over the entire interval to obtain a range of values between 0 and 1. These are shown below in the linearly-scaled, polar-coordinate plots. The three figures are obtained using separate runs involving a src_cmpt of E, E, and E. As expected, the J and J sources produce dipole radiation patterns while J has a monopole pattern.

ax = plt.subplot(111, projection='polar')

Focusing Properties of a Metasurface Lens

This example demonstrates how to compute the far-field profile at the focal length of a metasurface lens. The lens design, which is also part of the tutorial, is based on a supercell of binary-grating unit cells. For a review of the binary-grating geometry as well as a demonstration of computing its phasemap, see Tutorial/Mode Decomposition/Phase Map of a Subwavelength Binary Grating. The far-field calculation of the lens contains two separate components: (1) compute the phasemap of the unit cell as a function of a single geometric parameter, the duty cycle, while keeping its height and periodicity fixed (1.8 and 0.3 μm), and (2) form the supercell lens by tuning the local phase of each of a variable number of unit cells according to the quadratic formula for planar wavefront focusing. The design wavelength is 0.5 μm and the focal length is 0.2 mm. The input source is an Ez-polarized planewave at normal incidence.

The simulation script is in examples/ The notebook is examples/metasurface_lens.ipynb.

The key to the script is the function grating with three geometric input arguments (periodicity, height, and list of duty cycles) which performs the two main tasks: (1) for a unit cell, it computes the phase (as well as the transmittance) and then translates this value from the range of [-π,π] of Mode Decomposition to [-2π,0] in order to be consistent with the analytic formula for the local phase and (2) for a supercell, it computes the far-field intensity profile around the focal length of the lens.

import meep as mp
import numpy as np
import matplotlib.pyplot as plt

resolution = 50         # pixels/μm

dpml = 1.0              # PML thickness
dsub = 2.0              # substrate thickness
dpad = 2.0              # padding between grating and PML

lcen = 0.5              # center wavelength
fcen = 1/lcen           # center frequency
df = 0.2*fcen           # frequency width

focal_length = 200      # focal length of metalens
spot_length = 100       # far field line length
ff_res = 10             # far field resolution (points/μm)

k_point = mp.Vector3(0,0,0)

glass = mp.Medium(index=1.5)

pml_layers = [mp.PML(thickness=dpml,direction=mp.X)]


def grating(gp,gh,gdc_list):
  sx = dpml+dsub+gh+dpad+dpml
  src_pt = mp.Vector3(-0.5*sx+dpml+0.5*dsub)
  mon_pt = mp.Vector3(0.5*sx-dpml-0.5*dpad)
  geometry = [mp.Block(material=glass,

  num_cells = len(gdc_list)
  if num_cells == 1:
    sy = gp
    cell_size = mp.Vector3(sx,sy,0)

    sources = [mp.Source(mp.GaussianSource(fcen, fwidth=df),

    sim = mp.Simulation(resolution=resolution,

    flux_obj = sim.add_flux(fcen, 0, 1, mp.FluxRegion(center=mon_pt, size=mp.Vector3(y=sy)))

    input_flux = mp.get_fluxes(flux_obj)


    geometry.append(mp.Block(material=glass, size=mp.Vector3(gh,gdc_list[0]*gp,mp.inf), center=mp.Vector3(-0.5*sx+dpml+dsub+0.5*gh)))

    sim = mp.Simulation(resolution=resolution,

    flux_obj = sim.add_flux(fcen, 0, 1, mp.FluxRegion(center=mon_pt, size=mp.Vector3(y=sy)))

    freqs = mp.get_eigenmode_freqs(flux_obj)
    res = sim.get_eigenmode_coefficients(flux_obj, [1], eig_parity=mp.ODD_Z+mp.EVEN_Y)
    coeffs = res.alpha

    mode_tran = abs(coeffs[0,0,0])**2/input_flux[0]
    mode_phase = np.angle(coeffs[0,0,0])
    if mode_phase > 0:
      mode_phase -= 2*np.pi

    return mode_tran, mode_phase

    sy = num_cells*gp
    cell_size = mp.Vector3(sx,sy,0)

    sources = [mp.Source(mp.GaussianSource(fcen, fwidth=df),

    for j in range(num_cells):

    sim = mp.Simulation(resolution=resolution,

    n2f_obj = sim.add_near2far(fcen, 0, 1, mp.Near2FarRegion(center=mon_pt, size=mp.Vector3(y=sy)))

    return abs(sim.get_farfields(n2f_obj, ff_res, center=mp.Vector3(focal_length), size=mp.Vector3(spot_length))['Ez'])**2

In the first of two parts of the calculation, a phasemap of the binary-grating unit cell is generated based on varying the duty cycle from 0.1 to 0.9.

gp = 0.3                       # grating periodicity
gh = 1.8                       # grating height
gdc = np.linspace(0.1,0.9,30)  # grating duty cycle

mode_tran = np.empty((gdc.size))
mode_phase = np.empty((gdc.size))
for n in range(gdc.size):
  mode_tran[n], mode_phase[n] = grating(gp,gh,[gdc[n]])

plt.plot(gdc, mode_tran, 'bo-')
plt.xticks([t for t in np.linspace(0.1,0.9,5)])
plt.xlabel("grating duty cycle")
plt.yticks([t for t in np.linspace(0.96,1.00,5)])

plt.plot(gdc, mode_phase, 'rs-')
plt.xticks([t for t in np.linspace(0.1,0.9,5)])
plt.xlabel("grating duty cycle")
plt.yticks([t for t in np.linspace(-6,0,7)])
plt.title("phase (radians)")


The phasemap is shown below. The left figure shows the transmittance which is nearly unity for all values of the duty cycle; the Fresnel transmittance is 0.96 for the glass-air interface. This is expected since the periodicity is subwavelength. The right figure shows the phase. There is a subregion in the middle of the plot spanning the duty-cycle range of roughly 0.16 to 0.65 in which the phase varies continuously over the full range of -2π to 0. This structural regime is used to design the supercell lens.

In the second part of the calculation, the far-field energy-density profile of three supercell lens designs, comprised of 201, 401, and 801 unit cells, are computed using the quadratic formula for the local phase. Initially, this involves fitting the unit-cell phase data to a finer duty-cycle grid in order to enhance the local-phase interpolation of the supercell. This is important since as the number of unit cells in the lens increases, the local phase via the duty cycle varies more gradually from unit cell to unit cell. However, if the duty cycle becomes too gradual (i.e., less than a tenth of the pixel dimensions), the resolution may also need to be increased in order to improve the accuracy of subpixel smoothing.

gdc_new = np.linspace(0.16,0.65,500)
mode_phase_interp = np.interp(gdc_new, gdc, mode_phase)
print("phase-range:, {:.6f}".format(mode_phase_interp.max()-mode_phase_interp.min()))

phase_tol = 1e-2
num_cells = [100,200,400]
ff_nc = np.empty((spot_length*ff_res,len(num_cells)))

for k in range(len(num_cells)):
  gdc_list = []
  for j in range(-num_cells[k],num_cells[k]+1):
    phase_local = 2*np.pi/lcen * (focal_length-((j*gp)**2 + focal_length**2)**0.5)  # local phase at the center of the j'th unit cell
    phase_mod = phase_local % (-2*np.pi)                                            # restrict phase to [-2*pi,0]
    if phase_mod > mode_phase_interp.max():
      phase_mod = mode_phase_interp.max()
    if phase_mod < mode_phase_interp.min():
      phase_mod = mode_phase_interp.min()
    idx = np.transpose(np.nonzero(np.logical_and(mode_phase_interp > phase_mod-phase_tol, mode_phase_interp < phase_mod+phase_tol)))

  ff_nc[:,k] = grating(gp,gh,gdc_list)

x = np.linspace(focal_length-0.5*spot_length,focal_length+0.5*spot_length,ff_res*spot_length)
plt.semilogy(x,abs(ff_nc[:,0])**2,'bo-',label='num_cells = {}'.format(2*num_cells[0]+1))
plt.semilogy(x,abs(ff_nc[:,1])**2,'ro-',label='num_cells = {}'.format(2*num_cells[1]+1))
plt.semilogy(x,abs(ff_nc[:,2])**2,'go-',label='num_cells = {}'.format(2*num_cells[2]+1))
plt.xlabel('x coordinate (μm)')
plt.ylabel(r'energy density of far-field electric fields, |E$_z$|$^2$')
plt.title('focusing properties of a binary-grating metasurface lens')
plt.legend(loc='upper right')

Shown below is the supercell lens design involving 201 unit cells. Note that even though periodic boundaries are used in the supercell calculation (via the k_point), the choice of cell boundaries in the y (or longitudinal) direction is irrelevant given the finite length of the lens. For example, PMLs could also have been used (at the expense of a larger cell). Although add_near2far does support periodic boundaries (via the nperiods parameter), it is not necessary for this particular example.

The far-field energy-density profile is shown below for the three lens designs. As the number of unit cells increases, the focal spot becomes sharper and sharper. This is expected since the longer the focal length, the bigger the lens required to demonstrate focusing (which means more unit cells). In this example, the largest lens design contains 801 unit cells which corresponds to 0.24 mm or 1.2X the focal length.

Diffraction Spectrum of a Finite Binary Grating

In this example, we compute the diffraction spectrum of a binary phase grating with finite length. To compute the diffraction spectrum of the infinite periodic structure requires mode decomposition; for a demonstration, see Tutorials/Mode Decomposition/Diffraction Spectrum of a Binary Grating which also describes the grating geometry used in this example (i.e., periodicity of 10 μm, height of 0.5 μm, duty cycle of 0.5, and index 1.5 in air). Note that an infinite periodic structure actually has no spatial separation of the diffracted orders; they are all present at every far-field point. The focus of this tutorial is to demonstrate add_near2far's support for periodic boundaries.

The simulation script is in examples/ The notebook is examples/binary_grating_n2f.ipynb.

The simulation involves computing the scattered near fields of a finite-length grating for an Ez-polarized, pulsed planewave source spanning wavelengths of 0.4-0.6 μm at normal incidence. The far fields are then computed for 500 points along a line parallel to the grating axis positioned 100 m away (i.e., ≫ 2D2/λ, the Fraunhofer distance; D=NΛ where N is the number of unit cells and Λ is the grating periodicity, λ is the source wavelength) in the upper half plane of the symmetric finite structure with length corresponding to a 20° cone. The diffraction spectra is computed as the ratio of the energy density of the far fields from two separate runs: (1) an empty cell to obtain the fields from just the incident planewave and (2) a binary-grating unit cell to obtain the scattered fields.

Modeling a finite grating requires specifying the nperiods parameter of add_near2far which sums 2*nperiods+1 Bloch-periodic copies of the near fields. However, because of the way in which the edges of the structure are handled, this approach is only an approximation for a finite periodic surface. We will verify that the error from this approximation is O(1/nperiods) by comparing its result with that of a true finite periodic structure involving multiple periods in a supercell arrangement terminated with a flat surface extending into PML. (There are infinitely many ways to terminate a finite periodic structure, of course, and different choices will have slightly different errors compared to the periodic approximation.)

import meep as mp
import math
import numpy as np
from numpy import linalg as LA
import matplotlib.pyplot as plt

resolution = 25        # pixels/μm

dpml = 1.0             # PML thickness
dsub = 3.0             # substrate thickness
dpad = 3.0             # padding between grating and PML
gp = 10.0              # grating period
gh = 0.5               # grating height
gdc = 0.5              # grating duty cycle

nperiods = 10          # number of unit cells in finite periodic grating

ff_distance = 1e8      # far-field distance from near-field monitor
ff_angle = 20          # far-field cone angle
ff_npts = 500          # number of far-field points

ff_length = ff_distance*math.tan(math.radians(ff_angle))
ff_res = ff_npts/ff_length

sx = dpml+dsub+gh+dpad+dpml
cell_size = mp.Vector3(sx)

pml_layers = [mp.PML(thickness=dpml,direction=mp.X)]

symmetries = [mp.Mirror(mp.Y)]

wvl_min = 0.4           # min wavelength
wvl_max = 0.6           # max wavelength
fmin = 1/wvl_max        # min frequency
fmax = 1/wvl_min        # max frequency
fcen = 0.5*(fmin+fmax)  # center frequency
df = fmax-fmin          # frequency width

src_pt = mp.Vector3(-0.5*sx+dpml+0.5*dsub)
sources = [mp.Source(mp.GaussianSource(fcen, fwidth=df), component=mp.Ez, center=src_pt)]

k_point = mp.Vector3()

glass = mp.Medium(index=1.5)

sim = mp.Simulation(resolution=resolution,

nfreq = 21
n2f_pt = mp.Vector3(0.5*sx-dpml-0.5*dpad)
n2f_obj = sim.add_near2far(fcen, df, nfreq, mp.Near2FarRegion(center=n2f_pt)), mp.Ez, n2f_pt, 1e-9))

ff_source = sim.get_farfields(n2f_obj, ff_res, center=mp.Vector3(ff_distance,0.5*ff_length), size=mp.Vector3(y=ff_length))


### unit cell with periodic boundaries

sy = gp
cell_size = mp.Vector3(sx,sy)

sources = [mp.Source(mp.GaussianSource(fcen, fwidth=df), component=mp.Ez, center=src_pt, size=mp.Vector3(y=sy))]

geometry = [mp.Block(material=glass, size=mp.Vector3(dpml+dsub,mp.inf,mp.inf), center=mp.Vector3(-0.5*sx+0.5*(dpml+dsub))),
            mp.Block(material=glass, size=mp.Vector3(gh,gdc*gp,mp.inf), center=mp.Vector3(-0.5*sx+dpml+dsub+0.5*gh))]

sim = mp.Simulation(resolution=resolution,

n2f_obj = sim.add_near2far(fcen, df, nfreq, mp.Near2FarRegion(center=n2f_pt, size=mp.Vector3(y=sy)), nperiods=nperiods), mp.Ez, n2f_pt, 1e-9))

ff_unitcell = sim.get_farfields(n2f_obj, ff_res, center=mp.Vector3(ff_distance,0.5*ff_length), size=mp.Vector3(y=ff_length))


### finite periodic grating with flat surface termination extending into PML

num_cells = 2*nperiods+1
sy = dpml+num_cells*gp+dpml
cell_size = mp.Vector3(sx,sy)

pml_layers = [mp.PML(thickness=dpml)]

sources = [mp.Source(mp.GaussianSource(fcen, fwidth=df), component=mp.Ez, center=src_pt, size=mp.Vector3(y=sy-2*dpml))]

geometry = [mp.Block(material=glass, size=mp.Vector3(dpml+dsub,mp.inf,mp.inf), center=mp.Vector3(-0.5*sx+0.5*(dpml+dsub)))]

for j in range(num_cells):

sim = mp.Simulation(resolution=resolution,

n2f_obj = sim.add_near2far(fcen, df, nfreq, mp.Near2FarRegion(center=n2f_pt, size=mp.Vector3(y=sy-2*dpml))), mp.Ez, n2f_pt, 1e-9))

ff_supercell = sim.get_farfields(n2f_obj, ff_res, center=mp.Vector3(ff_distance,0.5*ff_length), size=mp.Vector3(y=ff_length))

norm_err = LA.norm(ff_unitcell['Ez']-ff_supercell['Ez'])/nperiods
print("error:, {}, {}".format(nperiods,norm_err))

A plot of (a) the diffraction/far-field spectra and (b) its cross section at a fixed wavelength of 0.5 μm, is generated using the commands below and shown in the accompanying figure for two cases: (1) nperiods = 1 (no tiling; default) and (2) nperiods = 10 (21 copies). Note that because the evenly-spaced points on the line used to compute the far fields are mapped to angles in the plot, the angular data is not evenly spaced. A similar non-uniformity occurs when transforming the far-field data from the frequency to wavelength domain.

freqs = mp.get_near2far_freqs(n2f_obj)
wvl = np.divide(1,freqs)
ff_lengths = np.linspace(0,ff_length,ff_npts)
angles = [math.degrees(math.atan(f)) for f in ff_lengths/ff_distance]

wvl_slice = 0.5
idx_slice = np.where(np.asarray(freqs) == 1/wvl_slice)[0][0]

rel_enh = np.absolute(ff_unitcell['Ez'])**2/np.absolute(ff_source['Ez'])**2


plt.xlabel("wavelength (μm)")
plt.ylabel("angle (degrees)")
plt.xticks([t for t in np.arange(wvl_min,wvl_max+0.1,0.1)])
plt.yticks([t for t in range(0,ff_angle+1,10)])
plt.title("far-field spectra")

plt.xticks([t for t in range(0,ff_angle+1,10)])
plt.xlabel("angle (degrees)")
plt.ylabel("relative enhancement")
plt.title("f.-f. spectra @  λ = {:.1} μm".format(wvl_slice))


For the case of nperiods = 1, three diffraction orders are present in the far-field spectra as broad peaks with finite angular width (a fourth peak/order is also visible). When nperiods = 10, the diffraction orders become sharp, narrow peaks. The three diffraction orders are labeled in the right inset of the bottom figure as m=1, 3, and 5 corresponding to angles 2.9°, 8.6°, and 14.5° which, along with the diffraction efficiency, can be computed analytically using scalar theory as described in Tutorials/Mode Decomposition/Diffraction Spectrum of a Binary Grating. As an additional validation of the simulation results, the ratio of any two diffraction peaks pa/pb (a,b = 1,3,5,...) is consistent with that of its diffraction efficiencies: b2/a2.

Finally, we verify that the error in add_near2far — defined as the L2-norm of the difference of the two far-field datasets from the unit- and super-cell calculations normalized by nperiods — is O(1/nperiods) by comparing results for three values of nperiods: 5, 10, and 20. The error values, which are displayed in the output in the line prefixed by error:, are: 0.0001195599054639075, 5.981324591508146e-05, and 2.989829913961854e-05. The pairwise ratios of these errors is nearly 2 as expected (i.e., doubling nperiods results in halving the error).

For a single process, the far-field calculation in both runs takes roughly the same amount of time. The wall-clock time is indicated by the getting farfields category of the Field time usage statistics displayed as part of the output after time stepping is complete. Time-stepping a supercell, however, which for nperiods=20 is more than 41 times larger than the unit cell (because of the PML termination) results in a total wall-clock time that is more than 40% larger. The slowdown is also due to the requirement of computing 41 times as many Fourier-transformed near fields. Thus, in the case of the unit-cell simulation, the reduced accuracy is a tradeoff for shorter runtime and less storage. In this example which involves multiple output wavelengths, the time for the far-field calculation can be reduced further on a single, shared-memory, multi-core machine via multithreading by compiling Meep with OpenMP and specifying the environment variable OMP_NUM_THREADS to be an integer greater than one prior to execution.

Far-Field Profile of a Cavity

For this demonstration, we will compute the far-field spectra of a resonant cavity mode in a holey waveguide; a structure we had explored in Tutorial/Resonant Modes and Transmission in a Waveguide Cavity. The script is in examples/ The notebook is examples/cavity-farfield.ipynb. The structure is shown at the bottom of the left image below.

center|Schematic of the computational cell for a holey waveguide with cavity showing the location of the "near" boundary surface and the far-field region.

To set this up, we simply remove the last portion of examples/, beginning right after the line:

sim.symmetries.append(mp.Mirror(mp.Y, phase=-1))
sim.symmetries.append(mp.Mirror(mp.X, phase=-1))

and insert the following lines:

d1 = 0.2

sim = mp.Simulation(cell_size=cell,

nearfield = sim.add_near2far(
    fcen, 0, 1,
    mp.Near2FarRegion(mp.Vector3(0, 0.5 * w + d1), size=mp.Vector3(2 * dpml - sx)),
    mp.Near2FarRegion(mp.Vector3(-0.5 * sx + dpml, 0.5 * w + 0.5 * d1), size=mp.Vector3(0, d1), weight=-1.0),
    mp.Near2FarRegion(mp.Vector3(0.5 * sx - dpml, 0.5 * w + 0.5 * d1), size=mp.Vector3(0, d1))

We are creating a "near" bounding surface, consisting of three separate regions surrounding the cavity, that captures all outgoing waves in the top-half of the cell. Note that the x-normal surface on the left has a weight of -1 corresponding to the direction of the outward normal vector relative to the x direction so that the far-field spectra is correctly computed from the outgoing fields, similar to the flux and force features. The parameter d1 is the distance between the edge of the waveguide and the bounding surface, as shown in the schematic above, and we will demonstrate that changing this parameter does not change the far-field spectra which we compute at a single frequency corresponding to the cavity mode.

We then time step the fields until, at a random point, they have sufficiently decayed away as the cell is surrounded by PMLs, and output the far-field spectra over a rectangular area that lies outside of the cell:, mp.Hz, mp.Vector3(0.12, -0.37), 1e-8))

d2 = 20
h = 4

sim.output_farfields(nearfield, "spectra-{}-{}-{}".format(d1, d2, h), resolution,
                     mp.Volume(mp.Vector3(0, (0.5 * w) + d2 + (0.5 * h)), size=mp.Vector3(sx - 2 * dpml, h)))

The first item to note is that the far-field region is located outside of the cell, although in principle it can be located anywhere. The second is that the far-field spectra can be interpolated onto a spatial grid that has any given resolution but in this example we used the same resolution as the simulation. Note that the simulation itself used purely real fields but the output, given its analytical nature, contains complex fields. Finally, given that the far-field spectra is derived from the Fourier-transformed fields which includes an arbitrary constant factor, we should expect an overall scale and phase difference in the results obtained using the near-to-far-field feature with those from a corresponding simulation involving the full computational volume. The key point is that the results will be qualitatively but not quantitatively identical. The data will be written out to an HDF5 file having a filename prefix with the values of the three main parameters. This file will includes the far-field spectra for all six field components, including real and imaginary parts.

We run the above modified control file and in post-processing create an image of the real and imaginary parts of H over the far-field region which is shown in insets (a) above. For comparison, we compute the steady-state fields using a larger cell that contains within it the far-field region. This involves a continuous source and complex fields. Results are shown in figure (b) above. The difference in the relative phases among any two points within each of the two field spectra is zero, which can be confirmed numerically. Also, as would be expected, it can be shown that increasing d1 does not change the far-field spectra as long as the results are sufficiently converged. This indicates that discretization effects are irrelevant.

In general, it is tricky to interpret the overall scale and phase of the far fields, because it is related to the scaling of the Fourier transforms of the near fields. It is simplest to use the near2far feature in situations where the overall scaling is irrelevant, e.g. when you are computing a ratio of fields in two simulations, or a fraction of the far field in some region, etcetera.