Python User Interface
This page is a listing of the functions exposed by the Python interface. For a gentler introduction, see Tutorial/Basics. Note that this page is not a complete listing of all functions. In particular, because of the SWIG wrappers, every function in the C++ interface is accessible from the Python module, but not all of these functions are documented or intended for end users. See also the instructions for parallel Meep.
The Python API functions and classes can be found in the meep
module, which should be installed in your Python system by Meep's make install
script. If you installed into a nonstandard location (e.g. your home directory), you may need to set the PYTHONPATH
environment variable as documented in the Installation section. You typically import the meep
module in Python with:
import meep as mp
The Simulation Class
The Simulation
class contains all the attributes that you can set to control various parameters of the Meep computation. The function signature of the Simulation
constructor with its default values is listed here for convenience:
class Simulation(object):
def __init__(self,
accurate_fields_near_cylorigin=False,
boundary_layers=[],
cell_size,
Courant=0.5,
default_material=mp.Medium(),
dimensions=2,
ensure_periodicity=False,
eps_averaging=True,
epsilon_func=None,
epsilon_input_file='',
extra_materials=[],
filename_prefix='',
force_complex_fields=False,
geometry=[],
k_point=False,
load_structure='',
m=0,
material_function=None,
num_chunks=0,
output_single_precision=False,
output_volume=None,
progress_interval=4,
resolution,
sources=[],
subpixel_maxeval=100000,
subpixel_tol=1e4,
symmetries=[],
verbose=False):
All Simulation
attributes are described here in further detail. In brackets after each variable is the type of value that it should hold. The classes, complex datatypes like GeometricObject
, are described in a later subsection. The basic datatypes, like integer
, boolean
, complex
, and string
are defined by Python. Vector3
is a meep
class.
geometry
[ list of GeometricObject
class ]
—
Specifies the geometric objects making up the structure being simulated. When objects overlap, later objects in the list take precedence. Defaults to no objects (empty list).
sources
[ list of Source
class ]
—
Specifies the current sources to be present in the simulation. Defaults to none (empty list).
symmetries
[ list of Symmetry
class ]
—
Specifies the spatial symmetries (mirror or rotation) to exploit in the simulation. Defaults to none (empty list). The symmetries must be obeyed by both the structure and the sources. See also Exploiting Symmetry.
boundary_layers
[ list of PML
class ]
—
Specifies the PML absorbing boundary layers to use. Defaults to none.
cell_size
[ Vector3
]
—
Specifies the size of the computational cell which is centered on the origin of the coordinate system. Any sizes of 0 imply a reduceddimensionality calculation. Strictly speaking, the dielectric function is taken to be uniform along that dimension. A 2d calculation is especially optimized. See dimensions
below. Note: because Maxwell's equations are scale invariant, you can use any units of distance you want to specify the cell size: nanometers, microns, centimeters, whatever. However, it is usually convenient to pick some characteristic lengthscale of your problem and set that length to 1. See also Units. Required argument (no default).
default_material
[Medium
class ]
—
Holds the default material that is used for points not in any object of the geometry list. Defaults to air
(ε=1). See also epsilon_input_file
below.
material_function
[ function ]
—
A Python function that takes a Vector3
and returns a Medium
. See also Medium. Defaults to None
.
epsilon_func
[ function ]
—
A Python function that takes a Vector3
and returns the dielectric constant at that point. See also Medium. Defaults to None
.
epsilon_input_file
[string
]
—
If this string is not empty (the default), then it should be the name of an HDF5 file whose first/only dataset defines a scalar, realvalued, frequencyindependent dielectric function over some discrete grid. Alternatively, the dataset name can be specified explicitly if the string is in the form "filename:dataset". This dielectric function is then used in place of the ε property of default_material
(i.e. where there are no geometry
objects). The grid of the epsilon file dataset need not match the computational grid; it is scaled and/or linearly interpolated as needed to map the file onto the computational cell. The structure is warped if the proportions of the grids do not match. Note: the file contents only override the ε property of the default_material
, whereas other properties (μ, susceptibilities, nonlinearities, etc.) of default_material
are still used.
dimensions
[integer
]
—
Explicitly specifies the dimensionality of the simulation, if the value is less than 3. If the value is 3 (the default), then the dimensions are automatically reduced to 2 if possible when cell_size
in the direction is 0
. If dimensions
is the special value of CYLINDRICAL
, then cylindrical coordinates are used and the and dimensions are interpreted as and , respectively. If dimensions
is 1, then the cell must be along the direction and only and field components are permitted. If dimensions
is 2, then the cell must be in the plane.
m
[number
]
—
For CYLINDRICAL
simulations, specifies that the angular dependence of the fields is of the form (default is m=0
). If the simulation cell includes the origin , then m
must be an integer.
accurate_fields_near_cylorigin
[boolean
]
—
For CYLINDRICAL
simulations with m > 1, compute more accurate fields near the origin at the expense of requiring a smaller Courant factor. Empirically, when this option is set to True
, a Courant factor of roughly or smaller seems to be needed. Default is False
, in which case the , , and fields within m pixels of the origin are forced to zero, which usually ensures stability with the default Courant factor of 0.5, at the expense of slowing convergence of the fields near .
resolution
[number
]
—
Specifies the computational grid resolution in pixels per distance unit. Required argument. No default.
k_point
[False
or Vector3
]
—
If False
(the default), then the boundaries are perfect metallic (zero electric field). If a vector, then the boundaries are Blochperiodic: the fields at one side are times the fields at the other side, separated by the lattice vector . The k_point
vector is specified in Cartesian coordinates in units of 2π/distance. Note: this is different from MPB, equivalent to taking MPB's k_points
through its function reciprocal>cartesian
.
ensure_periodicity
[boolean
]
—
If True
(the default) and if the boundary conditions are periodic (k_point
is not False
), then the geometric objects are automatically repeated periodically according to the lattice vectors which define the size of the computational cell.
eps_averaging
[boolean
]
—
If True
(the default), then subpixel averaging is used when initializing the dielectric function. For details, see Section 3 ("Interpolation and the illusion of continuity") of Computer Physics Communications, Vol. 181, pp. 687702, 2010. The input variables subpixel_maxeval
(default 10^{4}) and subpixel_tol
(default 10^{4}) specify the maximum number of function evaluations and the integration tolerance for subpixel averaging. Increasing/decreasing these, respectively, will cause a more accurate but slower computation of the average ε with diminishing returns for the actual FDTD error.
force_complex_fields
[boolean
]
—
By default, Meep runs its simulations with purely real fields whenever possible. It uses complex fields which require twice the memory and computation if the k_point
is nonzero or if m
is nonzero. However, by setting force_complex_fields
to True
, Meep will always use complex fields.
filename_prefix
[string
]
—
A string prepended to all output filenames. If empty (the default), then Meep uses the name of the current Python file, with ".py" replaced by "" (e.g. foo.py
uses a "foo"
prefix). See also Output File Names.
Courant
[number
]
—
Specify the Courant factor which relates the time step size to the spatial discretization: . Default is 0.5. For numerical stability, the Courant factor must be at most , where is the minimum refractive index (usually 1), and in practice should be slightly smaller.
output_volume
[Volume
class ]
—
Specifies the default region of space that is output by the HDF5 output functions (below); see also the Volume
class which manages meep::volume*
objects. Default is None
, which means that the whole computational cell is output. Normally, you should use the in_volume(...)
function to modify the output volume instead of setting output_volume
directly.
output_single_precision
[boolean
]
—
Meep performs its computations in double precision, and by default its output HDF5 files are in the same format. However, by setting this variable to True
(default is False
) you can instead output in single precision which saves a factor of two in space.
progress_interval
[number
]
—
Time interval (seconds) after which Meep prints a progress message. Default is 4 seconds.
extra_materials
[ list of Medium
class ]
—
By default, Meep turns off support for material dispersion, nonlinearities, and similar properties if none of the objects in geometry
have materials with these properties — since they are not needed, it is faster to omit their calculation. This doesn't work however if you use a material_function
: materials via a userspecified function of position instead of just geometric objects. If your material function only returns a nonlinear material, for example, Meep won't notice this unless you tell it explicitly via extra_materials
. extra_materials
is a list of materials that Meep should look for in the computational cell in addition to any materials that are specified by geometric objects. You should list any materials other than scalar dielectrics that are returned by material_function
here.
load_structure
[string
]
—
If not empty, Meep will load the structure specified by this string. The file must have been created by mp.dump_structure
. Defaults to an empty string. See Load and Dump Structure for more information.
The following require a bit more understanding of the inner workings of Meep to use. See also SWIG Wrappers.
structure
[meep::structure*
]
—
Pointer to the current structure being simulated; initialized by _init_structure
which is called automatically by init_sim()
which is called automatically by any of the run functions. The structure initailization is handled by the Simulation
class, and most users will not need to call _init_structure
.
fields
[meep::fields*
]
—
Pointer to the current fields being simulated; initialized by init_sim()
which is called automatically by any of the run functions.
num_chunks
[integer
]
—
Minimum number of "chunks" (subarrays) to divide the structure/fields into (default 0). Actual number is determined by number of processors, PML layers, etcetera. Mainly useful for debugging.
Predefined Variables
These are available directly via the meep
package.
air
, vacuum
[Medium
class ]
—
Two aliases for a predefined material type with a dielectric constant of 1.
perfect_electric_conductor
or metal
[Medium
class ]
—
A predefined material type corresponding to a perfect electric conductor at the boundary of which the parallel electric field is zero. Technically, .
perfect_magnetic_conductor
[Medium
class ]
—
A predefined material type corresponding to a perfect magnetic conductor at the boundary of which the parallel magnetic field is zero. Technically, .
inf
[number
]
—A big number (10^{20}) to use for "infinite" dimensions of objects.
Constants (Enumerated Types)
Several of the functions/classes in Meep ask you to specify e.g. a field component or a direction in the grid. These should be one of the following constants (which are available directly via the meep
package):
direction
constants
—
Specify a direction in the grid. One of X
, Y
, Z
, R
, P
for , , , , , respectively.
side
constants
—
Specify particular boundary in some direction (e.g. or ). One of Low
or High
.
component
constants
—
Specify a particular field or other component. One of Ex
, Ey
, Ez
, Er
, Ep
, Hx
, Hy
, Hz
, Hy
, Hp
, Hz
, Bx
, By
, Bz
, By
, Bp
, Bz
, Dx
, Dy
, Dz
, Dr
, Dp
, Dielectric
, Permeability
, for , , , , , , , , , , , , , , , , , , , , ε, μ, respectively.
derived_component
constants
—
These are additional components which are not actually stored by Meep but are computed as needed, mainly for use in output functions. One of Sx
, Sy
, Sz
, Sr
, Sp
, EnergyDensity
, D_EnergyDensity
, H_EnergyDensity
for , , , , (components of the Poynting vector ), , , , respectively.
Classes
Classes are complex datatypes with various properties which may have default values. Classes can be "subclasses" of other classes. Subclasses inherit all the properties of their superclass and can be used in any place the superclass is expected.
The meep
package defines several types of classes. The most important of these is the Simulation
class. Classes which are available directly from the meep
package are constructed with:
mp.ClassName(prop1=val1, prop2=val2, ...)
The most numerous are the geometric object classes which are the same as those used in MPB. You can get a list of the available classes (and constants) in the Python interpreter with:
import meep
[x for x in dir(meep) if x[0].isupper()]
More information, including their property types and default values, is available with the standard python help
function: help(mp.ClassName)
.
The following are available directly via the meep
package.
Medium
This class is used to specify the materials that geometric objects are made of. It represents an electromagnetic medium which is possibly nonlinear and/or dispersive. See also Materials. To model a perfectlyconducting metal, use the predefined metal
object, above. To model imperfect conductors, use a dispersive dielectric material. See also the Predefined Variables: metal
, perfect_electric_conductor
, and perfect_magnetic_conductor
.
epsilon
[number
]
—The frequencyindependent isotropic relative permittivity or dielectric constant. Default is 1. You can also use index=n
as a synonym for epsilon=n*n
; note that this is not really the refractive index if you also specify μ, since the true index is .
Using epsilon=ep
is actually a synonym for epsilon_diag=mp.Vector3(ep, ep, ep)
.
epsilon_diag
and epsilon_offdiag
[Vector3
]
—
These properties allow you to specify ε as an arbitrary realsymmetric tensor by giving the diagonal and offdiagonal parts. Specifying epsilon_diag=Vector3(a, b, c)
and/or epsilon_offdiag=Vector3(u, v, w)
corresponds to a relative permittivity ε tensor
\begin{pmatrix} a & u & v \\ u & b & w \\ v & w & c \end{pmatrix}
Default is the identity matrix ( and ).
mu
[number
]
—
The frequencyindependent isotropic relative permeability μ. Default is 1. Using mu=pm
is actually a synonym for mu_diag=mp.Vector3(pm, pm, pm)
.
mu_diag
and mu_offdiag
[Vector3
]
—
These properties allow you to specify μ as an arbitrary realsymmetric tensor by giving the diagonal and offdiagonal parts exactly as for ε above. Default is the identity matrix.
D_conductivity
[number
]
—
The frequencyindependent electric conductivity . Default is 0. You can also specify a diagonal anisotropic conductivity tensor by using the property D_conductivity_diag
which takes a Vector3
to give the tensor diagonal. See also Conductivity.
B_conductivity
[number
]
—
The frequencyindependent magnetic conductivity . Default is 0. You can also specify a diagonal anisotropic conductivity tensor by using the property B_conductivity_diag
which takes a Vector3
to give the tensor diagonal. See also Conductivity.
chi2
[number
]
—
The nonlinear (Pockels) susceptibility . Default is 0. See also Nonlinearity.
chi3
[number
]
—
The nonlinear (Kerr) susceptibility . Default is 0. See also Nonlinearity.
E_susceptibilities
[ list of Susceptibility
class ]
—
List of dispersive susceptibilities (see below) added to the dielectric constant ε in order to model material dispersion. Defaults to none (empty list). See also Material Dispersion.
H_susceptibilities
[ list of Susceptibility
class ]
—
List of dispersive susceptibilities (see below) added to the permeability μ in order to model material dispersion. Defaults to none (empty list). See also Material Dispersion.
material functions
Any function that accepts a Medium
instance can also accept a user defined Python function. This allows you to specify the material as an arbitrary function of position. The function must have one argument, the position Vector3
, and return the material at that point, which should be a Python Medium
instance. This is accomplished by passing a function to the material_function
keyword argument in the Simulation
constructor, or the material
keyword argument in any GeometricObject
constructor.
Instead of the material
or material_function
arguments, you can also use the epsilon_func
keyword argument to Simulation
and GeometricObject
, which takes a function of position that returns the dielectric constant at that point.
Important: If your material function returns nonlinear, dispersive (Lorentzian or conducting), or magnetic materials, you should also include a list of these materials in the extra_materials
input variable (above) to let Meep know that it needs to support these material types in your simulation. For dispersive materials, you need to include a material with the same γ_{n} and μ_{n} values, so you can only have a finite number of these, whereas σ_{n} can vary continuously and a matching σ_{n} need not be specified in extra_materials
. For nonlinear or conductivity materials, your extra_materials
list need not match the actual values of σ or χ returned by your material function, which can vary continuously.
Complex ε and μ: you cannot specify a frequencyindependent complex ε or μ in Meep where the imaginary part is a frequencyindependent loss but there is an alternative. That is because there are only two important physical situations. First, if you only care about the loss in a narrow bandwidth around some frequency, you can set the loss at that frequency via the conductivity. Second, if you care about a broad bandwidth, then all physical materials have a frequencydependent complex ε and/or μ, and you need to specify that frequency dependence by fitting to Lorentzian and/or Drude resonances via the LorentzianSusceptibility
or DrudeSusceptibility
classes below.
Dispersive dielectric and magnetic materials, above, are specified via a list of objects that are subclasses of type Susceptibility
.
Susceptibility
Parent class for various dispersive susceptibility terms, parameterized by an anisotropic amplitude σ. See Material Dispersion.
sigma
[number
]
—
The scale factor σ. You can also specify an anisotropic σ tensor by using the property sigma_diag
which takes three numbers or a Vector3
to give the σ tensor diagonal, and sigma_offdiag
which specifies the offdiagonal elements (defaults to 0). That is, sigma_diag=mp.Vector3(a, b, c)
and sigma_offdiag=mp.Vector3(u, v, w)
corresponds to a σ tensor
\begin{pmatrix} a & u & v \\ u & b & w \\ v & w & c \end{pmatrix}
LorentzianSusceptibility
Specifies a single dispersive susceptibility of Lorentzian (damped harmonic oscillator) form. See Material Dispersion, with the parameters (in addition to σ):
frequency
[number
]
—
The resonance frequency .
gamma
[number
]
—
The resonance loss rate .
DrudeSusceptibility
Specifies a single dispersive susceptibility of Drude form. See Material Dispersion, with the parameters (in addition to σ):
frequency
[number
]
—
The frequency scale factor which multiplies σ (not a resonance frequency).
gamma
[number
]
—
The loss rate .
Meep also supports a somewhat unusual polarizable medium, a Lorentzian susceptibility with a random noise term added into the dampedoscillator equation at each point. This can be used to directly model thermal radiation in both the far field and the near field. Note, however that it is more efficient to compute farfield thermal radiation using Kirchhoff's law of radiation, which states that emissivity equals absorptivity. Nearfield thermal radiation can usually be computed more efficiently using frequencydomain methods, e.g. via SCUFFEM.
NoisyLorentzianSusceptibility or NoisyDrudeSusceptibility
Specifies a single dispersive susceptibility of Lorentzian (damped harmonic oscillator) or Drude form. See Material Dispersion, with the same sigma
, frequency
, and gamma
parameters, but with an additional Gaussian random noise term (uncorrelated in space and time, zero mean) added to the P dampedoscillator equation.
noise_amp
[number
]
—
The noise has rootmean square amplitude σ
noise_amp
.
Vector3
Properties:
x
, y
, z
[float
or complex
]
—
The x
, y
, and z
components of the vector.
Vector3(x=0.0, y=0.0, z=0.0)
—
Create a new Vector3 with the given components. All three components default to zero.
v3 = v1 + v2
v3 = v1  v2
v3 = v1.cross(v2)
Return the sum, difference, or cross product of the two vectors.
c = v1 * b
c = b * v1
If b
is a Vector3
, returns the dot product v1
and b
. If b
is a number, then v1
is scaled by the number.
v3 = v1.dot(v2)
Returns the dot product of v1
and v2
.
v3 = v1.cross(v2)
Returns the cross product of v1
and v2
.
v3 = v1.cdot(v2)
Returns the conjugated dot product: v1* dot v2.
v2 = v1.norm()
Returns the length math.sqrt(abs(v1.dot(v1)))
of the given vector.
v2 = v1.unit()
Returns a unit vector in the direction of v1.
v1.close(v2, [tol])
Returns whether or not the corresponding components of the two vectors are within tol
of each other. Defaults to 1e7.
v1 == v2
Returns whether or not the two vectors are numerically equal. Beware of using this function after operations that may have some error due to the finite precision of floatingpoint numbers; use close
instead.
v2 = v1.rotate(axis, theta)
Returns the vector v1
rotated by an angle theta
(in radians) in the righthand direction around the axis
vector (whose length is ignored). You may find the python functions math.degrees
and math.radians
useful to convert angles between degrees and radians.
GeometricObject
This class, and its descendants, are used to specify the solid geometric objects that form the dielectric structure being simulated. The base class is:
GeometricObject
Properties:
material
[Medium
class or function ]
—
The material that the object is made of (usually some sort of dielectric). Uses default Medium
. If a function is supplied, it must take one argument and return a Python Medium
.
epsilon_func
[ function ]
—
A function that takes one argument (a Vector3
) and returns the dielectric constant at that point. Can be used instead of material
. Default is None
.
center
[Vector3
]
—
Center point of the object. Defaults to (0,0,0)
.
Methods:
shift
(vec [Vector3
])
—
Shifts the objects center
by vec
. This can also be accomplished via the +
operator: geomtric_obj + Vector3(10,10,10)
.
info
(indent_by [integer])
—
Displays all properties and current values of a GeometricObject
, indented by indent_by
spaces (default is 0).
One normally does not create objects of type GeometricObject
directly, however; instead, you use one of the following subclasses. Recall that subclasses inherit the properties of their superclass, so these subclasses automatically have the material
and center
properties and can be specified in a subclass's constructor via keyword arguments.
In a 2d calculation, only the intersections of the objects with the plane are considered.
Sphere
A sphere. Properties:
radius
[number
]
—
Radius of the sphere. No default value.
Cylinder
A cylinder, with circular crosssection and finite height. Properties:
radius
[number
]
—
Radius of the cylinder's crosssection. No default value.
height
[number
]
—
Length of the cylinder along its axis. No default value.
axis
[Vector3
]
—
Direction of the cylinder's axis; the length of this vector is ignored. Defaults to Vector3(x=0, y=0, z=1)
.
Cone
A cone, or possibly a truncated cone. This is actually a subclass of Cylinder
, and inherits all of the same properties, with one additional property. The radius of the base of the cone is given by the radius
property inherited from cylinder
, while the radius of the tip is given by the new property, radius2
. The center
of a cone is halfway between the two circular ends.
radius2
[number
]
—
Radius of the tip of the cone (i.e. the end of the cone pointed to by the axis
vector). Defaults to zero (a "sharp" cone).
Block
A parallelepiped (i.e., a brick, possibly with nonorthogonal axes).
size
[Vector3
]
—
The lengths of the block edges along each of its three axes. Not really a 3vector, but it has three components, each of which should be nonzero. No default value.
e1
, e2
, e3
[Vector3
]
—
The directions of the axes of the block; the lengths of these vectors are ignored. Must be linearly independent. They default to the three lattice directions.
Ellipsoid
An ellipsoid. This is actually a subclass of Block
, and inherits all the same properties, but defines an ellipsoid inscribed inside the block.
Prism
Polygonal prism type.
vertices
[list of Vector3
]
—
The vertices that make up the prism. They must lie in a plane that's perpendicular to the axis
. Note that infinite lengths are not supported. To simulate infinite geometry, just extend the edge of the prism beyond the cell.
height
[number
]
—
The prism thickness, extruded in the direction of axis
. mp.inf
can be used for infinite height.
axis
[Vector3
]
—
The axis perpendicular to the prism. Defaults to Vector3(0,0,1)
.
center
[Vector3
]
—
If center
is not specified, then the coordinates of the vertices
define the bottom of the prism
(with the top of the prism being at the same coordinates shifted by height*axis
).
If center
is specified, then center
is the coordinates of the centroid
of all the vertices (top and bottom) of the resulting 3d prism (so that the coordinates of the vertices
are
shifted accordingly).
These are some examples of geometric objects created using the above classes:
# A cylinder of infinite radius and height 0.25 pointing along the x axis,
# centered at the origin:
cyl = mp.Cylinder(center=mp.Vector3(0,0,0), height=0.25, radius=mp.inf,
axis=mp.Vector3(1,0,0), material=mp.Medium(index=3.5))
# An ellipsoid with its long axis pointing along (1,1,1), centered on
# the origin (the other two axes are orthogonal and have equal
# semiaxis lengths):
ell = mp.Ellipsoid(center=mp.Vector3(0,0,0), size=mp.Vector3(0.8,0.2,0.2),
e1=Vector3(1,1,1), e2=Vector3(0,1,1), e3=Vector3(2,1,1),
material=mp.Medium(epsilon=13))
# A unit cube of material mat with a spherical air hole of radius 0.2 at
# its center, the whole thing centered at (1,2,3):
geometry=[mp.Block(center=Vector3(1,2,3), size=Vector3(1,1,1), material=mp.metal),
mp.Sphere(center=Vector3(1,2,3), radius=0.2, material=mp.air)]
# A hexagon defined as a prism with six vertices centered on the origin
# of material crystalline silicon (from the materials library)
vertices = [mp.Vector3(1,0),
mp.Vector3(0.5,math.sqrt(3)/2),
mp.Vector3(0.5,math.sqrt(3)/2),
mp.Vector3(1,0),
mp.Vector3(0.5,math.sqrt(3)/2),
mp.Vector3(0.5,math.sqrt(3)/2)]
geometry = [mp.Prism(vertices, height=1.5, center=mp.Vector3(), material=cSi)]
Symmetry
This class is used for the symmetries
input variable to specify symmetries which must preserve both the structure and the sources. Any number of symmetries can be exploited simultaneously but there is no point in specifying redundant symmetries: the computational cell can be reduced by at most a factor of 4 in 2d and 8 in 3d. See also Exploiting Symmetry. This is the base class of the specific symmetries below, so normally you don't create it directly. However, it has two properties which are shared by all symmetries:
direction
[direction
constant ]
—
The direction of the symmetry (the normal to a mirror plane or the axis for a rotational symmetry). e.g. X
, Y
, or Z
(only Cartesian/grid directions are allowed). No default value.
phase
[complex
]
—
An additional phase to multiply the fields by when operating the symmetry on them. Default is +1, e.g. a phase of 1 for a mirror plane corresponds to an odd mirror. Technically, you are essentially specifying the representation of the symmetry group that your fields and sources transform under.
The specific symmetry subclasses are:
Mirror
—
A mirror symmetry plane. direction
is the direction normal to the mirror plane.
Rotate2
—
A 180° (twofold) rotational symmetry (a.k.a. ). direction
is the axis of the rotation.
Rotate4
—
A 90° (fourfold) rotational symmetry (a.k.a. ). direction
is the axis of the rotation.
PML
This class is used for specifying the PML absorbing boundary layers around the cell, if any, via the boundary_layers
input variable. See also Perfectly Matched Layers. boundary_layers
can be zero or more PML
objects, with multiple objects allowing you to specify different PML layers on different boundaries. The class represents a single PML layer specification, which sets up one or more PML layers around the boundaries according to the following properties.
thickness
[number
]
—
The spatial thickness of the PML layer which extends from the boundary towards the inside of the computational cell. The thinner it is, the more numerical reflections become a problem. No default value.
direction
[direction
constant ]
—
Specify the direction of the boundaries to put the PML layers next to. e.g. if X
, then specifies PML on the boundaries (depending on the value of side
, below). Default is the special value ALL
, which puts PML layers on the boundaries in all directions.
side
[side
constant ]
—
Specify which side, Low
or High
of the boundary or boundaries to put PML on. e.g. if side is Low
and direction is X
, then a PML layer is added to the boundary. Default is the special value ALL
, which puts PML layers on both sides.
R_asymptotic
[number
]
—
The asymptotic reflection in the limit of infinite resolution or infinite PML thickness, for refections from air (an upper bound for other media with index > 1). For a finite resolution or thickness, the reflection will be much larger, due to the discretization of Maxwell's equation. Default value is 10^{−15}, which should suffice for most purposes. You want to set this to be small enough so that waves propagating within the PML are attenuated sufficiently, but making R_asymptotic
too small will increase the numerical reflection due to discretization.
pml_profile
[function
]
—
By default, Meep turns on the PML conductivity quadratically within the PML layer — one doesn't want to turn it on suddenly, because that exacerbates reflections due to the discretization. More generally, with pml_profile
one can specify an arbitrary PML "profile" function that determines the shape of the PML absorption profile up to an overall constant factor. u goes from 0 to 1 at the start and end of the PML, and the default is . In some cases where a very thick PML is required, such as in a periodic medium (where there is technically no such thing as a true PML, only a pseudoPML), it can be advantageous to turn on the PML absorption more smoothly. See Optics Express, Vol. 16, pp. 1137692, 2008. For example, one can use a cubic profile by specifying pml_profile=lambda u: u*u*u
.
Absorber
Instead of a PML
layer, there is an alternative class called Absorber
which is a dropin replacement for PML
. For example, you can do boundary_layers=[mp.Absorber(thickness=2)]
instead of boundary_layers=[mp.PML(thickness=2)]
. All the parameters are the same as for PML
, above. You can have a mix of PML
on some boundaries and Absorber
on others.
The Absorber
class does not implement a perfectly matched layer (PML), however (except in 1d). Instead, it is simply a scalar electric and magnetic conductivity that turns on gradually within the layer according to the pml_profile
(defaulting to quadratic). Such a scalar conductivity gradient is only reflectionless in the limit as the layer becomes sufficiently thick.
The main reason to use Absorber
is if you have a case in which PML fails:
 No true PML exists for periodic media, and a scalar absorber is cheaper and generally just as good. See Optics Express, Vol. 16, pp. 1137692, 2008.
 PML can lead to divergent fields for certain waveguides with "backwardwave" modes; this can easily happen in metals with surface plasmons, and a scalar absorber is your only choice. See Physical Review E, Vol. 79, 065601, 2009.
 PML can fail if you have a waveguide hitting the edge of your computational cell at an angle. See J. Computational Physics, Vol. 230, pp. 236977, 2011.
Source
The Source
class is used to specify the current sources via the Simulation.sources
attribute. Note that all sources in Meep are separable in time and space, i.e. of the form for some functions and . Nonseparable sources can be simulated, however, by modifying the sources after each time step. When real fields are being used (which is the default in many cases; see Simulation.force_complex_fields
), only the real part of the current source is used.
Important note: These are current sources (J terms in Maxwell's equations), even though they are labelled by electric/magnetic field components. They do not specify a particular electric/magnetic field which would be what is called a "hard" source in the FDTD literature. There is no fixed relationship between the current source and the resulting field amplitudes; it depends on the surrounding geometry, as described in the FAQ and in Section 4.4 ("Currents and Fields: The Local Density of States") in Chapter 4 ("Electromagnetic Wave Source Conditions") of the book Advances in FDTD Computational Electrodynamics: Photonics and Nanotechnology.
Properties:
src
[SourceTime
class ]
—
Specify the timedependence of the source (see below). No default.
component
[component
constant ]
—
Specify the direction and type of the current component: e.g. mp.Ex
, mp.Ey
, etcetera for an electriccharge current, and mp.Hx
, mp.Hy
, etcetera for a magneticcharge current. Note that currents pointing in an arbitrary direction are specified simply as multiple current sources with the appropriate amplitudes for each component. No default.
center
[Vector3
]
—
The location of the center of the current source in the computational cell. No default.
size
[Vector3
]
—
The size of the current distribution along each direction of the computational cell. Default is (0,0,0)
: a pointdipole source.
amplitude
[complex
]
—
An overall complex amplitude multiplying the the current source. Default is 1.0.
amp_func
[function
]
—
A Python function of a single argument, that takes a Vector3
giving a position and returns a complex current amplitude for that point. The position argument is relative to the center
of the current source, so that you can move your current around without changing your function. Default is None
, meaning that a constant amplitude of 1.0 is used. Note that your amplitude function (if any) is multiplied by the amplitude
property, so both properties can be used simultaneously.
amp_func_file
[string
]
—
String of the form path_to_h5_file.h5:dataset
. The .h5
extension is optional. Meep will read the HDF5 file and create an amplitude function that interpolates into the grid specified by the file. Meep expects the data to be split into real and imaginary parts, so in the above example it will look for dataset.re
and dataset.im
in the file path_to_h5_file.h5
. Defaults to the empty string.
amp_data
[numpy.ndarray with dtype=numpy.complex128
]
—
Like amp_func_file
above, but instead of interpolating into an HDF5 file, interpolates into a complex NumPy array. The array should be three dimensions. For a 2d simulation, just pass 1 for the third dimension, e.g., arr = np.zeros((N, M, 1), dtype=np.complex128)
. Defaults to None
.
As described in Section 4.2 ("Incident Fields and Equivalent Currents") in Chapter 4 ("Electromagnetic Wave Source Conditions") of the book Advances in FDTD Computational Electrodynamics: Photonics and Nanotechnology, it is also possible to supply a source that is designed to couple exclusively into a single waveguide mode (or other mode of some cross section or periodic region) at a single frequency, and which couples primarily into that mode as long as the bandwidth is not too broad. This is possible if you have MPB installed: Meep will call MPB to compute the field profile of the desired mode, and uses the field profile to produce an equivalent current source. Note: this feature does not work in cylindrical coordinates. To do this, instead of a source
you should use an EigenModeSource
:
EigenModeSource
This is a subclass of Source
and has all of the properties of Source
above. However, you normally do not specify a component
. Instead of component
, the current source components and amplitude profile are computed by calling MPB to compute the modes of the dielectric profile in the region given by the size
and center
of the source, with the modes computed as if the source region were repeated periodically in all directions. If an amplitude
and/or amp_func
are supplied, they are multiplied by this current profile. The desired eigenmode and other features are specified by the following properties:
eig_band
[integer
]
—
The index n (1,2,3,...) of the desired band ω_{n}(k) to compute in MPB where 1 denotes the lowestfrequency band at a given k point, and so on.
direction
[mp.X
, mp.Y
, or mp.Z;
default mp.AUTOMATIC
], eig_match_freq
[boolean;
default True
], eig_kpoint
[Vector3
]
—
By default (if eig_match_freq
is True
), Meep tries to find a mode with the same frequency ω_{n}(k) as the src
property (above), by scanning k vectors in the given direction
using MPB's find_k
functionality. Alternatively, if eig_kpoint
is supplied, it is used as an initial guess and direction for k. By default, direction
is the direction normal to the source region, assuming size
is –1 dimensional in a dimensional simulation (e.g. a plane in 3d). Alternatively if eig_match_freq
is False
, you can specify a particular k vector of the desired mode with eig_kpoint
(in Meep units of 2π/). (By default, the k components in the plane of the source region are zero. However, if the source region spans the entire computational cell in some directions, and the cell has Blochperiodic boundary conditions via the k_point
parameter, then the mode's k components in those directions will match k_point
so that the mode satisfies the Meep boundary conditions, regardless of eig_kpoint
.)
eig_parity
[mp.NO_PARITY
(default), mp.EVEN_Z
, mp.ODD_Z
, mp.EVEN_Y
, mp.ODD_Y
]
—
The parity (= polarization in 2d) of the mode to calculate, assuming the structure has and/or mirror symmetry in the source region. If the structure has both and mirror symmetry, you can combine more than one of these, e.g. EVEN_Z + ODD_Y
. Default is NO_PARITY
, in which case MPB computes all of the bands which will still be even or odd if the structure has mirror symmetry, of course. This is especially useful in 2d simulations to restrict yourself to a desired polarization.
eig_resolution
[integer
, defaults to same as Meep resolution ]
—
The spatial resolution to use in MPB for the eigenmode calculations. This defaults to the same resolution as Meep, but you can use a higher resolution in which case the structure is linearly interpolated from the Meep pixels.
eig_tolerance
[number
, defaults to 10^{–7} ]
—
The tolerance to use in the MPB eigensolver. MPB terminates when the eigenvalues stop changing to less than this fractional tolerance.
component
[as above, but defaults to ALL_COMPONENTS
]
—
Once the MPB modes are computed, equivalent electric and magnetic sources are created within Mp. By default, these sources include magnetic and electric currents in all transverse directions within the source region, corresponding to the mode fields as described in Section 4.2 ("Incident Fields and Equivalent Currents") in Chapter 4 ("Electromagnetic Wave Source Conditions") of the book Advances in FDTD Computational Electrodynamics: Photonics and Nanotechnology. If you specify a component
property, however, you can include only one component of these currents if you wish. Most users won't need this feature.
eig_lattice_size
[Vector3
], eig_lattice_center
[Vector3
]
—
Normally, the MPB computational unit cell is the same as the source volume given by the size
and center
parameters. However, occasionally you want the unit cell to be larger than the source volume. For example, to create an eigenmode source in a periodic medium, you need to pass MPB the entire unit cell of the periodic medium, but once the mode is computed then the actual current sources need only lie on a cross section of that medium. To accomplish this, you can specify the optional eig_lattice_size
and eig_lattice_center
, which define a volume (which must enclose size
and center
) that is used for the unit cell in MPB with the dielectric function ε taken from the corresponding region in the Meep simulation.
Note that MPB only supports dispersionless nonmagnetic materials but it does support anisotropic ε. Any nonlinearities, magnetic responses μ, conductivities σ, or dispersive polarizations in your materials will be ignored when computing the eigenmode source. PML will also be ignored.
The src_time
object (Source.src
), which specifies the time dependence of the source, can be one of the following three classes.
ContinuousSource
A continuouswave source proportional to , possibly with a smooth (exponential/tanh) turnon/turnoff.
frequency
[number
]
—
The frequency f in units of /distance or ω in units of /distance. See Units. No default value. You can instead specify wavelength=x
or period=x
, which are both a synonym for frequency=1/x
; i.e. 1/ω in these units is the vacuum wavelength or the temporal period.
start_time
[number
]
—
The starting time for the source. Default is 0 (turn on at ).
end_time
[number
]
—
The end time for the source. Default is 10^{20} (never turn off).
width
[number
]
—
Roughly, the temporal width of the smoothing (technically, the inverse of the exponential rate at which the current turns off and on). Default is 0 (no smoothing). You can instead specify fwidth=x
, which is a synonym for width=1/x
(i.e. the frequency width is proportional to the inverse of the temporal width).
cutoff
[number
]
—
How many width
s the current decays for before we cut it off and set it to zero. Default is 3.0. A larger value of cutoff
will reduce the amount of highfrequency components that are introduced by the start/stop of the source, but will of course lead to longer simulation times.
GaussianSource
A Gaussianpulse source roughly proportional to . Technically, the "Gaussian" sources in Meep are the (discretetime) derivative of a Gaussian, i.e. they are , but the difference between this and a true Gaussian is usually irrelevant.
frequency
[number
]
—
The center frequency in units of /distance (or ω in units of /distance). See Units. No default value. You can instead specify wavelength=x
or period=x
, which are both a synonym for frequency=1/x
; i.e. 1/ω in these units is the vacuum wavelength or the temporal period.
width
[number
]
—
The width used in the Gaussian. No default value. You can instead specify fwidth=x
, which is a synonym for width=1/x
(i.e. the frequency width is proportional to the inverse of the temporal width).
start_time
[number
]
—
The starting time for the source; default is 0 (turn on at ). This is not the time of the peak. See below.
cutoff
[number
]
—
How many width
s the current decays for before we cut it off and set it to zero — this applies for both turnon and turnoff of the pulse. Default is 5.0. A larger value of cutoff
will reduce the amount of highfrequency components that are introduced by the start/stop of the source, but will of course lead to longer simulation times. The peak of the Gaussian is reached at the time =start_time + cutoff*width
.
CustomSource
A userspecified source function . You can also specify start/end times at which point your current is set to zero whether or not your function is actually zero. These are optional, but you must specify an end_time
explicitly if you want run
functions like until_after_sources
to work, since they need to know when your source turns off.
src_func
[function
]
—
The function specifying the timedependence of the source. It should take one argument (the time in Meep units) and return a complex number.
start_time
[number
]
—
The starting time for the source. Default is 10^{20}: turn on at . Note, however, that the simulation normally starts at with zero fields as the initial condition, so there is implicitly a sharp turnon at whether you specify it or not.
end_time
[number
]
—
The end time for the source. Default is 10^{20} (never turn off).
FluxRegion
A FluxRegion
object is used with add_flux
to specify a region in which Meep should accumulate the appropriate Fouriertransformed fields in order to compute a flux spectrum. It represents a region (volume, plane, line, or point) in which to compute the integral of the Poynting vector of the Fouriertransformed fields. ModeRegion
is an alias for FluxRegion
for use with add_mode_monitor
.
Properties:
center
[Vector3
]
—The center of the flux region (no default).
size
[Vector3
]
—The size of the flux region along each of the coordinate axes. Default is (0,0,0)
; a single point.
direction
[direction
constant ]
—The direction in which to compute the flux (e.g. mp.X
, mp.Y
, etcetera). Default is AUTOMATIC
, in which the direction is determined by taking the normal direction if the flux region is a plane (or a line, in 2d). If the normal direction is ambiguous (e.g. for a point or volume), then you must specify the direction
explicitly (not doing so will lead to an error).
weight
[complex
]
—A weight factor to multiply the flux by when it is computed. Default is 1.0.
Note that the flux is always computed in the positive coordinate direction, although this can effectively be flipped by using a weight
of 1.0. This is useful, for example, if you want to compute the outward flux through a box, so that the sides of the box add instead of subtract.
Volume
Many Meep functions require you to specify a volume in space, corresponding to the C++ type meep::volume
. This class creates such a volume object, given the center
and size
properties (just like e.g. a Block
object). If the size
is not specified, it defaults to (0,0,0)
, i.e. a single point. Any method that accepts such a volume also accepts center
and size
keyword arguments. If these are specified instead of the volume, the library will construct a volume for you.
Miscellaneous Functions
Output File Names
The output filenames used by Meep, e.g. for HDF5 files, are automatically prefixed by the input variable filename_prefix
. If filename_prefix
is empty (the default), however, then Meep constructs a default prefix based on the current Python filename with ".py"
replaced by ""
: e.g. test.py
implies a prefix of "test"
. You can get this prefix by running:
Simulation.get_filename_prefix()
—
Return the current prefix string that is prepended, by default, to all file names.
If you don't want to use any prefix, then you should set filename_prefix
to False
.
In addition to the filename prefix, you can also specify that all the output files be written into a newlycreated directory (if it does not yet exist). This is done by running:
Simulation.use_output_directory([dirname])
—
Put output in a subdirectory, which is created if necessary. If the optional argument dirname is specified, that is the name of the directory. Otherwise, the directory name is the current Python file name with ".py"
replaced by "out"
: e.g. test.py
implies a directory of "testout"
.
Simulation Time
Simulation.meep_time()
—
Return the current simulation time in simulation time units (e.g. during a run function). This is not the wallclock time.
Occasionally, e.g. for termination conditions of the form time < T?, it is desirable to round the time to single precision in order to avoid small differences in roundoff error from making your results different by one timestep from machine to machine (a difference much bigger than roundoff error); in this case you can call Simulation.round_time()
instead, which returns the time rounded to single precision.
Field Computations
Meep supports a large number of functions to perform computations on the fields. Most of them are accessed via the lowerlevel C++/SWIG interface. Some of them are based on the following simpler, higherlevel versions. They are accessible as methods of a Simulation
instance.
get_field_point(c, pt)
—
Given a component
or derived_component
constant c
and a Vector3
pt
, returns the value of that component at that point.
get_epsilon_point(pt)
—
Equivalent to get_field_point(mp.Dielectric, pt)
.
add_dft_fields(cs, freq_min, freq_max, nfreq, where=None, center=None, size=None)
—
Given a list of field components cs
, compute the Fourier transform of these fields for nfreq
equally spaced frequencies covering the frequency range freq_min
to freq_max
over the Volume
specified by where
(default to the entire computationall cell). The volume can also be specified via the center
and size
arguments.
flux_in_box(dir, box=None, center=None, size=None)
—
Given a direction
constant, and a mp.Volume
, returns the flux (the integral of ) in that volume. Most commonly, you specify a volume that is a plane or a line, and a direction perpendicular to it, e.g. flux_in_box(d=mp.X,mp.Volume(center=mp.Vector3(0,0,0),size=mp.Vector3(0,1,1)))
. If the center
and size
arguments are provided instead of box
, meep will construct the appropriate volume for you.
electric_energy_in_box(box=None, center=None, size=None)
—
Given a mp.Volume
, returns the integral of the electricfield energy in the given volume. If the volume has zero size along a dimension, a lowerdimensional integral is used. If the center
and size
arguments are provided instead of box
, meep will construct the appropriate volume for you.
magnetic_energy_in_box(box=None, center=None, size=None)
—
Given a mp.Volume
, returns the integral of the magneticfield energy in the given volume. If the volume has zero size along a dimension, a lowerdimensional integral is used. If the center
and size
arguments are provided instead of box
, meep will construct the appropriate volume for you.
field_energy_in_box(box=None, center=None, size=None)
—
Given a mp.Volume
, returns the integral of the electric and magneticfield energy in the given volume. If the volume has zero size along a dimension, a lowerdimensional integral is used. If the center
and size
arguments are provided instead of box
, meep will construct the appropriate volume for you.
modal_volume_in_box(box=None, center=None, size=None)
—
Given a mp.Volume
, returns the instantaneous modal volume according to the Purcelleffect definition: integral (εE^{2}) / maximum (εE^{2}). If no volume argument is provided, the entire computational cell is used by default. If the center
and size
arguments are provided instead of box
, Meep will construct the appropriate volume for you.
Note that if you are at a fixed frequency and you use complex fields (via Blochperiodic boundary conditions or fields_complex=True
), then one half of the flux or energy integrals above corresponds to the time average of the flux or energy for a simulation with real fields.
Often, you want the integration box to be the entire computational cell. A useful function to return this box, which you can then use for the box
arguments above, is Simulation.total_volume()
.
One versatile feature is that you can supply an arbitrary function of position and various field components and ask Meep to integrate it over a given volume, find its maximum, or output it (via output_field_function
, described later). This is done via the functions:
integrate_field_function(cs, func, where=None, center=None, size=None)
—
Returns the integral of the complexvalued function func
over the Volume
specified by where
(defaults to entire computational cell) for the meep::fields
contained in the Simulation
instance that calls this method. func
is a function of position (a Vector3
, its first argument) and zero or more field components specified by cs
: a list of component
constants. func
can be real or complexvalued. The volume can optionally be specified via the center
and size
arguments.
If any dimension of where
is zero, that dimension is not integrated over. In this way you can specify 1d, 2d, or 3d integrals.
max_abs_field_function(cs, func, where=None, center=None, size=None)
—
As integrate_field_function
, but returns the maximum absolute value of func
in the volume where
instead of its integral.
The integration is performed by summing over the grid points with a simple trapezoidal rule, and the maximum is similarly over the grid points. See Field Functions for examples of how to call integrate_field_function
and max_abs_field_function
. See Synchronizing the Magnetic and Electric Fields if you want to do computations combining the electric and magnetic fields. The volume can optionally be specified via the center
and size
arguments.
Occasionally, one wants to compute an integral that combines fields from two separate simulations (e.g. for nonlinear coupledmode calculations). This functionality is supported in Meep, as long as the two simulations have the same computational cell, the same resolution, the same boundary conditions and symmetries (if any), and the same PML layers (if any).
integrate2_field_function(fields2, cs1, cs2, func, where=None, center=None, size=None)
—Similar to integrate_field_function
, but takes additional parameters fields2
and cs2
. fields2
is a meep::fields*
object similar to the global fields
variable (see below) specifying the fields from another simulation. cs1
is a list of components to integrate with from the meep::fields
instance in Simulation.fields
, as for integrate_field_function
, while cs2
is a list of components to integrate from fields2
. Similar to integrate_field_function
, func
is a function that returns an number given arguments consisting of: the position vector, followed by the values of the components specified by cs1
(in order), followed by the values of the components specified by cs2
(in order). The volume can optionally be specified via the center
and size
arguments.
To get two fields in memory at once for integrate2_field_function
, the easiest way is to run one simulation within a given Python file, then save the results in another fields variable, then run a second simulation. This would look something like:
...set up and run first simulation...
fields2 = sim.fields # save the fields in a variable
sim.fields = None # prevent the fields from getting deallocated by resetmeep
sim.reset_meep()
...set up and run second simulation...
It is also possible to timestep both fields simultaneously (e.g. doing one timestep of one simulation then one timestep of another simulation, and so on, but this requires you to call much lowerlevel functions like fields_step()
.
Reloading Parameters
Once the fields/simulation have been initialized, you can change the values of various parameters by using the following functions (which are attributes of the Simulation
class):
reset_meep()
—
Reset all of Meep's parameters, deleting the fields, structures, etcetera, from memory as if you had not run any computations.
restart_fields()
—
Restart the fields at time zero, with zero fields. Does not reset the Fourier transforms of the flux planes, which continue to be accumulated.
change_k_point(k)
—
Change the k_point
(the Bloch periodicity).
change_sources(new_sources)
—
Change the list of sources in Simulation.sources
to new_sources
, and changes the sources used for the current simulation. new_sources
must be a list of Source
objects.
set_materials(geometry=None, default_material=None)
—
This can be called in a step function, and is useful for changing the geometry or default material as a function of time.
Flux Spectra
Given a bunch of FluxRegion
objects (see above), you can tell Meep to accumulate the Fourier transforms of the fields in those regions in order to compute flux spectra. See also the Introduction and Tutorial/Basics. These are attributes of the Simulation
class. The most important function is:
add_flux(fcen, df, nfreq, FluxRegions...)
—
Add a bunch of FluxRegion
s to the current simulation (initializing the fields if they have not yet been initialized), telling Meep to accumulate the appropriate field Fourier transforms for nfreq
equally spaced frequencies covering the frequency range fcendf/2
to fcen+df/2
. Return a flux object, which you can pass to the functions below to get the flux spectrum, etcetera.
As described in the tutorial, you normally use add_flux
via statements like:
transmission = sim.add_flux(...)
—
to store the flux object in a variable. add_flux
initializes the fields if necessary, just like calling run
, so you should only call it after initializing your Simulation
object which includes specifying geometry
, sources
, boundary_layers
, etcetera. You can create as many flux objects as you want, e.g. to look at powers flowing in different regions or in different frequency ranges. Note, however, that Meep has to store (and update at every time step) a number of Fourier components equal to the number of grid points intersecting the flux region multiplied by the number of electric and magnetic field components required to get the Poynting vector multiplied by nfreq
, so this can get quite expensive (in both memory and time) if you want a lot of frequency points over large regions of space.
Once you have called add_flux
, the Fourier transforms of the fields are accumulated automatically during timestepping by the run functions. At any time, you can ask for Meep to print out the current flux spectrum via:
display_fluxes(fluxes...)
—
Given a number of flux objects, this displays a commaseparated table of frequencies and flux spectra, prefixed by "flux1:" or similar (where the number is incremented after each run). All of the fluxes should be for the same fcen
/df
/nfreq
. The first column are the frequencies, and subsequent columns are the flux spectra.
You might have to do something lowerlevel if you have multiple flux regions corresponding to different frequency ranges, or have other special needs. display_fluxes(f1, f2, f3)
is actually equivalent to display_csv("flux", get_flux_freqs(f1), get_fluxes(f1), get_fluxes(f2), get_fluxes(f3))
, where display_csv
takes a bunch of lists of numbers and prints them as a commaseparated table, and we are calling two lowerlevel functions:
get_flux_freqs(flux)
—
Given a flux object, returns a list of the frequencies that it is computing the spectrum for.
get_fluxes(flux)
—
Given a flux object, returns a list of the current flux spectrum that it has accumulated.
As described in Tutorial/Basics, for a reflection spectrum you often want to save the Fouriertransformed fields from a "normalization" run and then load them into another run to be subtracted. This can be done via:
save_flux(filename, flux)
—
Save the Fouriertransformed fields corresponding to the given flux object in an HDF5 file of the given name without the ".h5" suffix (the current filenameprefix is prepended automatically).
load_flux(filename, flux)
—
Load the Fouriertransformed fields into the given flux object (replacing any values currently there) from an HDF5 file of the given name without the ".h5" suffix (the current filenameprefix is prepended automatically). You must load from a file that was saved by save_flux
in a simulation of the same dimensions (for both the computational cell and the flux regions) with the same number of processors.
load_minus_flux(filename, flux)
—
As load_flux
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
Sometimes it is more convenient to keep the Fouriertransformed fields in memory rather than writing them to a file and immediately loading them back again. To that end, the Simulation
class exposes the following three methods:
get_flux_data(flux)
—
Get the Fouriertransformed fields corresponding to the given flux object as a FluxData
, which is just a named tuple of NumPy arrays. Note that this object is only useful for passing to load_flux_data
below and should be considered opaque.
load_flux_data(flux, fdata)
—
Load the Fouriertransformed fields into the given flux object (replacing any values currently there) from the FluxData
object fdata
. You must load from an object that was created by get_flux_data
in a simulation of the same dimensions (for both the computational cell and the flux regions) with the same number of processors.
load_minus_flux_data(flux, fdata)
—
As load_flux_data
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
scale_flux_fields(s, flux)
—
Scale the Fouriertransformed fields in flux
by the complex number s
. e.g. load_minus_flux
is equivalent to load_flux
followed by scale_flux_fields
with s=1
.
get_eigenmode_coefficients(flux, bands, eig_parity, eig_vol, eig_resolution, eig_tolerance, kpoint_func)
—
Given a flux object and list of band indices, return a tuple of (1) the eigenmode coefficients as a 3d NumPy array of size (len(bands)
, flux.Nfreq
, 2
(modes in + and  directions)), (2) the group velocity as a NumPy array, and (3) a list of kpoints as mp.Vector3
s. The flux object must be created using add_mode_monitor
(an alias for add_flux
). eig_vol
is the volume passed to MPB for the eigenmode calculation (based on interpolating the discretized materials from the Yee grid); in most cases this will simply be the volume over which the frequencydomain fields are tabulated, which is the default (i.e. flux.where
). eig_parity
should be one of [mp.NO_PARITY
(default), mp.EVEN_Z
, mp.ODD_Z
, mp.EVEN_Y
, mp.ODD_Y
]. It is the parity (= polarization in 2d) of the mode to calculate, assuming the structure has and/or mirror symmetry in the source region. If the structure has both and mirror symmetry, you can combine more than one of these, e.g. EVEN_Z+ODD_Y
. Default is NO_PARITY
, in which case MPB computes all of the bands which will still be even or odd if the structure has mirror symmetry, of course. This is especially useful in 2d simulations to restrict yourself to a desired polarization. eig_resolution
is the spatial resolution to use in MPB for the eigenmode calculations. This defaults to the same resolution as Meep, but you can use a higher resolution in which case the structure is linearly interpolated from the Meep pixels. eig_tolerance
is the tolerance to use in the MPB eigensolver. MPB terminates when the eigenvalues stop changing to less than this fractional tolerance. Defaults to 1e7
. For examples, see Tutorial/Mode Decomposition.
Technically, MPB computes ωₙ(k)
and then inverts it with Newton's method to find the wavevector k
normal to eig_vol
and mode for a given frequency; in rare cases (primarily waveguides with nonmonotonic dispersion relations, which doesn't usually happen in simple dielectric waveguides), MPB may need you to supply an initial "guess" for k
in order for this Newton iteration to converge. You can supply this initial guess with kpoint_func
, which is a function kpoint_func(f, n)
that supplies a rough initial guess for the k
of band number n
at frequency f = ω/2π
. (By default, the k components in the plane of the eig_vol
region are zero. However, if this region spans the entire computational cell in some directions, and the cell has Blochperiodic boundary conditions via the k_point
parameter, then the mode's k components in those directions will match k_point
so that the mode satisfies the Meep boundary conditions, regardless of kpoint_func
.)
add_mode_monitor(fcen, df, nfreq, ModeRegions...)
—
Similar to add_flux
, but for use with get_eigenmode_coefficients
.
add_mode_monitor
works properly with arbitrary symmetries, but may be suboptimal because the Fouriertransformed region does not exploit the symmetry. As an optimization, if you have a mirror plane that bisects the mode monitor, you can instead use add_flux
to gain a factor of two, but in that case you must also pass the corresponding eig_parity
to get_eigenmode_coefficients
in order to only compute eigenmodes with the corresponding mirror symmetry.
get_eigenmode_freqs(flux)
—
Given a flux object, returns a list of the frequencies that it is computing the spectrum for.
Force Spectra
Very similar to flux spectra, you can also compute force spectra: forces on an object as a function of frequency, computed by Fourier transforming the fields and integrating the vacuum Maxwell stress tensor:
over a surface via . We recommend that you normally only evaluate the stress tensor over a surface lying in vacuum, as the interpretation and definition of the stress tensor in arbitrary media is often problematic (the subject of extensive and controversial literature). It is fine if the surface encloses an object made of arbitrary materials, as long as the surface itself is in vacuum.
See also Tutorial/Optical Forces.
Most commonly, you will want to normalize the force spectrum in some way, just as for flux spectra. Most simply, you could divide two different force spectra to compute the ratio of forces on two objects. Often, you will divide a force spectrum by a flux spectrum, to divide the force by the incident power on an object, in order to compute the useful dimensionless ratio / where in Meep units. For example, it is a simple exercise to show that the force on a perfectly reflecting mirror with normalincident power satisfies /, and for a perfectly absorbing (black) surface /.
The usage is similar to the flux spectra: you define a set of ForceRegion
objects telling Meep where it should compute the Fouriertransformed fields and stress tensors, and call add_force
to add these regions to the current simulation over a specified frequency bandwidth, and then use display_forces
to display the force spectra at the end. There are also save_force
, load_force
, and load_minus_force
functions that you can use to subtract the fields from two simulation, e.g. in order to compute just the force from scattered fields, similar to the flux spectra. These types and functions are defined as follows:
ForceRegion
A region (volume, plane, line, or point) in which to compute the integral of the stress tensor of the Fouriertransformed fields. Its properties are:
center [ Vector3 ]
—
The center of the force region (no default).
size [ Vector3 ]
—
The size of the force region along each of the coordinate axes. Default is (0,0,0)
(a single point).
direction [ direction constant ]
—
The direction of the force that you wish to compute (e.g. X
, Y
, etcetera). Unlike FluxRegion
, you must specify this explicitly, because there is not generally any relationship between the direction of the force and the orientation of the force region.
weight [ complex ]
—
A weight factor to multiply the force by when it is computed. Default is 1.0.
In most circumstances, you should define a set of ForceRegion
s whose union is a closed surface lying in vacuum and enclosing the object that is experiencing the force.
Simulation.add_force(fcen, df, nfreq, ForceRegions...)
—
Add a bunch of ForceRegion
s to the current simulation (initializing the fields if they have not yet been initialized), telling Meep to accumulate the appropriate field Fourier transforms for nfreq
equally spaced frequencies covering the frequency range fcendf/2
to fcen+df/2
. Return a force object, which you can pass to the functions below to get the force spectrum, etcetera.
As for flux regions, you normally use add_force
via statements like:
Fx = sim.add_force(...)
to store the flux object in a variable. add_force
initializes the fields if necessary, just like calling run
, so you should only call it after initializing your Simulation
object which includes specifiying geometry
, sources
, boundary_layers
, etcetera. You can create as many force objects as you want, e.g. to look at forces on different objects, in different directions, or in different frequency ranges. Note, however, that Meep has to store (and update at every time step) a number of Fourier components equal to the number of grid points intersecting the force region, multiplied by the number of electric and magnetic field components required to get the stress vector, multiplied by nfreq
, so this can get quite expensive (in both memory and time) if you want a lot of frequency points over large regions of space.
Once you have called add_force
, the Fourier transforms of the fields are accumulated automatically during timestepping by the run
functions. At any time, you can ask for Meep to print out the current force spectrum via:
display_forces(forces...)
—
Given a number of force objects, this displays a commaseparated table of frequencies and force spectra, prefixed by "force1:" or similar (where the number is incremented after each run). All of the forces should be for the same fcen
/df
/nfreq
. The first column are the frequencies, and subsequent columns are the force spectra.
You might have to do something lowerlevel if you have multiple force regions corresponding to different frequency ranges, or have other special needs. display_forces(f1, f2, f3)
is actually equivalent to display_csv("force", get_force_freqs(f1), get_forces(f1), get_forces(f2), get_forces(f3))
, where display_csv
takes a bunch of lists of numbers and prints them as a commaseparated table, and we are calling two lowerlevel functions:
get_force_freqs(force)
—
Given a force object, returns a list of the frequencies that it is computing the spectrum for.
get_forces(flux)
—
Given a force object, returns a list of the current force spectrum that it has accumulated.
As described in Tutorial/Basics, to compute the force from scattered fields often want to save the Fouriertransformed fields from a "normalization" run and then load them into another run to be subtracted. This can be done via:
save_force(filename, force)
—
Save the Fouriertransformed fields corresponding to the given force object in an HDF5 file of the given name without the ".h5" suffix (the current filenameprefix is prepended automatically).
load_force(filename, force)
—
Load the Fouriertransformed fields into the given force object (replacing any values currently there) from an HDF5 file of the given name without the ".h5" suffix (the current filenameprefix is prepended automatically). You must load from a file that was saved by save_force
in a simulation of the same dimensions for both the computational cell and the force regions with the same number of processors.
load_minus_force(filename, force)
—
As load_force
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
To keep the fields in memory and avoid writing to and reading from a file, use the following three methods:
get_force_data(force)
—
Get the Fouriertransformed fields corresponding to the given force object as a ForceData
, which is just a named tuple of NumPy arrays. Note that this object is only useful for passing to load_force_data
below and should be considered opaque.
load_force_data(force, fdata)
—
Load the Fouriertransformed fields into the given force object (replacing any values currently there) from the ForceData
object fdata
. You must load from an object that was created by get_force_data
in a simulation of the same dimensions (for both the computational cell and the flux regions) with the same number of processors.
load_minus_force_data(filename, force)
—
As load_force_data
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
LDOS spectra
Meep can also calculate the LDOS (local density of states) spectrum, as described in Tutorial/Local Density of States. To do this, you simply pass the following step function to your run
command:
dft_ldos(fcen, df, nfreq)
—
Compute the power spectrum of the sources (usually a single point dipole source), normalized to correspond to the LDOS, in a frequency bandwith df
centered at fcen
, at nfreq
frequency points.
get_ldos_freqs(ldos)
—
Given an ldos object, returns a list of the frequencies that it is computing the spectrum for.
The resulting spectrum is outputted as commadelimited text, prefixed by ldos:,
, and is also stored in the dft_ldos_data
global variable after the run
is complete.
Analytically, the perpolarization LDOS is exactly proportional to the power radiated by an oriented pointdipole current, , at a given position in space. For a more mathematical treatment of the theory behind the LDOS, we refer you to the relevant discussion in Section 4.4 ("Currents and Fields: The Local Density of States") in Chapter 4 ("Electromagnetic Wave Source Conditions") of the book Advances in FDTD Computational Electrodynamics: Photonics and Nanotechnology, but for now we simply give the definition:
where the normalization is necessary for obtaining the power exerted by a unitamplitude dipole (assuming linear materials), and hats denote Fourier transforms. It is this quantity that is computed by the dft_ldos
command for a single dipole source. For a volumetric source, the numerator and denominator are both integrated over the current volume, but "LDOS" computation is less meaningful in this case.
NeartoFarField Spectra
Meep can compute a neartofarfield transformation in the frequency domain as described in Tutorial/NeartoFar Field Spectra: given the fields on a "near" bounding surface inside the computational cell, it can compute the fields arbitrarily far away using an analytical transformation, assuming that the "near" surface and the "far" region lie in a single homogeneous nonperiodic 2d or 3d region. That is, in a simulation surrounded by PML that absorbs outgoing waves, the neartofarfield feature can compute the fields outside the computational cell as if the outgoing waves had not been absorbed (i.e. in the fictitious infinite open volume). Moreover, this operation is performed on the Fouriertransformed fields: like the flux and force spectra above, you specify a set of desired frequencies, Meep accumulates the Fourier transforms, and then Meep computes the fields at each frequency for the desired farfield points.
This is based on the principle of equivalence: given the Fouriertransformed tangential fields on the "near" surface, Meep computes equivalent currents and convolves them with the analytical Green's functions in order to compute the fields at any desired point in the "far" region. For details, see Section 4.2.1 ("The Principle of Equivalence") in Chapter 4 ("Electromagnetic Wave Source Conditions") of the book Advances in FDTD Computational Electrodynamics: Photonics and Nanotechnology.
There are three steps to using the neartofarfield feature: first, define the "near" surface(s) as a set of surfaces capturing all outgoing radiation in the desired direction(s); second, run the simulation, typically with a pulsed source, to allow Meep to accumulate the Fourier transforms on the near surface(s); third, tell Meep to compute the far fields at any desired points (optionally saving the far fields from a grid of points to an HDF5 file). To define the near surfaces, use:
add_near2far(fcen, df, nfreq, Near2FarRegions...)
—
Add a bunch of Near2FarRegion
s to the current simulation (initializing the fields if they have not yet been initialized), telling Meep to accumulate the appropriate field Fourier transforms for nfreq
equallyspaced frequencies covering the frequency range fcendf/2
to fcen+df/2
. Return a near2far
object, which you can pass to the functions below to get the far fields.
Each Near2FarRegion
is identical to FluxRegion
except for the name: in 3d, these give a set of planes (important: all these "near surfaces" must lie in a single homogeneous material with isotropic ε and μ — and they should not lie in the PML regions) surrounding the source(s) of outgoing radiation that you want to capture and convert to a far field. Ideally, these should form a closed surface, but in practice it is sufficient for the Near2FarRegion
s to capture all of the radiation in the direction of the farfield points. Important: as for flux computations, each Near2FarRegion
should be assigned a weight
of ±1 indicating the direction of the outward normal relative to the +coordinate direction. So, for example, if you have six regions defining the six faces of a cube, i.e. the faces in the +x, x, +y, y, +z, and z directions, then they should have weights +1, 1, +1, 1, +1, and 1 respectively. Note that, neglecting discretization errors, all nearfield surfaces that enclose the same outgoing fields are equivalent and will yield the same far fields with a discretizationinduced difference that vanishes with increasing resolution etc.
After the simulation run is complete, you can compute the far fields. This is usually for a pulsed source so that the fields have decayed away and the Fourier transforms have finished accumulating.
get_farfield(near2far, x)
—
Given a Vector3
point x
which can lie anywhere outside the nearfield surface, including outside the computational cell and a near2far
object, returns the computed (Fouriertransformed) "far" fields at x
as list of length 6nfreq
, consisting of fields (Ex1,Ey1,Ez1,Hx1,Hy1,Hz1,Ex2,Ey2,Ez2,Hx2,Hy2,Hz2,...) for the frequencies 1,2,…,nfreq
.
get_near2far_freqs(n2f)
—
Given a near2far object, returns a list of the frequencies that it is computing the spectrum for.
output_farfields(near2far, fname, resolution, where=None, center=None, size=None)
—
Given an HDF5 file name fname
(does not include the .h5
suffix), a Volume
given by where
(may be 0d, 1d, 2d, or 3d), and a resolution
(in grid points / distance unit), outputs the far fields in where
(which may lie outside the computational cell) in a grid with the given resolution (which may differ from the FDTD grid resolution) to the HDF5 file as a set of twelve array datasets ex.r
, ex.i
, ..., hz.r
, hz.i
, giving the real and imaginary parts of the Fouriertransformed and fields on this grid. Each dataset is an nx×ny×nz×nfreq 4d array of space×frequency although dimensions that =1 are omitted. The volume can optionally be specified via center
and size
.
Note that far fields have the same units and scaling as the Fourier transforms of the fields, and hence cannot be directly compared to timedomain fields. In practice, it is easiest to use the far fields in computations where overall scaling (units) cancel out or are irrelevant, e.g. to compute the fraction of the far fields in one region vs. another region.
For a scatteredfield computation, you often want to separate the scattered and incident fields. Just as is described in Tutorial/Basics for flux computations, you can do this by saving the Fouriertransformed incident from a "normalization" run and then load them into another run to be subtracted. This can be done via:
save_near2far(filename, near2far)
—
Save the Fouriertransformed fields corresponding to the given near2far
object in an HDF5 file of the given name (without the ".h5" suffix). The current filenameprefix is prepended automatically.
load_near2far(filename, near2far)
—
Load the Fouriertransformed fields into the given near2far
object (replacing any values currently there) from an HDF5 file of the given name without the ".h5" suffix (the current filenameprefix is prepended automatically). You must load from a file that was saved by save_near2far
in a simulation of the same dimensions for both the computational cell and the near2far regions with the same number of processors.
load_minus_near2far(filename, near2far)
—
As load_near2far
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
To keep the fields in memory and avoid writing to and reading from a file, use the following three methods:
get_near2far_data(n2f)
—
Get the Fouriertransformed fields corresponding to the given near2far object as a NearToFarData
, which is just a named tuple of NumPy arrays. Note that this object is only useful for passing to load_near2far_data
below and should be considered opaque.
load_near2far_data(n2f, n2fdata)
—
Load the Fouriertransformed fields into the given near2far object (replacing any values currently there) from the NearToFarData
object n2fdata
. You must load from an object that was created by get_near2far_data
in a simulation of the same dimensions (for both the computational cell and the flux regions) with the same number of processors.
load_minus_near2far_data(n2f, n2fdata)
—
As load_near2far_data
, but negates the Fouriertransformed fields after they are loaded. This means that they will be subtracted from any future field Fourier transforms that are accumulated.
scale_near2far_fields(s, near2far)
—
Scale the Fouriertransformed fields in near2far
by the complex number s
. e.g. load_minus_near2far
is equivalent to load_near2far
followed by scale_near2far_fields
with s=1
.
Load and Dump Structure
These functions dump the raw ε data to disk and load it back for doing multiple simulations with the same materials but different sources etc. The only prerequisite is that the dump/load simulations have the same chunks (i.e. the same grid, number of processors, and PML). Currently only stores ε and μ, and not nonlinear coefficients or polarizability.
Simulation.dump_structure(fname)
—
Dumps the structure to the file fname
.
Simulation.load_structure(fname)
—
Loads a structure from the file fname
. A file name to load can also be passed to the Simulation
constructor via the load_structure
keyword argument.
FrequencyDomain Solver
Meep contains a frequencydomain solver that computes the fields produced in a geometry in response to a continuouswave (CW) source. This is based on an iterative linear solver instead of timestepping. For details, see Section 5.3 ("Frequencydomain solver") of Computer Physics Communications, Vol. 181, pp. 687702, 2010. Benchmarking results have shown that in many instances, such as cavities (e.g., ring resonators) with longlived resonant modes, this solver converges much faster than simply running an equivalent timedomain simulation with a CW source, timestepping until all transient effects from the source turnon have disappeared, especially if the fields are desired to a very high accuracy. To use it, simply define a ContinuousSrc
with the desired frequency and initialize the fields and geometry via init_sim()
:
sim = mp.Simulation(...)
sim.init_sim()
sim.solve_cw(tol, maxiters, L)
The first two parameters to the frequencydomain solver are the tolerance tol
for the iterative solver (10^{−8}, by default) and a maximum number of iterations maxiters
(10^{4}, by default). Finally, there is a parameter that determines a tradeoff between memory and work per step and convergence rate of the iterative algorithm, biconjugate gradient stabilized (BiCGSTABL), that is used; larger values of will often lead to faster convergence at the expense of more memory and more work per iteration. Default is , and normally a value ≥ 2 should be used.
The frequencydomain solver supports arbitrary geometries, PML, boundary conditions, symmetries, parallelism, conductors, and arbitrary nondispersive materials. LorentzDrude dispersive materials are not currently supported in the frequencydomain solver, but since you are solving at a known fixed frequency rather than timestepping, you should be able to pick conductivities etcetera in order to obtain any desired complex ε and μ at that frequency.
The frequencydomain solver requires you to use complexvalued fields, via force_complex_fields=True
.
After solve_cw
completes, it should be as if you had just run the simulation for an infinite time with the source at that frequency. You can call the various fieldoutput functions and so on as usual at this point.
GDSII Support
mp.get_GDSII_prisms(material, gdsii_filename, layer)
—
Returns a list of GeometricObject
s with material
(mp.Medium
) on layer layer
of a GDSII file gdsii_filename
.
Run and Step Functions
The actual work in Meep is performed by run functions, which timestep the simulation for a given amount of time or until a given condition is satisfied. These are attributes of the Simulation
class.
The run functions, in turn, can be modified by use of step functions: these are called at every time step and can perform any arbitrary computation on the fields, do outputs and I/O, or even modify the simulation. The step functions can be transformed by many modifier functions, like at_beginning, during_sources, etcetera which cause them to only be called at certain times, etcetera, instead of at every time step.
A common point of confusion is described in The Run Function Is Not A Loop. Read this article if you want to make Meep do some customized action on each time step, as many users make the same mistake. What you really want to in that case is to write a step function, as described below.
Run Functions
run(step_functions..., until=condition/time)
—
Run the simulation until a certain time or condition, calling the given step functions (if any) at each timestep. The keyword argument until
is either a number, in which case it is an additional time (in Meep units) to run for, or it is a function (of no arguments) which returns True
when the simulation should stop.
run(step_functions..., until_after_sources=condition/time)
—
Run the simulation until all sources have turned off, calling the given step functions (if any) at each timestep. The keyword argument until_after_sources
is either a number, in which case it is an additional time (in Meep units) to run for after the sources are off, or it is a function (of no arguments). In the latter case, the simulation runs until the sources are off and condition
returns True
.
In particular, a useful value for until_after_sources
or until
is often stop_when_field_decayed
, which is demonstrated in Tutorial/Basics:
stop_when_fields_decayed(dT, c, pt, decay_by)
—
Return a condition
function, suitable for passing to until
/until_after_sources
, that examines the component c
(e.g. Ex
, etc.) at the point pt
(a Vector3
) and keeps running until its absolute value squared has decayed by at least decay_by
from its maximum previous value. In particular, it keeps incrementing the run time by dT
(in Meep units) and checks the maximum value over that time period — in this way, it won't be fooled just because the field happens to go through 0 at some instant.
Note that, if you make decay_by
very small, you may need to increase the cutoff
property of your source(s), to decrease the amplitude of the small highfrequency components that are excited when the source turns off. High frequencies near the Nyquist frequency of the grid have slow group velocities and are absorbed poorly by PML.
Finally, another run function, useful for computing ω(k) band diagrams, is:
run_k_points(T, k_points)
—
Given a list of Vector3
, k_points
of k vectors, runs a simulation for each k point (i.e. specifying Blochperiodic boundary conditions) and extracts the eigenfrequencies, and returns a list of the complex frequencies. In particular, you should have specified one or more Gaussian sources. It will run the simulation until the sources are turned off plus an additional time units. It will run Harminv at the same point/component as the first Gaussian source and look for modes in the union of the frequency ranges for all sources. Returns a list of lists of frequencies (one list of frequencies for each k). Also prints out a commadelimited list of frequencies, prefixed by freqs:
, and their imaginary parts, prefixed by freqsim:
. See Tutorial/Resonant Modes and Transmission in a Waveguide Cavity.
Predefined Step Functions
Several useful step functions are predefined by Meep. These are available directly via the meep
package but require a Simulation
instance as an argument.
Output Functions
The most common step function is an output function, which outputs some field component to an HDF5 file. Normally, you will want to modify this by one of the at_*
functions, below, as outputting a field at every time step can get quite time and storageconsuming.
Note that although the various field components are stored at different places in the Yee lattice, when they are outputted they are all linearly interpolated to the same grid: to the points at the centers of the Yee cells, i.e. in 3d.
output_epsilon()
—
Output the dielectric function (relative permittivity) ε. Note that this only outputs the frequencyindependent part of ε (the limit).
output_mu()
—
Output the relative permeability function μ. Note that this only outputs the frequencyindependent part of μ (the limit).
output_dft(dft_fields, fname, where=None, center=None, size=None)
—
Output the Fouriertransformed fields in dft_fields
(created by add_dft_fields
) to an HDF5 file with name fname
(does not include the .h5
suffix). The Volume
where
defaults to the entire computational cell. The volume can also be specified via the center
and size
arguments.
output_hpwr()
—
Output the magneticfield energy density
output_dpwr()
—
Output the electricfield energy density
output_tot_pwr()
—
Output the total electric and magnetic energy density. Note that you might want to wrap this step function in synchronized_magnetic
to compute it more accurately. See Synchronizing the Magnetic and Electric Fields.
output_Xfield_x(), output_Xfield_y(), output_Xfield_z(), output_Xfield_r(), output_Xfield_p()
—
Output the , , , , or component respectively, of the field X, where X is either h
, b
, e
, d
, or s
for the magnetic, electric, displacement, or Poynting field, respectively. If the field is complex, outputs two datasets, e.g. ex.r
and ex.i
, within the same HDF5 file for the real and imaginary parts, respectively. Note that for outputting the Poynting field, you might want to wrap the step function in synchronized_magnetic
to compute it more accurately. See Synchronizing the Magnetic and Electric Fields.
output_Xfield()
—
Outputs all the components of the field X, where X is either h
, b
, e
, d
, or s
as above, to an HDF5 file. That is, the different components are stored as different datasets within the same file.
output_png(component, h5topng_options)
—
Output the given field component (e.g. Ex
, etc.) as a PNG image, by first outputting the HDF5 file, then converting to PNG via h5topng, then deleting the HDF5 file. The second argument is a string giving options to pass to h5topng (e.g. "Zc bluered"
). See also Tutorial/Basics.
It is often useful to use the h5topng C
or A
options to overlay the dielectric function when outputting fields. To do this, you need to know the name of the dielectricfunction .h5
file which must have been previously output by output_epsilon
. To make this easier, a builtin shell variable $EPS
is provided which refers to the lastoutput dielectricfunction .h5
file. So, for example output_png(mp.Ez,"C $EPS")
will output the field and overlay the dielectric contours.
By default, output_png
deletes the .h5
file when it is done. To preserve the .h5
file requires output_png(component, h5topng_options, rm_h5=False)
.
More generally, it is possible to output an arbitrary function of position and zero or more field components, similar to the integrate_field_function
described above. This is done by:
output_field_function(name, cs, func, real_only=False)
—
Output the field function func
to an HDF5 file in the datasets named name*.r
and name*.i
for the real and imaginary parts. Similar to integrate_field_function
, func
is a function of position (a Vector3
) and the field components corresponding to cs
: a list of component
constants. If real_only
is True, only outputs the real part of func
.
See also Field Function Examples, and Synchronizing the Magnetic and Electric Fields if you want to do computations combining the electric and magnetic fields.
Array Slices
The output functions described above write the data for the fields and materials for the entire computational volume to an HDF5 file. This is useful for postprocessing as you can later read in the HDF5 file to obtain field/material data as a NumPy array. However, in some cases it is convenient to bypass the disk altogether to obtain the data directly in the form of a NumPy array without writing/reading HDF5 files. Additionally, you may want the field/material data on just a subregion (or slice) of the entire volume. This functionality is provided by the get_array
method which takes as input a subregion of the computational volume and the field/material component. The method returns a NumPy array containing values of the field/material at the current simulation time.
get_array(vol=None, center=None, size=None component=mp.Ez, cmplx=False, arr=None)
with the following input parameters:

vol
:Volume
; the orthogonal subregion/slice of the computational volume. The return value ofget_array
has the same dimensions as theVolume
'ssize
attribute. IfNone
(default), then asize
andcenter
must be specified. 
center
,size
:Vector3
; if both are specified, the library will construct an apporpriateVolume
. This is a convenience feature and alternative to supplying aVolume
. 
component
: field/material component (i.e.,mp.Ex
,mp.Hy
,mp.Sz
,mp.Dielectric
, etc). Defaults tomp.Ez
. 
cmplx
:boolean
; ifTrue
, return complexvalued data otherwise return realvalued data (default). 
arr
: optional field to pass a preallocated NumPy array of the correct size, which will be overwritten with the field/material data instead of allocating a new array. Normally, this will be the array returned from a previous call toget_array
for a similar slice, allowing one to reusearr
(e.g., when fetching the same slice repeatedly at different times).
get_dft_array(dft_obj, component, num_freq)
—
Returns the Fouriertransformed fields as a NumPy array.

dft_obj
: adft_flux
,dft_force
,dft_fields
, ordft_near2far
object obtained from calling the appropriateadd
function (e.g.,mp.add_flux
). 
component
: A field component (e.g.,mp.Ez
) 
num_freq
: The index of the frequency: (an integer in the range0...nfreq1
, wherenfreq
is the number of frequencies stored indft_obj,
as set by thenfreq
parameter toadd_dft_fields
,add_dft_flux
, etc.)
Harminv
The following step function collects field data from a given point and runs Harminv on that data to extract the frequencies, decay rates, and other information.
Harminv(c, pt, fcen, df, [maxbands])
—
Harminv
is implemented as a class whose constructor returns a step function that collects data from the field component c
(e.g. , etc.) at the given point pt
(a Vector3
). Then, at the end of the run, it uses Harminv to look for modes in the given frequency range (center fcen
and width df
), printing the results to standard output (prefixed by harminv:
) as commadelimited text, and also storing them to the variable Harminv.modes
. The optional argument maxbands
is the maximum number of modes to search for. Defaults to 100.
Important: normally, you should only use Harminv to analyze data after the sources are off. Wrapping it in after_sources(mp.Harminv(...))
is sufficient.
In particular, Harminv takes the time series corresponding to the given field component as a function of time and decomposes it (within the specified bandwidth) as:
The results are stored in the list Harminv.modes
, which is a list of tuples holding the frequency, amplitude, and error of the modes. Given one of these tuples (e.g., first_mode = harminv_instance.modes[0]
), you can extract its various components:
freq
—
The complex frequency ω (in the usual Meep units).
freq.real
—
The real part of the frequency ω.
freq.decay
—
The imaginary part of the frequency ω.
Q
—
The dimensionless lifetime, or quality factor defined as .
amp
—
The complex amplitude .
err
—
A crude measure of the error in the frequency (both real and imaginary)...if the error is much larger than the imaginary part, for example, then you can't trust the to be accurate. Note: this error is only the uncertainty in the signal processing, and tells you nothing about the errors from finite resolution, finite cell size, and so on.
For example, [m.freq for m in harminv_instance.modes]
gives a list of the real parts of the frequencies. Be sure to save a reference to the Harminv
instance if you wish to use the results after the simulation:
sim = mp.Simulation(...)
h = mp.Harminv(...)
sim.run(mp.after_sources(h))
# do something with h.modes
StepFunction Modifiers
Rather than writing a brandnew step function every time we want to do something a bit different, the following "modifier" functions take a bunch of step functions and produce new step functions with modified behavior. See also Tutorial/Basics for examples.
Miscellaneous StepFunction Modifiers
combine_step_funcs(step_functions...)
—
Given zero or more step functions, return a new step function that on each step calls all of the passed step functions.
synchronized_magnetic(step_functions...)
—
Given zero or more step functions, return a new step function that on each step calls all of the passed step functions with the magnetic field synchronized in time with the electric field. See Synchronizing the Magnetic and Electric Fields.
Controlling When a Step Function Executes
when_true(condition, step_functions...)
—
Given zero or more step functions and a condition function condition
(a function of no arguments), evaluate the step functions whenever condition
returns True
.
when_false(condition, step_functions...)
—
Given zero or more step functions and a condition function condition
(a function of no arguments), evaluate the step functions whenever condition
returns False
.
at_every(dT, step_functions...)
—
Given zero or more step functions, evaluates them at every time interval of units (rounded up to the next time step).
after_time(T, step_functions...)
—
Given zero or more step functions, evaluates them only for times after a time units have elapsed from the start of the run.
before_time(T, step_functions...)
—
Given zero or more step functions, evaluates them only for times before a time units have elapsed from the start of the run.
at_time(T, step_functions...)
—
Given zero or more step functions, evaluates them only once, after a time units have elapsed from the start of the run.
after_sources(step_functions...)
—
Given zero or more step functions, evaluates them only for times after all of the sources have turned off.
after_sources_and_time(T, step_functions...)
—
Given zero or more step functions, evaluates them only for times after all of the sources have turned off, plus an additional time units have elapsed.
during_sources(step_functions...)
—
Given zero or more step functions, evaluates them only for times before all of the sources have turned off.
at_beginning(step_functions...)
—
Given zero or more step functions, evaluates them only once, at the beginning of the run.
at_end(step_functions...)
—
Given zero or more step functions, evaluates them only once, at the end of the run.
Modifying HDF5 Output
in_volume(v, step_functions...)
—
Given zero or more step functions, modifies any output functions among them to only output a subset (or a superset) of the computational cell, corresponding to the meep::volume* v
(created by the Volume
function).
in_point(pt, step_functions...)
—
Given zero or more step functions, modifies any output functions among them to only output a single point of data, at pt
(a Vector3
).
to_appended(filename, step_functions...)
—
Given zero or more step functions, modifies any output functions among them to append their data to datasets in a single newlycreated file named filename
(plus an .h5
suffix and the current filename prefix). They append by adding an extra dimension to their datasets, corresponding to time.
with_prefix(prefix, step_functions...)
—
Given zero or more step functions, modifies any output functions among them to prepend the string prefix
to the file names (much like filename_prefix
, above).
Writing Your Own Step Functions
A step function can take two forms. The simplest is just a function with one argument (the simulation instance), which is called at every time step unless modified by one of the modifier functions above. e.g.
def my_step(sim):
print("Hello world!")
If one then does sim.run(my_step, until=100)
, Meep will run for 100 time units and print "Hello world!" at every time step.
This suffices for most purposes. However, sometimes you need a step function that opens a file, or accumulates some computation, and you need to clean up (e.g. close the file or print the results) at the end of the run. For this case, you can write a step function of two arguments: the second argument will either be step
when it is called during timestepping, or finish
when it is called at the end of the run:
def my_step(sim, todo):
if todo == 'step':
# do something
elif todo == 'finish':
# do something else
# access simulation attributes
sim.fields ...etc.
LowLevel Functions
By default, Meep initializes C++ objects like meep::structure
and meep::fields
in the Simulation
object based on attributes like sources
and geometry
. Theses objects are then accessible via simulation_instance.structure
and simulation_instance.fields
. Given these, you can then call essentially any function in the C++ interface, because all of the C++ functions are automatically made accessible to Python by the wrappergenerator program SWIG.
Initializing the Structure and Fields
The structure
and fields
variables are automatically initialized when any of the run functions is called, or by various other functions such as add_flux
. To initialize them separately, you can call Simulation.init_sim()
manually, or Simulation._init_structure(k_point)
to just initialize the structure.
If you want to time step more than one field simultaneously, the easiest way is probably to do something like:
sim = Simulation(cell_size, resolution).init_sim()
my_fields = sim.fields
sim.fields = None
sim.reset_meep()
and then change the geometry etc. and rerun sim.init_sim()
. Then you'll have two field objects in memory.
SWIG Wrappers
If you look at a function in the C++ interface, then there are a few simple rules to infer the name of the corresponding Python function.
 First, all functions in the
meep::
namespace are available in the Meep Python module from the toplevelmeep
package.  Second, any method of a class is accessible via the standard Python class interface. For example,
meep::fields::step
, which is the function that performs a timestep, is exposed to Python asfields_instance.step()
where a fields instance is usually accessible from Simulation.fields.  C++ constructors are called using the normal Python class instantiation. E.g.,
fields = mp.fields(...)
returns a newmeep::fields
object. Calling destructors is not necessary because objects are automatically garbage collected.
Some argument type conversion is performed automatically, e.g. types like complex numbers are converted to complex<double>
, etcetera. Vector3
vectors are converted to meep::vec
, but to do this we need to know the dimensionality of the problem in C++. The problem dimensions are automatically initialized by Simulation._init_structure
, but if you want to pass vector arguments to C++ before that time you should call Simulation.require_dimensions()
, which infers the dimensions from the cell_size
, k_point
, and dimensions
variables.