tidy3d.FluxData#
- class FluxData[source]#
Bases:
MonitorData
Data associated with a
FluxMonitor
: flux data in the frequency-domain.- Parameters:
attrs (dict = {}) โ Dictionary storing arbitrary metadata for a Tidy3D object. This dictionary can be freely used by the user for storing data without affecting the operation of Tidy3D as it is not used internally. Note that, unlike regular Tidy3D fields,
attrs
are mutable. For example, the following is allowed for setting anattr
obj.attrs['foo'] = bar
. Also note that Tidy3D` will raise aTypeError
ifattrs
contain objects that can not be serialized. One can check ifattrs
are serializable by callingobj.json()
.monitor (FluxMonitor) โ Frequency-domain flux monitor associated with the data.
flux (FluxDataArray) โ Flux values in the frequency-domain.
Notes
The data is stored as a DataArray object using the xarray package.
We can access the data for each monitor by indexing into the
SimulationData
with the monitor.name
. For the flux monitor data, we can access the raw flux data as a function of frequency with.flux
. As most data are multidimensional, itโs often very helpful to print out the data and directly inspect its structure.Example
>>> from tidy3d import FluxDataArray >>> f = [2e14, 3e14] >>> coords = dict(f=f) >>> flux_data = FluxDataArray(np.random.random(2), coords=coords) >>> monitor = FluxMonitor(size=(2,0,6), freqs=[2e14, 3e14], name='flux') >>> data = FluxData(monitor=monitor, flux=flux_data)
See also
Attributes
Methods
make_adjoint_sources
(dataset_names,ย fwidth)Converts a
FieldData
to a list of adjoint current or point sources.normalize
(source_spectrum_fn)Return copy of self after normalization is applied using source spectrum function.
Inherited Common Usage
- monitor#
- flux#
- make_adjoint_sources(dataset_names, fwidth)[source]#
Converts a
FieldData
to a list of adjoint current or point sources.
- normalize(source_spectrum_fn)[source]#
Return copy of self after normalization is applied using source spectrum function.
- __hash__()#
Hash method.