mne.beamformer.make_dics¶

mne.beamformer.
make_dics
(info, forward, csd, reg=0.05, noise_csd=None, label=None, pick_ori=None, rank=None, weight_norm=None, reduce_rank=False, depth=1.0, real_filter=False, inversion='matrix', normalize_fwd=None, verbose=None)[source]¶ Compute a Dynamic Imaging of Coherent Sources (DICS) spatial filter.
This is a beamformer filter that can be used to estimate the source power at a specific frequency range 1. It does this by constructing a spatial filter for each source point. The computation of these filters is very similar to those of the LCMV beamformer (
make_lcmv()
), but instead of operating on a covariance matrix, the CSD matrix is used. When applying these filters to a CSD matrix (seeapply_dics_csd()
), the source power can be estimated for each source point. Parameters
 infoinstance of
Info
Measurement info, e.g.
epochs.info
. forwardinstance of
Forward
Forward operator.
 csdinstance of
CrossSpectralDensity
The data crossspectral density (CSD) matrices. A source estimate is performed for each frequency or frequencybin defined in the CSD object.
 reg
float
The regularization to apply to the crossspectral density before computing the inverse.
 noise_csdinstance of
CrossSpectralDensity
None
Noise crossspectral density (CSD) matrices. If provided, whitening will be done. The noise CSDs need to have been computed for the same frequencies as the data CSDs. Providing noise CSDs is mandatory if you mix sensor types, e.g. gradiometers with magnetometers or EEG with MEG.
New in version 0.20.
 label
Label
None
Restricts the solution to a given label.
 pick_ori
None
str
For forward solutions with fixed orientation, None (default) must be used and a scalar beamformer is computed. For freeorientation forward solutions, a vector beamformer is computed and:
None
Orientations are pooled after computing a vector beamformer (Default).
'normal'
Filters are computed for the orientation tangential to the cortical surface.
'maxpower'
Filters are computed for the orientation that maximizes power.
 rank
None
dict
 ‘info’  ‘full’ This controls the rank computation that can be read from the measurement info or estimated from the data. See
Notes
ofmne.compute_rank()
for details.The default is None.New in version 0.17.
 weight_norm
str
None
Can be:
None
The unitgain LCMV beamformer 2 will be computed.
'unitnoisegain'
The unitnoise gain minimum variance beamformer will be computed (BorgiottiKaplan beamformer) 2, which is not rotation invariant when
pick_ori='vector'
. This should be combined withstc.project('pca')
to follow the definition in 2.
'nai'
The Neural Activity Index 3 will be computed, which simply scales all values from
'unitnoisegain'
by a fixed value.
'unitnoisegaininvariante'
Compute a rotationinvariant normalization using the matrix square root. This differs from
'unitnoisegain'
only whenpick_ori='vector'
, creating a solution that:Is rotation invariant (
'unitnoisegain'
is not);Satisfies the first requirement from 2 that
w @ w.conj().T == I
, whereas'unitnoisegain'
has nonzero offdiagonals; butDoes not satisfy the second requirement that
w @ G.T = θI
, which arguably does not make sense for a rotationinvariant solution.
Defaults to
None
, in which case no normalization is performed. reduce_rankbool
If True, the rank of the denominator of the beamformer formula (i.e., during pseudoinversion) will be reduced by one for each spatial location. Setting
reduce_rank=True
is typically necessary if you use a single sphere model with MEG data.Changed in version 0.20: Support for reducing rank in all modes (previously only supported
pick='max_power'
with weight normalization). depth
None
float
dict
How to weight (or normalize) the forward using a depth prior. If float (default 0.8), it acts as the depth weighting exponent (
exp
) to use, which must be between 0 and 1. None is equivalent to 0, meaning no depth weighting is performed. It can also be adict
containing keyword arguments to pass tomne.forward.compute_depth_prior()
(see docstring for details and defaults). This is effectively ignored whenmethod='eLORETA'
.Changed in version 0.20: Depth bias ignored for
method='eLORETA'
. real_filterbool
If
True
, take only the real part of the crossspectraldensity matrices to compute real filters. Defaults toFalse
. inversion‘single’  ‘matrix’
This determines how the beamformer deals with source spaces in “free” orientation. Such source spaces define three orthogonal dipoles at each source point. When
inversion='single'
, each dipole is considered as an individual source and the corresponding spatial filter is computed for each dipole separately. Wheninversion='matrix'
, all three dipoles at a source vertex are considered as a group and the spatial filters are computed jointly using a matrix inversion. Whileinversion='single'
is more stable,inversion='matrix'
is more precise. See section 5 of 4. Defaults to'matrix'
.Changed in version 0.21: Default changed to
'matrix'
. normalize_fwdbool
Deprecated, use
depth
instead. verbosebool,
str
,int
, orNone
If not None, override default verbose level (see
mne.verbose()
and Logging documentation for more). If used, it should be passed as a keywordargument only.
 infoinstance of
 Returns
 filtersinstance of
Beamformer
Dictionary containing filter weights from DICS beamformer. Contains the following keys:
 ‘kind’str
The type of beamformer, in this case ‘DICS’.
 ‘weights’ndarray, shape (n_frequencies, n_weights)
For each frequency, the filter weights of the beamformer.
 ‘csd’instance of CrossSpectralDensity
The data crossspectral density matrices used to compute the beamformer.
 ‘ch_names’list of str
Channels used to compute the beamformer.
 ‘proj’ndarray, shape (n_channels, n_channels)
Projections used to compute the beamformer.
 ‘vertices’list of ndarray
Vertices for which the filter weights were computed.
 ‘n_sources’int
Number of source location for which the filter weight were computed.
 ‘subject’str
The subject ID.
 ‘pickori’None  ‘maxpower’  ‘normal’  ‘vector’
The orientation in which the beamformer filters were computed.
 ‘inversion’‘single’  ‘matrix’
Whether the spatial filters were computed for each dipole separately or jointly for all dipoles at each vertex using a matrix inversion.
 ‘weight_norm’None  ‘unitnoisegain’
The normalization of the weights.
 ‘src_type’str
Type of source space.
 ‘is_free_ori’bool
Whether the filter was computed in a fixed direction (pick_ori=’maxpower’, pick_ori=’normal’) or not.
 ‘whitener’None  ndarray, shape (n_channels, n_channels)
Whitening matrix, provided if whitening was applied to the covariance matrix and leadfield during computation of the beamformer weights.
 ‘maxpowerori’ndarray, shape (n_sources, 3)  None
When pick_ori=’maxpower’, this fields contains the estimated direction of maximum power at each source location.
 filtersinstance of
See also
Notes
The original reference is 1. See 4 for a tutorial style paper on the topic.
The DICS beamformer is very similar to the LCMV (
make_lcmv()
) beamformer and many of the parameters are shared. However,make_dics()
andmake_lcmv()
currently have different defaults for these parameters, which were settled on separately through extensive practical use case testing (but not necessarily exhaustive parameter space searching), and it remains to be seen how functionally interchangeable they could be.The default setting reproduce the DICS beamformer as described in 4:
inversion='single', weight_norm=None, depth=1.
To use the
make_lcmv()
defaults, use:inversion='matrix', weight_norm='unitnoisegaininvariant', depth=None
For more information about
real_filter
, see the supplemental information from 5.References
 1(1,2)
Joachim Groß, Jan Kujala, Matti S. Hämäläinen, Lars Timmermann, Alfons Schnitzler, and Riitta Salmelin. Dynamic imaging of coherent sources: studying neural interactions in the human brain. Proceedings of the National Academy of Sciences, 98(2):694–699, 2001. doi:10.1073/pnas.98.2.694.
 2(1,2,3,4)
Kensuke Sekihara and Srikantan S. Nagarajan. Adaptive Spatial Filters for Electromagnetic Brain Imaging. Series in Biomedical Engineering. Springer, Berlin; Heidelberg, 2008. ISBN 9783540793694 9783540793700. doi:10.1007/9783540793700.
 3
Barry D. Van Veen, Wim van Drongelen, Moshe Yuchtman, and Akifumi Suzuki. Localization of brain electrical activity via linearly constrained minimum variance spatial filtering. IEEE Transactions on Biomedical Engineering, 44(9):867–880, 1997. doi:10.1109/10.623056.
 4(1,2,3)
Marijn van Vliet, Mia Liljeström, Susanna Aro, Riitta Salmelin, and Jan Kujala. Analysis of functional connectivity and oscillatory power using DICS: from raw MEG data to grouplevel statistics in Python. bioRxiv, 2018. doi:10.1101/245530.
 5
Joerg F. Hipp, Andreas K. Engel, and Markus Siegel. Oscillatory synchronization in largescale cortical networks predicts perception. Neuron, 69(2):387–396, 2011. doi:10.1016/j.neuron.2010.12.027.