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%matplotlib inline

Source reconstruction using an LCMV beamformer

This tutorial gives an overview of the beamformer method and shows how to use an LCMV beamformer to reconstruct source activity. :depth: 2


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# Author: Britta Westner <britta.wstnr@gmail.com>
#
# License: BSD (3-clause)

import matplotlib.pyplot as plt
import mne
from mne.datasets import sample, fetch_fsaverage
from mne.beamformer import make_lcmv, apply_lcmv

Introduction to beamformers

A beamformer is a spatial filter that reconstructs source activity by scanning through a grid of pre-defined source points and estimating activity at each of those source points independently. A set of weights is constructed for each defined source location which defines the contribution of each sensor to this source. Beamformers are often used for their focal reconstructions and their ability to reconstruct deeper sources. They can also suppress external noise sources. The beamforming method applied in this tutorial is the linearly constrained minimum variance (LCMV) beamformer :footcite:VanVeenEtAl1997 operates on time series. Frequency-resolved data can be reconstructed with the dynamic imaging of coherent sources (DICS) beamforming method :footcite:GrossEtAl2001. As we will see in the following, the spatial filter is computed from two ingredients: the forward model solution and the covariance matrix of the data.

Data processing

We will use the sample data set for this tutorial and reconstruct source activity on the trials with left auditory stimulation.


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data_path = sample.data_path()
subjects_dir = data_path + '/subjects'
raw_fname = data_path + '/MEG/sample/sample_audvis_filt-0-40_raw.fif'

# Read the raw data
raw = mne.io.read_raw_fif(raw_fname)
raw.info['bads'] = ['MEG 2443']  # bad MEG channel

# Set up the epoching
event_id = 1  # those are the trials with left-ear auditory stimuli
tmin, tmax = -0.2, 0.5
events = mne.find_events(raw)

# pick relevant channels
raw.pick(['meg', 'eog'])  # pick channels of interest

# Create epochs
proj = False  # already applied
epochs = mne.Epochs(raw, events, event_id, tmin, tmax,
                    baseline=(None, 0), preload=True, proj=proj,
                    reject=dict(grad=4000e-13, mag=4e-12, eog=150e-6))

# Visualize averaged sensor space data
evoked = epochs.average()
evoked.plot_joint()

del raw  # save memory

Computing the covariance matrices

Spatial filters use the data covariance to estimate the filter weights. The data covariance matrix will be inverted_ during the spatial filter computation, so it is valuable to plot the covariance matrix and its eigenvalues to gauge whether matrix inversion will be possible. Also, because we want to combine different channel types (magnetometers and gradiometers), we need to account for the different amplitude scales of these channel types. To do this we will supply a noise covariance matrix to the beamformer, which will be used for whitening. The data covariance matrix should be estimated from a time window that includes the brain signal of interest, and incorporate enough samples for a stable estimate. A rule of thumb is to use more samples than there are channels in the data set; see :footcite:BrookesEtAl2008 for more detailed advice on covariance estimation for beamformers. Here, we use a time window incorporating the expected auditory response at around 100 ms post stimulus and extend the period to account for a low number of trials (72) and low sampling rate of 150 Hz.


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data_cov = mne.compute_covariance(epochs, tmin=0.01, tmax=0.25,
                                  method='empirical')
noise_cov = mne.compute_covariance(epochs, tmin=tmin, tmax=0,
                                   method='empirical')

data_cov.plot(epochs.info)

When looking at the covariance matrix plots, we can see that our data is slightly rank-deficient as the rank is not equal to the number of channels. Thus, we will have to regularize the covariance matrix before inverting it in the beamformer calculation. This can be achieved by setting the parameter reg=0.05 when calculating the spatial filter with :func:~mne.beamformer.make_lcmv. This corresponds to loading the diagonal of the covariance matrix with 5% of the sensor power.

The forward model

The forward model is the other important ingredient for the computation of a spatial filter. Here, we will load the forward model from disk; more information on how to create a forward model can be found in this tutorial: tut-forward. Note that beamformers are usually computed in a :class:`volume source space

<mne.VolSourceEstimate>`, because estimating only cortical surface activation can misrepresent the data.


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# Read forward model

fwd_fname = data_path + '/MEG/sample/sample_audvis-meg-vol-7-fwd.fif'
forward = mne.read_forward_solution(fwd_fname)

Handling depth bias

The forward model solution is inherently biased toward superficial sources. When analyzing single conditions it is best to mitigate the depth bias somehow. There are several ways to do this:

  • :func:mne.beamformer.make_lcmv has a depth parameter that normalizes the forward model prior to computing the spatial filters. See the docstring for details.
  • Unit-noise gain beamformers handle depth bias by normalizing the weights of the spatial filter. Choose this by setting weight_norm='unit-noise-gain'.
  • When computing the Neural activity index, the depth bias is handled by normalizing both the weights and the estimated noise (see :footcite:VanVeenEtAl1997). Choose this by setting weight_norm='nai'.

Note that when comparing conditions, the depth bias will cancel out and it is possible to set both parameters to None.

Compute the spatial filter

Now we can compute the spatial filter. We'll use a unit-noise gain beamformer to deal with depth bias, and will also optimize the orientation of the sources such that output power is maximized. This is achieved by setting pick_ori='max-power'. This gives us one source estimate per source (i.e., voxel), which is known as a scalar beamformer.


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filters = make_lcmv(evoked.info, forward, data_cov, reg=0.05,
                    noise_cov=noise_cov, pick_ori='max-power',
                    weight_norm='unit-noise-gain', rank=None)

# You can save the filter for later use with:
# filters.save('filters-lcmv.h5')

It is also possible to compute a vector beamformer, which gives back three estimates per voxel, corresponding to the three direction components of the source. This can be achieved by setting pick_ori='vector' and will yield a :class:`volume vector source estimate

<mne.VolVectorSourceEstimate>`. So we will compute another set of filters using the vector beamformer approach:


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filters_vec = make_lcmv(evoked.info, forward, data_cov, reg=0.05,
                        noise_cov=noise_cov, pick_ori='vector',
                        weight_norm='unit-noise-gain', rank=None)

Apply the spatial filter

The spatial filter can be applied to different data types: raw, epochs, evoked data or the data covariance matrix to gain a static image of power. The function to apply the spatial filter to :class:~mne.Evoked data is :func:~mne.beamformer.apply_lcmv which is what we will use here. The other functions are :func:~mne.beamformer.apply_lcmv_raw, :func:~mne.beamformer.apply_lcmv_epochs, and :func:~mne.beamformer.apply_lcmv_cov.


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stc = apply_lcmv(evoked, filters, max_ori_out='signed')
stc_vec = apply_lcmv(evoked, filters_vec, max_ori_out='signed')

Visualize the reconstructed source activity

We can visualize the source estimate in different ways, e.g. as an overlay onto the MRI or as a glass brain. The plots for the scalar beamformer show brain activity in the right temporal lobe around 100 ms post stimulus. This is expected given the left-ear auditory stimulation of the experiment.


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lims = [0.3, 0.45, 0.6]

kwargs = dict(src=forward['src'], subject='sample', subjects_dir=subjects_dir,
              initial_time=0.087, verbose=True)

stc.plot(mode='stat_map', clim=dict(kind='value', pos_lims=lims), **kwargs)

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stc.plot(mode='glass_brain', clim=dict(kind='value', lims=lims), **kwargs)

Now let's visualize the vector beamformer case. Here we get three source time courses out per voxel (one for each component of the dipole moment: x, y, and z). To be able to visualize this, the plotting function combines those estimates into one:


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stc_vec.plot(mode='stat_map', clim=dict(kind='value', pos_lims=lims), **kwargs)

Visualize the activity of the maximum voxel with all three components

We can also visualize all three components in the peak voxel. For this, we will first find the peak voxel and then plot the time courses of this voxel.


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peak_vox, _ = stc_vec.get_peak(tmin=0.08, tmax=0.1, vert_as_index=True)

ori_labels = ['x', 'y', 'z']
fig, ax = plt.subplots(1)
for ori, label in zip(stc_vec.data[peak_vox, :, :], ori_labels):
    ax.plot(stc_vec.times, ori, label='%s component' % label)
ax.legend(loc='lower right')
ax.set(title='Activity per orientation in the peak voxel', xlabel='Time (s)',
       ylabel='Amplitude (a. u.)')
mne.viz.utils.plt_show()

Morph the output to fsaverage

We can also use volumetric morphing to get the data to fsaverage space. This is for example necessary when comparing activity across subjects. Here, we will use the scalar beamformer example. We pass a :class:mne.SourceMorph as the src argument to mne.VolSourceEstimate.plot. To save some computational load when applying the morph, we will crop the stc:


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fetch_fsaverage(subjects_dir)  # ensure fsaverage src exists
fname_fs_src = subjects_dir + '/fsaverage/bem/fsaverage-vol-5-src.fif'

src_fs = mne.read_source_spaces(fname_fs_src)
morph = mne.compute_source_morph(
    forward['src'], subject_from='sample', src_to=src_fs,
    subjects_dir=subjects_dir,
    niter_sdr=[10, 10, 5], niter_affine=[10, 10, 5],  # just for speed
    verbose=True)
stc_fs = morph.apply(stc.crop(0.05, 0.15))

stc_fs.plot(
    src=src_fs, mode='stat_map', initial_time=0.085, subjects_dir=subjects_dir,
    clim=dict(kind='value', pos_lims=lims), verbose=True)

References

.. footbibliography::

.. LINKS