Check out our installation instructions.
See Getting help.
If PyVista plotting in Jupyter Notebooks doesn’t work well, using the IPython
magic %gui qt
should help.
%gui qt
Python uses some backends that interfere with the macOS energy saver when
using an IDE such as Spyder or PyCharm. To test it, import time
and run:
start = time.time(); time.sleep(0.0005); print(time.time() - start)
If it takes several seconds you can either:
Install the module appnope
and run in your script:
import appnope
appnope.nope()
Change the configuration defaults by running in your terminal:
$ defaults write org.python.python NSAppSleepDisabled -bool YES
Knowing “the right thing” to do with EEG and MEG data is challenging. We use the MNE Forum to discuss analysis strategies for different kinds of data. It’s worth searching the archives to see if there have been relevant discussions in the past, but don’t hesitate to ask a new question if the answer isn’t out there already.
When you encounter an error message or unexpected results, it can be hard to tell whether it happened because of a bug in MNE-Python, a mistake in user code, a corrupted data file, or irregularities in the data itself. Your first step when asking for help should be the MNE Forum, not GitHub. This bears repeating: the GitHub issue tracker is not for usage help — it is for software bugs, feature requests, and improvements to documentation. If you open an issue that contains only a usage question, we will close the issue and direct you to the forum. If you’re pretty sure the problem you’ve encountered is a software bug (not bad data or user error):
Make sure you’re using the most current version. You can check it locally at a shell prompt with:
$ mne sys_info
which will also give you version info about important MNE-Python dependencies.
If you’re already on the most current version, if possible try using the latest development version, as the bug may have been fixed already since the latest release. If you can’t try the latest development version, search the GitHub issues page to see if the problem has already been reported and/or fixed.
Try to replicate the problem with one of the MNE sample datasets. If you can’t replicate it with a built-in dataset, provide a link to a small, anonymized portion of your data that does yield the error.
If the problem persists, open a new issue and include the smallest possible code sample that replicates the error you’re seeing. Paste the code sample into the issue, with a line containing three backticks (```) above and below the lines of code. This minimal working example should be self-contained, which means that MNE-Python contributors should be able to copy and paste the provided snippet and replicate the bug on their own computers.
Pickling data and MNE-Python objects for later use can be tempting due to its simplicity and generality, but it is usually not the best option. Pickling is not designed for stable persistence, and it is likely that you will not be able to read your data in the not-too-distant future. For details, see:
MNE-Python is designed to provide its own file saving formats (often based on
the FIF standard) for its objects usually via a save
method or write_*
method, e.g. mne.io.Raw.save()
, mne.Epochs.save()
,
mne.write_evokeds()
, mne.SourceEstimate.save()
. If you have some
data that you want to save but can’t figure out how, post to the MNE Forum
or to the GitHub issues page.
If you want to write your own data to disk (e.g., subject behavioral scores), we strongly recommend using h5io, which is based on the HDF5 format and h5py, to save data in a fast, future-compatible, standard format.
The default location for the MNE-sample data is ~/mne_data
. If you
downloaded data and an example asks you whether to download it again, make sure
the data reside in the examples directory and that you run the script from its
current directory:
$ cd examples/preprocessing
Then in Python you can do:
In [1]: %run plot_find_ecg_artifacts.py
See Datasets Overview for a list of all available datasets and some advanced configuration options, e.g. to specify a custom location for storing the datasets.
Ordinarily in MNE-python the parallel
module is used to deploy multiple
cores via the n_jobs
variable. However, functions like
mne.preprocessing.maxwell_filter()
that use scipy.linalg
do not
have an n_jobs
flag but may still use multiple cores. This is because
scipy.linalg
is built with linear algebra libraries that natively
support multithreading:
Intel Math Kernel Library (MKL), which uses OpenMP
To control how many cores are used for linear-algebra-heavy functions like
mne.preprocessing.maxwell_filter()
, you can set the OMP_NUM_THREADS
or OPENBLAS_NUM_THREADS
environment variable to the desired number of cores
for MKL or OpenBLAS, respectively. This can be done before running Python, or
inside Python you can achieve the same effect by, e.g.:
>>> import os
>>> num_cpu = '4' # Set as a string
>>> os.environ['OMP_NUM_THREADS'] = num_cpu
This must be done before running linear algebra functions; subsequent changes in the same Python session will have no effect.
The mne.what()
function can be called on any .fif
file to
identify the kind of data contained in the file. This will help you determine
whether to use mne.read_cov()
, mne.read_epochs()
,
mne.read_evokeds()
, etc. There is also a corresponding command line tool
mne what:
$ mne what sample_audvis_eog-eve.fif
events
There are many functions in MNE-Python for changing the effective sampling rate of data. We’ll discuss some major ones here, with some of their implications:
mne.io.Raw.resample()
is used to resample (typically downsample) raw
data. Resampling is the two-step process of applying a low-pass FIR filter
and subselecting samples from the data.
Using this function to resample data before forming mne.Epochs
for final analysis is generally discouraged because doing so effectively
loses precision of (and jitters) the event timings, see
this gist as
a demonstration. However, resampling raw data can be useful for
(at least):
Computing projectors in low- or band-passed data
Exploring data
mne.preprocessing.ICA.fit()
decimates data without low-passing,
but is only used for fitting a statistical model to the data.
mne.Epochs.decimate()
, which does the same thing as the
decim
parameter in the mne.Epochs
constructor, sub-selects every
\(N^{th}\) sample before and after each event. This should only be
used when the raw data have been sufficiently low-passed e.g. by
mne.io.Raw.filter()
to avoid aliasing artifacts.
mne.Epochs.resample()
, mne.Evoked.resample()
, and
mne.SourceEstimate.resample()
all resample data.
This process avoids potential aliasing artifacts because the
resampling process applies a low-pass filter. However, this filtering
introduces edge artifacts. Edge artifacts also exist when using
mne.io.Raw.resample()
, but there the edge artifacts are constrained
to two times: the start and end of the recording. With these three methods,
edge artifacts are introduced to the start and end of every epoch
of data (or the start and end of the mne.Evoked
or
mne.SourceEstimate
data), which often has a more pronounced
effect on the data.
mne.SourceEstimate.bin()
can be used to decimate, with or without
“binning” (averaging across data points). This is equivalent to applying
a moving-average (boxcar) filter to the data and decimating. A boxcar in
time is a sinc in
frequency, so this acts as a simplistic, non-ideal low-pass filter;
this will reduce but not eliminate aliasing if data were not sufficiently
low-passed. In the case where the “filter” or bin-width is a single sample
(i.e., an impulse) this operation simplifies to decimation without filtering.
mne.io.Raw.resample()
has a parameter npad=='auto'
. This is the
default, but if you’ve changed it you could try changing it back to 'auto'
,
it might help.
If you have an NVIDIA GPU you could also try using GPU acceleration with CUDA, which can sometimes speed up filtering and resampling operations by an order of magnitude.
The estimated covariance can be numerically unstable and tends to induce correlations between estimated source amplitudes and the number of samples available. It is thus suggested to regularize the noise covariance matrix (see Regularization of the noise-covariance matrix), especially if only few samples are available. Unfortunately it is not easy to tell the effective number of samples, hence, to choose the appropriate regularization. In MNE-Python, regularization is done using advanced regularization methods described in [1]. For this the ‘auto’ option can be used. With this option cross-validation will be used to learn the optimal regularization:
>>> import mne
>>> epochs = mne.read_epochs(epochs_path)
>>> cov = mne.compute_covariance(epochs, tmax=0., method='auto')
This procedure evaluates the noise covariance quantitatively by how well it
whitens the data using the negative log-likelihood of unseen data. The final
result can also be visually inspected. Under the assumption that the baseline
does not contain a systematic signal (time-locked to the event of interest),
the whitened baseline signal should be follow a multivariate Gaussian
distribution, i.e., whitened baseline signals should be between -1.96 and 1.96
at a given time sample. Based on the same reasoning, the expected value for the
global field power (GFP) is 1 (calculation of the GFP
should take into account the true degrees of freedom, e.g. ddof=3
with 2
active SSP vectors):
>>> evoked = epochs.average()
>>> evoked.plot_white(cov)
This plot displays both, the whitened evoked signals for each channels and the whitened GFP. The numbers in the GFP panel represent the estimated rank of the data, which amounts to the effective degrees of freedom by which the squared sum across sensors is divided when computing the whitened GFP. The whitened GFP also helps detecting spurious late evoked components which can be the consequence of over- or under-regularization.
Note that if data have been processed using signal space separation (SSS) [2], gradiometers and magnetometers will be displayed jointly because both are reconstructed from the same SSS basis vectors with the same numerical rank. This also implies that both sensor types are not any longer linearly independent.
These methods for evaluation can be used to assess model violations. Additional introductory materials can be found here.
For expert use cases or debugging the alternative estimators can also be compared:
>>> covs = mne.compute_covariance(epochs, tmax=0., method='auto', return_estimators=True)
>>> evoked = epochs.average()
>>> evoked.plot_white(covs)
This will plot the whitened evoked for the optimal estimator and display the GFP for all estimators as separate lines in the related panel.
After using mne watershed_bem or mne.bem.make_watershed_bem()
you might find that the BEM meshes for the brain, inner skull, outer skull,
and/or scalp surfaces do not look correct in mne.viz.plot_alignment()
and mne.viz.plot_bem()
.
MNE relies on FreeSurfer’s mri_watershed to compute the BEM meshes. Freesurfer’s watershed bem strategy is to:
Compute the outer skin (scalp) surface
Shrink outer skin inward make the “outer skull”
Compute brain surface
Expand brain surface outward to make the “inner skull”
A common problem is to see:
the surface inner skull is not completely inside surface outer skull
When looking at the meshes, the inner skull surface (expanded brain surface) will have defects, and these defects will protrude into the outer skull surface (shrunken scalp surface). In these cases, you can try (in rough ascending order of difficulty):
Changing the --preflood
/ -p
parameter in
mne watershed_bem.
Changing the --atlas
and --gcaatlas
options of
mne watershed_bem.
Manually editing the meshes (see this tutorial).
Manually running mri_watershed with various FreeSurfer flags (e.g.,
-less
to fix the output).
Going farther back in your Freesurfer pipeline to fix the problem.
In particular, mri/brainmask.mgz
could be incorrectly generated by the
autorecon1 step and contain some dura and/or skull within the brain mask.
You can check by using freeview or some other MRI-viewing tool.
Consult the Freesurfer docs on fixing errors.
Try tweaking the mri_normalize parameters via xopts, e.g.:
$ mri_normalize -mprage -b 20 -n 5
Try manually setting the control points and/or using -gentle.
Examine the talairach transformation to see if it’s not quite right, and if it’s not, adjust it manually.
Search the FreeSurfer listserv for other ideas
It can be helpful to run recon_all -autorecon1 -xopts xopts.txt
in a
clean directory first to see if this fixes everything, and, if not, then
resorting to manual control point setting and/or talairach adjustment.
Once everything looks good at the end of -autorecon1
, you can then run
mne watershed_bem to see if the output is good. Once it is
(and once brainmask.mgz is correct), you can then proceed with
recon_all -autorecon2
and recon_all -autorecon3
to effectively
complete all recon_all
steps.