MRIStackedNUFFTGPU#
- class mrinufft.operators.MRIStackedNUFFTGPU(samples, shape, smaps=None, n_coils=1, n_batchs=1, n_trans=1, z_index: ndarray[tuple[int, ...], dtype[_ScalarType_co]] | None | Literal['auto'] = 'auto', squeeze_dims=False, smaps_cached=False, density=False, backend='cufinufft', **kwargs)[source]#
Bases:
MRIStackedNUFFTStacked NUFFT Operator for MRI using GPU only backend.
This requires cufinufft to be installed.
- Parameters:
samples (array-like) – Sample locations in a 2D kspace
shape (tuple) – Shape of the image.
z_index (array-like) – Cartesian z index of masked plan. if “auto” the z_index is computed from the samples, if they are 3D, using the last coordinate.
smaps (array-like) – Sensitivity maps.
n_coils (int) – Number of coils.
n_batchs (int) – Number of batchs.
**kwargs (dict) – Additional arguments to pass to the backend.
Methods
__init__Adjoint operator.
Validate the shapes of the image or k-space data against operator shapes.
Compute the density compensation weights and set it.
Compute the sensitivity maps and set it.
Compute the gradient data consistency.
Return the Lipschitz constant of the operator.
Make a new Operator with autodiff support.
Make a new DeepInv Physics with NUFFT operator.
Create a Scipy Linear Operator from the NUFFT operator.
Forward operator.
Solves the linear system Ax = y.
Update the samples of the NUFFT operator.
Return a Fourier operator with autograd capabilities.
Return a new operator with Off Resonnance Correction.
Attributes
Return complex floating precision of the operator.
Density compensation of the operator.
Return dtype.
Full image shape with batch and coil dimensions.
Full kspace shape with batch and coil dimensions.
Number of coils for the operator.
Number of coils for the operator.
Return number of samples.
Number of dimensions in image space of the operator.
Norm factor of the operator.
Return samples as a N_slice x N_samples x 3 array.
Shape of the image space of the operator.
Sensitivity maps of the operator.
Return True if the operator uses density compensation.
Return True if the operator uses sensitivity maps.
- op(data, ksp=None)[source]#
Forward operator.
Note
This function uses
numpyfor all CPU arrays, andcupyfor all on-gpu array. It will convert all its array argument to the respective array library. The outputs will be converted back to the original array module and device.
- static _init_samples(samples: ndarray[tuple[int, ...], dtype[_ScalarType_co]], z_index: Literal['auto'] | ndarray[tuple[int, ...], dtype[_ScalarType_co]] | None, shape: tuple[int, ...]) tuple[ndarray[tuple[int, ...], dtype[_ScalarType_co]], ndarray[tuple[int, ...], dtype[_ScalarType_co]]][source]#
- check_shape(*, image=None, ksp=None)[source]#
Validate the shapes of the image or k-space data against operator shapes.
- Parameters:
image (NDArray, optional) – If passed, the shape of image data will be checked.
ksp (NDArray or object, optional) – If passed, the shape of the k-space data will be checked.
- Raises:
ValueError – If the shape of the provided image does not match the expected operator shape, or if the number of k-space samples does not match the expected number of samples.
- compute_density(method: Callable[[...], ndarray[tuple[int, ...], dtype[_ScalarType_co]]] | bool | None | str | dict[str, Any] = None)[source]#
Compute the density compensation weights and set it.
- Parameters:
method (str or callable or array or dict or bool) –
The method to use to compute the density compensation.
If a string, the method should be registered in the density registry.
If a callable, it should take the samples and the shape as input.
If a dict, it should have a key ‘name’, to determine which method to use. other items will be used as kwargs.
If an array, it should be of shape (Nsamples,) and will be used as is.
If True, the method pipe is chosen as default estimation method.
Notes
The “pipe” method is only available for the following backends: tensorflow, finufft, cufinufft, gpunufft, torchkbnufft-cpu and torchkbnufft-gpu.
- compute_smaps(method: ndarray[tuple[int, ...], dtype[_ScalarType_co]] | Callable[[...], ndarray[tuple[int, ...], dtype[_ScalarType_co]]] | str | dict[str, Any] | None = None)[source]#
Compute the sensitivity maps and set it.
- Parameters:
method (callable or dict or array) – The method to use to compute the sensitivity maps. If an array, it should be of shape (NCoils,XYZ) and will be used as is. If a dict, it should have a key ‘name’, to determine which method to use. other items will be used as kwargs. If a callable, it should take the samples and the shape as input. Note that this callable function should also hold the k-space data (use funtools.partial)
- data_consistency(image_data: ndarray[tuple[int, ...], dtype[_ScalarType_co]], obs_data: ndarray[tuple[int, ...], dtype[_ScalarType_co]]) ndarray[tuple[int, ...], dtype[_ScalarType_co]][source]#
Compute the gradient data consistency.
This is the naive implementation using adj_op(op(x)-y). Specific backend can (and should!) implement a more efficient version.
- property density: ndarray[tuple[int, ...], dtype[floating]] | None[source]#
Density compensation of the operator.
- interfaces: dict[str, tuple[bool, type[FourierOperatorBase]]] = {'bart': (False, <class 'mrinufft.operators.interfaces.bart.MRIBartNUFFT'>), 'cartesian': (True, <class 'mrinufft.operators.cartesian.MRICartesianOperator'>), 'cufinufft': (True, <class 'mrinufft.operators.interfaces.cufinufft.MRICufiNUFFT'>), 'ducc0': (False, <class 'mrinufft.operators.interfaces.ducc0.MRIDUCC0'>), 'finufft': (True, <class 'mrinufft.operators.interfaces.finufft.MRIfinufft'>), 'gpunufft': (True, <class 'mrinufft.operators.interfaces.gpunufft.MRIGpuNUFFT'>), 'numpy': (True, <class 'mrinufft.operators.interfaces.nudft_numpy.MRInumpy'>), 'pynfft': (False, <class 'mrinufft.operators.interfaces.nfft.MRInfft'>), 'pynufft-cpu': (False, <class 'mrinufft.operators.interfaces.pynufft_cpu.MRIPynufft'>), 'sigpy': (True, <class 'mrinufft.operators.interfaces.sigpy.MRISigpyNUFFT'>), 'stacked': (True, <class 'mrinufft.operators.stacked.MRIStackedNUFFT'>), 'stacked-cufinufft': (True, <class 'mrinufft.operators.stacked.MRIStackedNUFFTGPU'>), 'tensorflow': (False, <class 'mrinufft.operators.interfaces.tfnufft.MRITensorflowNUFFT'>), 'torchkbnufft-cpu': (False, <class 'mrinufft.operators.interfaces.torchkbnufft.TorchKbNUFFTcpu'>), 'torchkbnufft-gpu': (False, <class 'mrinufft.operators.interfaces.torchkbnufft.TorchKbNUFFTgpu'>)}[source]#
- property ksp_full_shape: tuple[int, int, int][source]#
Full kspace shape with batch and coil dimensions.
- make_autograd(*, wrt_data: bool = True, wrt_traj: bool = False, paired_batch: bool = False) MRINufftAutoGrad[source]#
Make a new Operator with autodiff support.
- Parameters:
wrt_data (bool, optional) – If the gradient with respect to the data is computed, default is true
wrt_traj (bool, optional) – If the gradient with respect to the trajectory is computed, default is false
paired_batch (int, optional) – If provided, specifies batch size for varying data/smaps pairs. Default is None, which means no batching
- Returns:
A NUFFT operator with autodiff capabilities.
- Return type:
torch.nn.module
- Raises:
ValueError – If autograd is not available.
- make_deepinv_phy(*args, **kwargs) DeepInvPhyNufft[source]#
Make a new DeepInv Physics with NUFFT operator.
- Parameters:
wrt_data (bool, optional) – If the gradient with respect to the data is computed, default is true
wrt_traj (bool, optional) – If the gradient with respect to the trajectory is computed, default is false
paired_batch (int, optional) – If provided, specifies batch size for varying data/smaps pairs. Default is None, which means no batching
viewed_as_real (bool, optional) – If True, the DeepInverse physics wrapper accepts and returns real-view tensors with a final dimension of size 2 representing the real and imaginary parts. Default is False.
- Returns:
A NUFFT operator with autodiff capabilities.
- Return type:
torch.nn.module
- Raises:
ValueError – If autograd is not available.
- make_linops(*, cupy: bool = False)[source]#
Create a Scipy Linear Operator from the NUFFT operator.
We add a _nufft private attribute with the current operator.
- Parameters:
cupy (bool, default False) – If True, create a Cupy Linear Operator
See also
-,-
- pinv_solver(kspace_data, optim='lsqr', **kwargs)[source]#
Solves the linear system Ax = y.
It uses a least-square optimization solver,
- Parameters:
kspace_data (NDArray) – The k-space data to reconstruct.
optim (str, default "lsqr") – name of the least-square optimizer to use.
**kwargs – Extra arguments to pass to the least-square optimizer.
- Returns:
Reconstructed image
- Return type:
NDArray
- property samples[source]#
Return samples as a N_slice x N_samples x 3 array.
Built from the 2D samples and the z_index normalized to [-0.5, 0.5).
- update_samples(new_samples: ndarray[tuple[int, ...], dtype[floating]], *, unsafe: bool = False)[source]#
Update the samples of the NUFFT operator.
- Parameters:
new_samples (np.ndarray or GPUArray) – The new samples location of shape
Nsamples x N_dimensions.unsafe (bool, default False) – If True, the original array is used directly without any checks. This should be used with caution as it might lead to unexpected behavior.
Notes
If unsafe is True, the new_samples should be of shape (Nsamples, N_dimensions), F-ordered (column-major) and in the range [-pi, pi]. If not, this will lead to unexpected behavior. You have been warned.
If unsafe is False, this is automatically handled.
- classmethod with_autograd(wrt_data=True, wrt_traj=False, paired_batch=False, *args, **kwargs)[source]#
Return a Fourier operator with autograd capabilities.
- with_off_resonance_correction(readout_time: NDArray, b0_map: NDArray | None = None, r2star_map: NDArray | None = None, mask: NDArray | None = None, interpolator: str | dict | tuple[NDArray, NDArray] = 'svd') MRIFourierCorrected[source]#
Return a new operator with Off Resonnance Correction.
- Return type:
- adj_op(coeffs, img=None)[source]#
Adjoint operator.
Note
This function uses
numpyfor all CPU arrays, andcupyfor all on-gpu array. It will convert all its array argument to the respective array library. The outputs will be converted back to the original array module and device.