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: MRIStackedNUFFT

Stacked 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__

adj_op

Adjoint operator.

check_shape

Validate the shapes of the image or k-space data against operator shapes.

compute_density

Compute the density compensation weights and set it.

compute_smaps

Compute the sensitivity maps and set it.

data_consistency

Compute the gradient data consistency.

get_lipschitz_cst

Return the Lipschitz constant of the operator.

make_autograd

Make a new Operator with autodiff support.

make_deepinv_phy

Make a new DeepInv Physics with NUFFT operator.

make_linops

Create a Scipy Linear Operator from the NUFFT operator.

op

Forward operator.

pinv_solver

Solves the linear system Ax = y.

update_samples

Update the samples of the NUFFT operator.

with_autograd

Return a Fourier operator with autograd capabilities.

with_off_resonance_correction

Return a new operator with Off Resonnance Correction.

Attributes

autograd_available

available

backend

cpx_dtype

Return complex floating precision of the operator.

density

Density compensation of the operator.

dtype

Return dtype.

img_full_shape

Full image shape with batch and coil dimensions.

interfaces

ksp_full_shape

Full kspace shape with batch and coil dimensions.

n_batchs

Number of coils for the operator.

n_coils

Number of coils for the operator.

n_samples

Return number of samples.

ndim

Number of dimensions in image space of the operator.

norm_factor

Norm factor of the operator.

samples

Return samples as a N_slice x N_samples x 3 array.

shape

Shape of the image space of the operator.

smaps

Sensitivity maps of the operator.

uses_density

Return True if the operator uses density compensation.

uses_sense

Return True if the operator uses sensitivity maps.

backend: ClassVar[str] = 'stacked-cufinufft'[source]#
available: ClassVar[bool] = True[source]#
property shape: tuple[int, ...][source]#

Shape of the image space of the operator.

property n_coils: int[source]#

Number of coils for the operator.

property n_batchs[source]#

Number of coils for the operator.

property smaps[source]#

Sensitivity maps of the operator.

property norm_factor[source]#

Norm factor of the operator.

static _fftz(data)[source]#

Apply FFT on z-axis.

static _ifftz(data)[source]#

Apply IFFT on z-axis.

op(data, ksp=None)[source]#

Forward operator.

Note

This function uses numpy for all CPU arrays, and cupy for 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.

_op_sense_host(data, ksp=None)[source]#
_abc_impl = <_abc._abc_data object>[source]#
_adj_op_calibless(coeffs, img)[source]#
_adj_op_sense(coeffs, img)[source]#
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]#
Return type:

tuple[ndarray[tuple[int, …], dtype[_ScalarType_co]], ndarray[tuple[int, …], dtype[_ScalarType_co]]]

_op_calibless(data, ksp=None)[source]#
_op_sense(data, ksp=None)[source]#

Apply SENSE operator.

_op_sense_device(data, ksp)[source]#
_safe_squeeze(arr)[source]#

Squeeze the first two dimensions of shape of the operator.

autograd_available = False[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)

property cpx_dtype[source]#

Return complex floating precision of the operator.

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.

Return type:

ndarray[tuple[int, …], dtype[_ScalarType_co]]

property density: ndarray[tuple[int, ...], dtype[floating]] | None[source]#

Density compensation of the operator.

property dtype[source]#

Return dtype.

property img_full_shape: tuple[int, ...][source]#

Full image shape with batch and coil dimensions.

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

-, -

property n_samples[source]#

Return number of samples.

property ndim[source]#

Number of dimensions in image space of the operator.

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.

property uses_density[source]#

Return True if the operator uses density compensation.

property uses_sense[source]#

Return True if the operator uses sensitivity maps.

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:

MRIFourierCorrected

_op_calibless_host(data, ksp=None)[source]#
_op_calibless_device(data, ksp=None)[source]#
adj_op(coeffs, img=None)[source]#

Adjoint operator.

Note

This function uses numpy for all CPU arrays, and cupy for 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.

_adj_op_sense_host(coeffs, img_d=None)[source]#
_adj_op_sense_device(coeffs, img)[source]#
_adj_op_calibless_host(coeffs, img=None)[source]#
_adj_op_calibless_device(coeffs, img)[source]#
get_lipschitz_cst(max_iter=10, **kwargs)[source]#

Return the Lipschitz constant of the operator.

Parameters:
  • max_iter (int) – Number of iteration to perform to estimate the Lipschitz constant.

  • kwargs – Extra kwargs for the cufinufft operator.

Returns:

Lipschitz constant of the operator.

Return type:

float