Reconstruction

Constrained Spherical Deconvolution (CSD)

This method is mainly useful with datasets with gradient directions acquired in Cartesian coordinates that can be resampled to spherical coordinates so as to use SD methods.

The basic idea of spherical deconvolution methods lies in the fact that the underlying fiber distribution can be obtained by deconvolving the measured diffusion signal with a fiber response function, provided that we are able to accurately estimate the latter.

In this way, the reconstruction of the fiber orientation distribution function (fODF) in CSD involves two steps:

• Estimation of the fiber response function.

• Use the response function to reconstruct the fODF.

We will be using the stanford_hardi dataset for the CSD command line interface demonstration purposes.

We will start by creating the directories to which to save the peaks volume (e.g.: recons_csd_output) and mask file (e.g.: stanford_hardi_mask):

mkdir recons_csd_output stanford_hardi_mask

The workflow for the CSD reconstruction method requires the paths to the diffusion input file, b-values file, b-vectors file and mask file. The optional arguments can also be provided. In this case, we will specify the FA threshold for calculating the response function (fa_thr), spherical harmonics order used in the CSA fit (sh_order), whether to use parallelization in peak-finding during the calibration procedure or not (parallel), and the output directory (out_dir).

To get the mask file, we will use the median Otsu thresholding method by calling the dipy_median_otsu command:

dipy_median_otsu data/stanford_hardi/HARDI150.nii.gz --vol_idx 3 4 5 6 --out_dir "stanford_hardi_mask"

Then, to perform the CSD reconstruction we will run the dipy_fit_csd command as:

dipy_fit_csd data/stanford_hardi/HARDI150.nii.gz data/stanford_hardi/HARDI150.bval data/stanford_hardi/HARDI150.bvec stanford_hardi_mask/brain_mask.nii.gz --fa_thr 0.7 --sh_order 8 --parallel --out_dir "recons_csd_output"

This command will save the CSD metrics to the specified output directory.

Mean Apparent Propagator (MAP)-MRI

The MAP-MRI basis allows for the computation of directional indices, such as the Return To the Axis Probability (RTAP), the Return To the Plane Probability (RTPP), and the parallel and perpendicular Non-Gaussianity.

The estimation of analytical Orientation Distribution Function (ODF) and a variety of scalar indices from noisy DWIs requires that the fitting of the MAPMRI basis is regularized.

We will use the cfin_multib dataset in DIPY to showcase this reconstruction method. You can also use your own data!

We will create the output directory in which to save the MAP-MRI metrics (e.g.: recons_mapmri_output):

mkdir recons_mapmri_output

The Mean Apparent Propagator reconstruction method requires the paths to the diffusion input file, b-values file, b-vectors file, small delta value, big delta value. The optional parameters can also be provided. In this case, we will be specifying the threshold used to find b0 volumes (b0_threshold) and the output directory (out_dir).

To run the MAP-MRI reconstruction method on the data, execute the dipy_fit_mapmri command, e.g.:

dipy_fit_mapmri data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.nii data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.bval data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.bvec 0.0157 0.0365 --b0_threshold 80.0 --out_dir recons_mapmri_output

This command will save the MAP-MRI metrics to the specified output directory.

Diffusion Tensor Imaging (DTI)

The diffusion tensor model is a model that describes the diffusion within a voxel. First proposed by Basser and colleagues [Basser1994], it has been very influential in demonstrating the utility of diffusion MRI in characterizing the micro-structure of white matter tissue and of the biophysical properties of tissue, inferred from local diffusion properties and it is still very commonly used.

The diffusion tensor models the diffusion signal as:

Where \(\mathbf{g}\) is a unit vector in 3D space indicating the direction of measurement and b are the parameters of measurement, such as the strength and duration of the diffusion-weighting gradient. \(S(\mathbf{g}, b)\) is the measured diffusion-weighted signal and \(S_0\) is the signal conducted in a measurement with no diffusion weighting. \(\mathbf{D}\) is a positive-definite quadratic form, which contains six free parameters to be fit. These six parameters are:

This matrix is a variance/covariance matrix of the diffusivity along the three spatial dimensions. Note that we can assume that diffusivity has antipodal symmetry, so elements across the diagonal are equal. For example: \(D_{xy} = D_{yx}\). This is why there are only 6 free parameters to estimate here.

We will use the stanford_hardi dataset in DIPY to showcase this reconstruction method. As with any other workflow in DIPY, you can also use your own data!

We will first create a directory in which to save the output volumes(e.g.: recons_dti_output):

mkdir recons_dti_output

To run the Diffusion Tensor Imaging reconstruction method, we need to specify the paths to the diffusion input file, b-values file, b-vectors file and mask file, followed by optional arguments. In this case, we will be specifying the list of metrics to save (save_metrics), the output directory (out_dir), and the name of the tensors volume to be saved (out_tensor).

The DTI reconstruction is performed by calling the dipy_fit_dti command, e.g.:

dipy_fit_dti data/stanford_hardi/HARDI150.nii.gz data/stanford_hardi/HARDI150.bval data/stanford_hardi/HARDI150.bvec stanford_hardi_mask/brain_mask.nii.gz --save_metrics "md" "mode" "tensor" --out_dir "recons_dti_output" --out_tensor "dti_tensors.nii.gz"

This command will save the DTI metrics to the specified output directory. The tensors will be saved as a 4D data with last dimension representing (Dxx, Dxy, Dyy, Dxz, Dyz, Dzz).

Diffusion Kurtosis Imaging (DKI)

The diffusion kurtosis model is an expansion of the diffusion tensor model. In addition to the diffusion tensor (DT), the diffusion kurtosis model quantifies the degree to which water diffusion in biological tissues is non-Gaussian using the kurtosis tensor (KT) [Jensen2005].

Measurements of non-Gaussian diffusion from the diffusion kurtosis model are of interest because they can be used to characterize tissue microstructural heterogeneity [Jensen2010].

Moreover, DKI can be used to:

• Derive concrete biophysical parameters, such as the density of axonal fibers and diffusion tortuosity [Fierem2011].

• Resolve crossing fibers in tractography and to obtain invariant rotational measures not limited to well-aligned fiber populations [NetoHe2015].

We will use the cfin_multib dataset in DIPY to showcase this reconstruction method. You can also use your own data!

We will create the directories in which to save the DKI metrics (e.g.: recons_dki_output) and mask file (e.g.: cfin_multib_mask):

mkdir recons_dki_output cfin_multib_mask

The Diffusion Kurtosis Imaging reconstruction method requires the paths to the diffusion input file, b-values file, b-vectors file and mask file. The optional parameters can also be provided. In this case, we will be specifying the threshold used to find b0 volumes (b0_threshold) and the output directory (out_dir).

To get the mask file, we will use the median Otsu thresholding method by calling the dipy_median_otsu command:

dipy_median_otsu data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.nii --vol_idx 3 4 5 6 --out_dir "cfin_multib_mask"

To run the DKI reconstruction method on the data, execute the dipy_fit_dki command, e.g.:

dipy_fit_dki data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.nii data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.bval data/cfin_multib/__DTI_AX_ep2d_2_5_iso_33d_20141015095334_4.bvec cfin_multib_mask/brain_mask.nii.gz --b0_threshold 70.0 --out_dir recons_dki_output

This command will save the DKI metrics to the specified output directory.

Constant Solid Angle (CSA)

We are using stanford_hardi dataset. As with any other workflow in DIPY, you can also use your own data!

We will create a directory in which to save the peaks volume (e.g.: recons_csa_output):

mkdir recons_csa_output

The workflow for the CSA reconstruction method requires the paths to the diffusion input file, b-values file, b-vectors file and mask file. The optional arguments can also be provided. In this case, we will be specifying whether or not to save pam volumes as single nifti files (extract_pam_values) and the output directory (out_dir).

Then, to perform the CSA reconstruction we will run the dipy_fit_csa command as:

dipy_fit_csa data/stanford_hardi/HARDI150.nii.gz data/stanford_hardi/HARDI150.bval data/stanford_hardi/HARDI150.bvec stanford_hardi_mask/brain_mask.nii.gz --extract_pam_values --out_dir "recons_csa_output"

This command will save the CSA metrics to the specified output directory.

Intravoxel Incoherent Motion (IVIM)

The intravoxel incoherent motion (IVIM) model describes diffusion and perfusion in the signal acquired with a diffusion MRI sequence that contains multiple low b-values. The IVIM model can be understood as an adaptation of the work of Stejskal and Tanner [Stejskal65] in biological tissue, and was proposed by Le Bihan [LeBihan84]. The model assumes two compartments: a slow moving compartment, where particles diffuse in a Brownian fashion as a consequence of thermal energy, and a fast moving compartment (the vascular compartment), where blood moves as a consequence of a pressure gradient. In the first compartment, the diffusion coefficient is \(\mathbf{D}\) while in the second compartment, a pseudo diffusion term \(\mathbf{D^*}\) is introduced that describes the displacement of the blood elements in an assumed randomly laid out vascular network, at the macroscopic level. According to [LeBihan84], \(\mathbf{D^*}\) is greater than \(\mathbf{D}\).

We will be using the ivim dataset for the IVIM command line interface demonstration purposes.

We will start by creating the directories in which to save the output volumes (e.g.: recons_ivim_output) and mask file (e.g.: ivim_mask):

mkdir recons_ivim_output ivim_mask

In order to run the IVIM reconstruction method, we need to specify the locations of the diffusion input file, b-values file, b-vectors file and mask file followed by the optional arguments. In this case, we will be specifying the value to split the bvals to estimate D for the two-stage process of fitting (split_b_D) and the output directory (out_dir).

To get the mask file, we will use the median Otsu thresholding method by calling the dipy_median_otsu command:

dipy_median_otsu data/ivim/HARDI150.nii.gz --vol_idx 3 4 5 6 --out_dir "ivim_mask"

Then, to perform the IVIM reconstruction we will run the command as:

dipy_fit_ivim data/ivim/ivim.nii.gz data/ivim/ivim.nii.gz.bval data/ivim/ivim.nii.gz.bvec ivim_mask/brain_mask.nii.gz --split_b_D 250 --out_dir "recons_ivim_output"

This command will save the IVIM metrics to the directory recons_ivim_output.

In case the output directory was not specified, the output volumes will be saved to the current directory by default.