Metadata-Version: 2.4
Name: warpfield
Version: 0.0.2
Summary: GPU-accelerated 3D non-rigid registration
Author: jlab.berlin, Maximilian Hoffmann, Benjamin Judkewitz
License: MIT
Project-URL: Homepage, https://github.com/danionella/warpfield
Keywords: warpfield,python
Requires-Python: >=3.9
Description-Content-Type: text/markdown
License-File: LICENSE
Requires-Dist: numpy
Requires-Dist: scipy
Requires-Dist: cupy
Requires-Dist: tqdm
Requires-Dist: pydantic
Requires-Dist: pyyaml
Requires-Dist: h5py
Requires-Dist: hdf5plugin
Requires-Dist: nibabel
Requires-Dist: pydicom
Requires-Dist: tifffile
Dynamic: license-file

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<img src="https://github.com/user-attachments/assets/09b2109d-5db6-4f7e-8e3d-000361455a0f"/>
<sup>Example shown: region-level 3D registration across subjects (video slowed down ~5x). Cell-level registration of microscopy data is also possible.</sup>

# warpfield

A GPU-accelerated Python library for non-rigid volumetric image registration / warping.

Links: [API documentation](http://danionella.github.io/warpfield), [GitHub repository](https://github.com/danionella/warpfield)


### Features

- GPU-accelerated code for high performance ([CuPy](https://cupy.dev/), CUDA kernels & FFT plans)
- Typical speedup compared to CPU-based methods: > 1000x (seconds vs. hours)
- Forward and inverse transform of 3D volumes as well as point coordinates
- Support for .h5, .npy, .nii and .tiff file formats
- Python API and command-line interface (CLI)

### General Principle

The registration process aligns a moving 3D volume to a fixed reference volume by estimating and applying a displacement field. The process is typically performed in a multi-resolution (pyramid) fashion, starting with coarse alignment and progressively refining the displacement field at finer resolutions.

The key steps are:

1. **Preprocessing**: Enhance features in the volumes (e.g., using Difference-of-Gaussian or 'DoG' filtering) to improve registration accuracy.
2. **Block Matching**: Divide the volumes into smaller 3D blocks, project them to 2D (along each axis) for memory and compute efficiency, and calculate 2D cross-correlation maps. After smoothing these 2D maps across neighboring blocks, use their maxima to determine the block-level 3D displacement vector.
3. **Displacement Field Estimation**: Combine block-level displacement vectors into a displacement field (and optionaly apply a median filter or fit an affine transform)
4. **Warping**: Apply the displacement field to the moving volume to align it with the fixed volume.
5. **Multi-Resolution Refinement**: Repeat the above steps at progressively finer resolutions to refine the alignment.

## Hardware requirements

- A computer running Linux (recommended) or Windows
- A CUDA-compatible GPU with sufficient GPU memory: ≥ 30 bytes per voxel (30 GB / gigavoxel) of your 3D volume


## Installation

We recommend installing all dependencies via **conda** or **mamba**.

```bash
# Change into the repository root directory, then type:
mamba env create -n warpfield -f environment.yml
mamba activate warpfield
pip install -e .
```

## Quickstart
```python
import warpfield 

# 1. Load data (note: the two volumes are expected to be of the same array shape and resolution)
vol_ref = np.load("reference_volume.npy")
vol_mov = np.load("moving_volume.npy")

# 2. Choose registration recipe (here: loaded from a YAML file. See below for alternatives)
recipe = warpfield.Recipe.from_yaml('default.yml')

# 3. Register moving volume
vol_mov_reg, warp_map, _ = warpfield.register_volume(vol_ref, vol_mov, recipe)

# 4. Optional: apply the transformation to another volume (same shape and resolution)
vol_another_reg = warp_map.apply(vol_another)

# 5. Optional: apply inverse transformation to the reference volume
vol_ref_reg = warp_map.invert_fast().unwarp(vol_ref)

# 6. Optional: apply the warp transformation to a set of coordiantes (3-by-n array, in voxel units)
points = np.array([[1, 2, 3, 4], [5, 6, 7, 8], [9, 10, 11, 12]])
points_pushed = warp_map.push_coordinates(points)
points_pulled = warp_map.pull_coordinates(points) # inverse transformation
```

## Command-Line Interface (CLI)

The `warpfield` library provides a command-line interface. This allows you to perform registration directly from the terminal without writing Python code.

#### Usage

```bash
python -m warpfield --fixed <fixed_image_path> --moving <moving_image_path> --recipe <recipe_path> [options]
# You can use the `--help` flag to see detailed instructions for the CLI:
python -m warpfield --help
```

#### Required Arguments

- `--fixed`: Path to the fixed image/volume file (e.g., `.nii`, `.h5`, `.npy`, etc.).
- `--moving`: Path to the moving image/volume file (e.g., `.nii`, `.h5`, `.npy`, etc.).
- `--recipe`: Path to the recipe YAML file for registration.

#### Optional Arguments

- `--output`: Path to save the registered image/volume. Defaults to `<moving>_registered.h5` if not provided.
- `--compression`: Compression method for saving the registered volume. Default is `gzip`.
- `--invert`: Additionally, register the moving image to the fixed image.

#### Output Structure

The output file is an HDF5 file containing the following datasets:
- `/moving_reg`: The registered moving image.
- `/warp_map`: A group containing the warp field and its metadata:
  - `/warp_field`: The displacement field.
  - `/block_size`: The block size (in voxels).
  - `/block_stride`: The block stride (in voxels).
- `/fixed_reg_inv` (optional): The fixed image registered to the moving image (if `--invert` is used).

## Recipes

The registration pipeline is defined by a recipe. The recipe consists of a pre-filter that is applied to all volumes (typically a DoG filter to sharpen features) and list of levels, each of which contains a set of parameters for the registration process. Typically, each level corresponds to a different resolution of the displacement field (the block size), with the first level being the coarsest and the last level being the finest.

### Recipe parameters

| Pre-filter parameter      | Description                                                                 |
|-------------------|-----------------------------------------------------------------------------|
| `clip_thresh`     | Pixel value threshold for clipping each volume. Default is 0. This setting helps remove DC background, which can otherwise cause edges (the shifted volume is 0 outside the FOV).  |
| `dog`             | If True, apply a 3D Difference-of-Gaussians (DoG) pre-filter to each volume. Default is True.                 |
| `low`             | The σ<sub>low</sub> value for the 3D DoG pre-filter. Default is 0.5           |
| `high`            | The σ<sub>high</sub> value for the 3D DoG pre-filter. Default is 10.0. Note: σ<sub>low</sub> and σ<sub>high</sub> should be smaller and bigger than the feature of interest, respectively. A σ of 1 correponds to a FWHM of ~ 2.4.)             |


| Level parameter      | Description                                                                 |
|-------------------|-----------------------------------------------------------------------------|
| `block_size`      | Shape of blocks, whose rigid displacement is estimated. Positive numbers indicate block shape in voxels (e.g. [32, 16, 32]), while negative numbers are interpreted as "divide axis into this many blocks" (e.g. [-5, -5, -5] results in 5 blocks along each axis)|
| `block_stride`    | Block stride – determines whether blocks overlap. Either list of int (stride sizes in voxels) or scalar float (fraction of block_size). Default is 1.0 (no overlap). Set this to a smaller value (e.g. 0.5) for overlaping blocks and higher precision, but larger (e.g. 8x) memory footprint   |
| `project.max`     | If True, apply 3D -> 2D max projections to each volume block. If false, apply mean projections. Default is True           |
| `project.dog`     | If True, apply a DoG filter to each 2D projection. Default is True           |
| `project.low`     | The σ<sub>low</sub> value for the 2D DoG filter. Default is 0.5 voxels (pixels).                 |
| `project.high`    | The σ<sub>high</sub> value for the 2D DoG filter. Default is 10.0 voxels (pixels).               |
| `project.normalize`    | Whether to normalize the projections before calculating the cross-covariance (which would make it a cross-correlation). Defaults to False or 0.0. Values can range from 0.0 (False) to 1.0 (True). Values in between imply normalisation by `l2_norm**project.normalize`            |
| `project.periodic_smooth` | If True, apply periodic smoothing. Default is False. This can help reduce block-edge effects (affecting FFT-based correlation). |
| `tukey_ref`    | if not None, apply a Tukey window to the reference projections (alpha = tukey_ref). Default is 0.5. The Tukey window can reduce block-edge effects. |
| `smooth.sigmas`   | Sigmas for smoothing cross-correlations across blocks. Default is [1.0, 1.0, 1.0] blocks. |
| `smooth.shear`    | Shear parameter (specific to oblique plane wobble – ignore otherwise). Default is None.                      |
| `smooth.long_range_ratio` | Long range ratio for double gaussian kernel. Default is None. To deal with empty or low contrast regions, a second smooth with a larger (5x) sigma is applied to the cross-correlation maps and added. Typical values are between 0 (or None) and 0.1
| `median_filter`   | If True, apply median filter to the displacement field. Default is True                  |
| `affine`        | If True, fit affine transformation to the displacement field. Default is False. The affine fit ignores all edge voxels (to reduce edge effects) and therefore needs at least 4 blocks along each axis |
| `repeat`          | Number of iterations for this level. More repeats allow each block to deviate further from neighbors, despite smoothing. Typical values range from 1-10. Disable a level by setting repeats to 0.|


### Defining recipes

Recipes can be loaded from YAML files (either those shipped with this package, such as [default.yml](https://github.com/danionella/warpfield/blob/main/src/warpfield/recipes/default.yml), or your own): 

```python
recipe = warpfield.Recipe.from_yaml("default.yml")
# or your own recipe:
# recipe = warpfield.recipes.from_yaml("path/to/your/recipe.yaml")

# You can then modify recipe parameters programmatically, e.g.;
recipe.pre_filter.clip_thresh=10
recipe.levels[2].block_size = [32, 8, 32]
# ... etc.
```

Alternatively, you can define a recipe from scratch using the `Recipe` class. For example:

```python
# create a basic recipe with one affine registration level and a default pre-filter:
recipe = warpfield.Recipe()

# add non-rigid registration levels:
recipe.add_level(block_size=[128,128,128])
recipe.levels[-1].smooth.sigmas = [1.0,1.0,1.0]
recipe.levels[-1].repeat = 5

recipe.add_level(block_size=[64,64,64])
recipe.levels[-1].block_stride = 0.5
recipe.levels[-1].smooth.sigmas = [1.0,1.0,1.0]
recipe.levels[-1].repeat = 5

recipe.add_level(block_size=[32,32,32])
recipe.levels[-1].block_stride = 0.5
recipe.levels[-1].smooth.sigmas = [4.0,4.0,4.0]
recipe.levels[-1].smooth.long_range_ratio = 0.1
recipe.levels[-1].repeat = 5
```


## See also

- [Advanced Normalization Tools in Python (ANTsPy)](https://github.com/ANTsX/ANTsPy)
- [Computational Morphometry Toolkit (CMTK)](https://www.nitrc.org/projects/cmtk)
- [Constrained Large Deformation Diffeomorphic Image Registration (CLAIRE)
](https://github.com/andreasmang/claire)
