Awesome
Learned SAR Speckle Filter: Despeckling Synthetic-Aperture Radar images using a Deep Residual Convolutional Neural Network
Tim Davis, Vinit Jain
Abstract:
Synthetic Aperture Radar (SAR) images suffer from the effects of speckle noise which arises from coherent summation of the signals scattered from ground scatters distributed randomly within each pixel. Speckling affects the human- and machine-readability of the images. Here, we propose to use deep learning to train a convolutional neural network model that outputs a despeckled SAR image. Convolutional Neural network architectures such as Noise2Noise and Noise2Void have been proven successful when the ground truth of the input image is not available. Hence, the primary goal of this research project is to train a deep residual CNN to ameliorate speckling in SAR images based on noisy input only. Lee and BM3D filters were evaluated to compare the results. The CNN models performed comparably to the filters in terms when evaluating against quasi-ground-truth images, and significantly outperformed the filters in terms of processing efficiency.
<p align="center">SAR image before and after despeckling </p>
Principal components
Pipeline
Please note that all code was written for and tested in Python3.
filter.py
This is the complete pipeline for processing raw SAR inputs into despeckled intensity images using a pretrained model.
It depends on tif2intensity.py
for converting the raw SAR input into a
(speckled) intensity image, predictor.py
for predicting despeckled image
patchs, and model.util
for helper functions.
usage: filter.py [-h] -o OUTPUT [--channels_last] -m MODEL
[--mean_correction MEAN_CORRECTION] [--no_weighting] [-r]
[-s STRIDE] [--single_channel_output]
input
positional arguments:
input tif image or directory of tif images
optional arguments:
-h, --help show this help message and exit
-o OUTPUT, --output OUTPUT
output file or directory
--channels_last indicate if the image channels are stored last
-m MODEL, --model MODEL
which model to use for processing [lin|log]
--mean_correction MEAN_CORRECTION
when to apply mean-correction to images
[smart|always|never]
--no_weighting do not center-weight image patches
-r recursively process subdirectories
-s STRIDE, --stride STRIDE
stride when processing images (default 128)
--single_channel_output
create a separate file for each channel (polarity)
Example usage with provided sample.tif
python3 filter.py -o result.tif -m lin --single_channel_output ./images/sample.tif
tif2intensity.py
These are helper functions for turning a raw SAR image into a (speckled) intensity image.
predictor.py
This is a class for making predictions using specified weights.
Training
Dataset generation
The model was trained using 2-channel intensity images, with the first channel for
the VH intensity image and the second channel for the VV intensity image. These 2-channel
intensity images were created from 4-channel raw SAR images using tif2intensity.py
.
The data must be batched into sets of identical views, for which batcher.py
was used.
This takes a .csv
file as input that indicates to which set each image belongs (see
example below) and batches each set into its own directory. Set number 0 is reserved for
"bad" images that are either in an incorrect format or do not fit into any other set.
These will be ignored by the batcher. Negative numbered sets are validation images
and will be excluded from the training data by model.pairgenerator.py
during training,
but still copied to the output directory for later use in validation.
volcano | orbit | image | set |
---|---|---|---|
Ambrym | 59 | S1_20181211T182129_59_int | 0 |
... | ... | ... | ... |
train.py
Actual training of the model is handled by train.py
. It depends on model.py
for
the model specification, pairgenerator.py
for loading the dataset, and util.py
for
helper functions
usage: train.py [-h] --image_dir IMAGE_DIR [--batch_size BATCH_SIZE]
[--nb_epochs NB_EPOCHS] [--lr LR] [--steps STEPS]
[--weight WEIGHT] [--output_path OUTPUT_PATH] [--model MODEL]
[--min_date_separation MIN_DATE_SEPARATION]
[--logspace LOGSPACE]
train noise2noise model
optional arguments:
-h, --help show this help message and exit
--image_dir IMAGE_DIR
image dir for input and target values (default: None)
--batch_size BATCH_SIZE
batch size (default: 32)
--nb_epochs NB_EPOCHS
number of epochs (default: 20)
--lr LR learning rate (default: 0.01)
--steps STEPS steps per epoch (default: 32)
--weight WEIGHT weight file for restart (default: None)
--output_path OUTPUT_PATH
checkpoint dir (default: checkpoints)
--model MODEL model architecture (default: red30)
--min_date_separation MIN_DATE_SEPARATION
Minimum date between image pair acquisition (default:
6)
--logspace LOGSPACE Convert images to logspace before training (default:
False)
The following command was used for linear-space training:
python ./model/train.py --image_dir ./vhvv_sets/ --batch_size 16 --nb_epochs 1000 --lr 0.001 --steps 32 --output_path ./checkpoints_vhvv_lin/ --min_date_separation 90
The following command was used for logarithmic-space training:
python ./model/train.py --image_dir ./vhvv_sets/ --batch_size 16 --nb_epochs 1000 --lr 0.001 --steps 32 --output_path ./checkpoints_vhvv/ --min_date_separation 90 --logspace
model.py
This contains the specification for the architecture of the model.
pairgenerator.py
This contains the imgloader
class, which extends keras.utils.Sequence
and is used for
loading the dataset during training. All loading is done through on-the-fly loading
of randomly selected, matching image patches.
Evaluation
Evaluation of the results was done using compare_psnr
and compare_ssim
from skimage.measure
.
All images for two volcanoes (Ertaale and Pitonfournaise) were either dedicated to evaluation sets
or excluded from training set, so that no knowledge of these specific volcanoes was acquired by
the CNN during the training process.
Lee, Kuan, and Frost filters were taken from the PyRadar package. BM3D filtering was done using the PyBM3D package.