Category Archives: Julia

Super fast pattern search: The FFT trick

By: Júlio Hoffimann

Re-posted from: https://juliohm.github.io/science/fft-trick/

In today’s post, I would like to document an old trick in image processing sometimes referred to as “The FFT trick” for exhaustive pattern search.

Although I would like to give credit to the person who introduced the trick in the literature, I don’t have this information with me. Please leave a comment if you have references.

Learning with a sliding window

Filtering an image with a sliding window is a routine operation in various disciplines like image processing, computer vision, geostatistics, and deep learning (e.g. convolutional neural networks), to name a few.

Sliding window on my breakfast.

Depending on the application, this operation serves different purposes. It is used everywhere as illustrated in the table:

Field of study Typical window Purposes
Image processing
  • Sobel kernel: $$\small\begin{bmatrix}1 & 0 & -1 \\ 2 & 0 & -2\\ 1 & 0 & -1\end{bmatrix}$$
  • Gaussian blur: $$\small\frac{1}{16}\begin{bmatrix}1 & 2 & 1 \\ 2 & 4 & 2\\ 1 & 2 & 1\end{bmatrix}$$
  • Edge detection
  • Blurring
  • Denoising
Computer vision Same as in Image processing
  • Image descriptors (e.g. GIST, HoG)
  • Invariance and alignment
Geostatistics A spatial pattern:
  • Pattern search
Deep learning Random weights:
  • Convolutional neural networks

BRAINSTORM: Why sliding windows? Couldn’t we learn more by using a different technique? What does a sliding window misses in terms of learning? :thinking:

Given its importance, a great deal of time was devoted by the scientific community to optimizing software and hardware for filtering images (or arrays) with sliding windows.

This post is about a clever trick that exploits legacy high-performance filtering algorithms to speed up pattern search on very large images.

FFT filtering

Consider a first naive implementation of the filtering operation in Julia that loops over the input image, extracts a subimage, multiplies it with the window entrywise, and adds the results:

function naivefilter(image::AbstractArray, window::AbstractArray)
  nx, ny = size(image)
  wx, wy = size(window)

  [sum(window .* image[i:i+wx-1,j:j+wy-1]) for i=1:nx-wx+1, j=1:ny-wy+1]
end

It works well, but is relatively slow for industry standards. Compare it to the efficient implementation available in Images.jl:

using Images
using BenchmarkTools

image = zeros(100,100)
window = zeros(3,3)

@benchmark naivefilter(image, window)
@benchmark imfilter(image, window)

# BenchmarkTools.Trial: (naivefilter)
#   memory estimate:  7.99 MiB
#   allocs estimate:  192093
#   --------------
#   minimum time:     6.512 ms (0.00% GC)
#   median time:      6.638 ms (0.00% GC)
#   mean time:        7.209 ms (7.67% GC)
#   maximum time:     10.569 ms (15.77% GC)
#   --------------
#   samples:          693
#   evals/sample:     1
#   time tolerance:   5.00%
#   memory tolerance: 1.00%
#
# BenchmarkTools.Trial: (imfilter)
#   memory estimate:  204.03 KiB
#   allocs estimate:  268
#   --------------
#   minimum time:     378.637 μs (0.00% GC)
#   median time:      388.839 μs (0.00% GC)
#   mean time:        406.210 μs (2.51% GC)
#   maximum time:     2.035 ms (78.63% GC)
#   --------------
#   samples:          10000
#   evals/sample:     1
#   time tolerance:   5.00%
#   memory tolerance: 1.00%

From the output, we notice turning into s and MiB turning into KiB. Besides the cache-friendly code that Tim Holy and others have written, I would like to comment on another optimization that Images.jl does that is not available in other image processing packages and programming languages.

Image filtering can alternatively be implemented with Fast Fourier Transforms (FFTs). The details of the algorithm and the theory behind it are beyond the scope of this post. The message that I want to convey is that depending on the window size, particularly for large windows, the FFT algorithm is much faster.

In Images.jl you can call the FFT algorithm explicitly by using:

imfilter(image, window, Algorithm.FFT())

but you don’t need to, Images.jl will call the faster algorithm depending on the window size you pass to it! :raised_hands:

The switch point between algorithms was set by means of benchmarks on a few modern processors. Feel free to submit a pull request if you feel that the switch point isn’t quite right for your hardware.

Now that we’ve seen that image filtering is a super efficient operation (specially in Julia), let’s exploit it to find patterns in images.

Given an image and a spatial pattern , an exhaustive pattern search consists of computing a distance (or dissimilarity) between and all subimages of . The subimages for which the distance is smallest are called matches. If the computed distance is zero, the match is called a perfect match.

Now is the trick. Consider the Euclidean distance and relax the notation to mean

Loop over all subimages of and compute

where and have the same size. It turns out that we can implement this operation by rewriting

and replacing the original inefficient loop with two FFT filtering + one reduction:

 = imfilter(A.^2, ones(B))
AB = imfilter(A, B)
 = sumabs2(B)

D = abs( - 2AB + ) # here "abs" takes care of floating point errors

Isn’t that awesome? This trick was crucial in my ImageQuilting.jl package, it allowed me to process large 3D images in minutes instead of hours.

Finally, I would like to add that high-performance GPU implementations of FFT filtering are available in Julia. You can set an option in your package to use CLFFT.jl and have the fastest software in the market. :blush:

Build & Deploy Machine Learning Apps on Big Data Platforms with Microsoft Linux Data Science Virtual Machine

This post is authored by Gopi Kumar, Principal Program Manager in the Data Group at Microsoft.

This post covers our latest additions to the Microsoft Linux Data Science Virtual Machine (DSVM), a custom VM image on Azure, purpose-built for data science, deep learning and analytics. Offered in both Microsoft Windows and Linux editions, DSVM includes a rich collection of tools, seen in the picture below, and makes you more productive when it comes to building and deploying advanced machine learning and analytics apps.

The central theme of our latest Linux DSVM release is to enable the development and testing of ML apps for deployment to distributed scalable platforms such as Spark, Hadoop and Microsoft R Server, for operating on data at a very large scale. In addition, with this release, DSVM also offers Julia Computing’s JuliaPro on both Linux and Windows editions.


Here’s more on the new DSVM components you can use to build and deploy intelligent apps to big data platforms:

Microsoft R Server 9.0

Version 9.0 of Microsoft R Server (MRS) is a major update to enterprise-scale R from Microsoft, supporting parallel and distributed computation. MRS 9.0 supports analytics execution in the Spark 2.0 context. There’s a new architecture and simplified interface for deploying R models and functions as web services via a new library called mrsdeploy, which makes it easy to consume models from other apps using the open Swagger framework.

Local Spark Standalone Instance

Spark is one of the premier platforms for highly scalable big data analytics and machine learning. Spark 2.0 launched in mid-2016 and brings several improvements such as the revised machine learning library (MLLib), scaling and performance optimization, better ANSI SQL compliance and unified APIs. The Linux DSVM now offers a standalone Spark instance (based on the Apache Spark distribution), PySpark kernel in Jupyter to help you build and test applications on the DSVM and deploy them on large scale clusters like Azure HDInsight Spark or your own on-premises Spark cluster. You can develop your code using either Jupyter notebook or with the included community edition of the Pycharm IDE for Python or RStudio for R.

Single Node Local Hadoop (HDFS and YARN) Instance

To make it easier to develop Hadoop programs and/or use HDFS storage locally for development and testing, a single node Hadoop installation is built into the VM. Also, if you are developing on the Microsoft R Server for execution in Hadoop or Spark remote contexts, you can first test things locally on the Linux DSVM and then deploy the code to a remote scaled out Hadoop or Spark cluster or to Microsoft R Server. These DSVM additions are designed to help you iterate rapidly when developing and testing your apps, before they get deployed into large-scale production big data clusters.

The DSVM is also a great environment for self-learning and running training classes on big data technologies. We provide sample code and notebooks to help you get started quickly on the different data science tools and technologies offered.

DSVM Resources

New to DSVM? Here are resources to get you started:

Linux Edition

Windows Edition

The goal of DSVM is to make data scientists and developers highly productive in their work and provide a broad array of popular tools. We hope you find it useful to have these new big data tools pre-installed with the DSVM.

We always appreciate feedback, so please send in your comments below or share your thoughts with us at the DSVM community forum.

Gopi

imfilter and arrays

By: Michele Pratusevich

Re-posted from: http://learningjulia.com/2017/03/09/imfilter-and-arrays.html

Whereas in my last post I manually wrote a blur kernel and code to convolve an image, I didn’t want to do that every time an image convolution came up. So in this post I learned about the imfilter function from the ImageFiltering.jl package. I also learned about the @time macro and had a small aside on array creation.

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