#image #comparison #labs #nvidia #error #flip #bindings

sys nv-flip-sys

FFI bindings to Nvidia Labs's ꟻLIP image comparison and error visualization library

2 releases

0.1.1 Jun 4, 2023
0.1.0 Jun 4, 2023

#231 in Visualization

Download history 1093/week @ 2023-12-13 691/week @ 2023-12-20 805/week @ 2023-12-27 1497/week @ 2024-01-03 1418/week @ 2024-01-10 1243/week @ 2024-01-17 1383/week @ 2024-01-24 1414/week @ 2024-01-31 1256/week @ 2024-02-07 903/week @ 2024-02-14 1505/week @ 2024-02-21 3332/week @ 2024-02-28 4447/week @ 2024-03-06 5101/week @ 2024-03-13 4758/week @ 2024-03-20 3667/week @ 2024-03-27

19,064 downloads per month
Used in nv-flip

(MIT OR Apache-2…

215KB
433 lines

nv-flip

bindings to Nvidia Labs's ꟻLIP image comparison and error visualization library.

This library allows you to visualize and reason about the human-noticable differences between rendered images. Especially when comparing images that are noisy or other small differences, FLIP's comparison can be more meaningful than a simple pixel-wise comparison.

comp

In order to keep a small dependency closure, this crate does not depend on image, but interop is simple.

Example

// First we load the "reference image". This is the image we want to compare against.
//
// We make sure to turn the image into RGB8 as FLIP doesn't deal with alpha.
let ref_image_data = image::open("../etc/tree-ref.png").unwrap().into_rgb8();
let ref_image = nv_flip::FlipImageRgb8::with_data(
    ref_image_data.width(),
    ref_image_data.height(),
    &ref_image_data
);

// We then load the "test image". This is the image we want to compare to the reference.
let test_image_data = image::open("../etc/tree-test.png").unwrap().into_rgb8();
let test_image = nv_flip::FlipImageRgb8::with_data(
    test_image_data.width(),
    test_image_data.height(),
    &test_image_data
);

// We now run the comparison. This will produce a "error map" that that is the per-pixel
// visual difference between the two images between 0 and 1.
//
// The last parameter is the number of pixels per degree of visual angle. This is used
// to determine the size of imperfections that can be seen. See the `pixels_per_degree`
// for more information. By default this value is 67.0.
let error_map = nv_flip::flip(ref_image, test_image, nv_flip::DEFAULT_PIXELS_PER_DEGREE);

// We can now visualize the error map using a LUT that maps the error value to a color.
let visualized = error_map.apply_color_lut(&nv_flip::magma_lut());

// Finally we can the final image into an `image` crate image and save it.
let image = image::RgbImage::from_raw(
    visualized.width(),
    visualized.height(),
    visualized.to_vec()
).unwrap();

// We can get statistics about the error map by using their "Pool" type,
// which is essentially a weighted histogram.
let mut pool = nv_flip::FlipPool::from_image(&error_map);

// These are the same statistics shown by the command line.
//
// The paper's writers recommend that, if you are to use a single number to
// represent the error, they recommend the mean.
println!("Mean: {}", pool.mean());
println!("Weighted median: {}", pool.get_percentile(0.5, true));
println!("1st weighted quartile: {}", pool.get_percentile(0.25, true));
println!("3rd weighted quartile: {}", pool.get_percentile(0.75, true));
println!("Min: {}", pool.min_value());
println!("Max: {}", pool.max_value());

The result of this example looks like this:

Reference ⠀⠀Test⠀⠀ ⠀Result⠀
comp comp comp

License

The binding and rust interop code is tri-licensed under MIT, Apache-2.0, and ZLib.

The ꟻLIP library itself is licensed under the BSD-3-Clause license.

The example images used are licensed under the Unsplash License.

License: MIT OR Apache-2.0 OR Zlib

Dependencies