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Volumetric Image Visualization Alexandre Xavier Falc ao LIDS - Institute of Computing - UNICAMP afalcao@ic.unicamp.br Alexandre Xavier Falc ao Volumetric Image Visualization The Simplest Visualization Methods In order to visualize the


  1. Volumetric Image Visualization Alexandre Xavier Falc˜ ao LIDS - Institute of Computing - UNICAMP afalcao@ic.unicamp.br Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  2. The Simplest Visualization Methods In order to visualize the image content, the simplest methods are the extraction of axial, coronal, and sagital slices, Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  3. The Simplest Visualization Methods In order to visualize the image content, the simplest methods are the extraction of axial, coronal, and sagital slices, the adjustments of brightness and contrast by radiometric transformations , when presenting the images of those slices, Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  4. The Simplest Visualization Methods In order to visualize the image content, the simplest methods are the extraction of axial, coronal, and sagital slices, the adjustments of brightness and contrast by radiometric transformations , when presenting the images of those slices, the use of color compositions to further enhance nuances in those images, given that humans can perceive 7 millions of colors and only 30 tones of gray. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  5. Radiometric Transformation For an image ˆ I = ( D I , I ) with voxel intensities I ( p ) = l in the range [ l min , l max ] for any p ∈ D I , a radiometric transformation is a mapping T ( l ) = k that creates another image ˆ J = ( D I , J ) with values J ( p ) = k ∈ [ k min , k max ]. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  6. Radiometric Transformation Given that T changes the image’s intensity interval, it affects the distribution of its gray values, named histogram . A normalized histogram h ( l ), for instance, is defined as 1 � h ( l ) = δ ( l − I ( p )) , | D I | ∀ p ∈ D I where δ ( x ) = 1, for x = 0, and δ ( x ) = 0, otherwise. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  7. Radiometric Transformation Given that T changes the image’s intensity interval, it affects the distribution of its gray values, named histogram . A normalized histogram h ( l ), for instance, is defined as 1 � h ( l ) = δ ( l − I ( p )) , | D I | ∀ p ∈ D I where δ ( x ) = 1, for x = 0, and δ ( x ) = 0, otherwise. It reveals that dark (bright) images with low contrast present higher concentration of voxels with low (high) values. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  8. Radiometric Transformation Given that T changes the image’s intensity interval, it affects the distribution of its gray values, named histogram . A normalized histogram h ( l ), for instance, is defined as 1 � h ( l ) = δ ( l − I ( p )) , | D I | ∀ p ∈ D I where δ ( x ) = 1, for x = 0, and δ ( x ) = 0, otherwise. It reveals that dark (bright) images with low contrast present higher concentration of voxels with low (high) values. A radiometric transformation can improve brightness and contrast by distributing those values within the possible range [0 , 2 b − 1], for a depth b bits per voxel. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  9. Linear Stretching A linear stretching is the simplest way to map intensities from [ l 1 , l 2 ], l min ≤ l 1 ≤ l 2 ≤ l max into [ k 1 , k 2 ], when transforming ˆ I = ( D I , I ) into ˆ J = ( D I , J ).  k 1 , for l < l 1 ,   ( k 2 − k 1 ) = ( l 2 − l 1 ) ( l − l 1 ) + k 1 , for l 1 ≤ l < l 2 , k  k 2 , for l ≥ l 2 .  It is called Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  10. Linear Stretching A linear stretching is the simplest way to map intensities from [ l 1 , l 2 ], l min ≤ l 1 ≤ l 2 ≤ l max into [ k 1 , k 2 ], when transforming ˆ I = ( D I , I ) into ˆ J = ( D I , J ).  k 1 , for l < l 1 ,   ( k 2 − k 1 ) = ( l 2 − l 1 ) ( l − l 1 ) + k 1 , for l 1 ≤ l < l 2 , k  k 2 , for l ≥ l 2 .  It is called ao, when k 2 = 2 b − 1, k 1 = 0, l 1 = l min , and normaliza¸ c˜ l 2 = l max ; Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  11. Linear Stretching A linear stretching is the simplest way to map intensities from [ l 1 , l 2 ], l min ≤ l 1 ≤ l 2 ≤ l max into [ k 1 , k 2 ], when transforming ˆ I = ( D I , I ) into ˆ J = ( D I , J ).  k 1 , for l < l 1 ,   ( k 2 − k 1 ) = ( l 2 − l 1 ) ( l − l 1 ) + k 1 , for l 1 ≤ l < l 2 , k  k 2 , for l ≥ l 2 .  It is called ao, when k 2 = 2 b − 1, k 1 = 0, l 1 = l min , and normaliza¸ c˜ l 2 = l max ; negative, when k 2 = l min , k 1 = l max , l 1 = l min , and l 2 = l max ; Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  12. Linear Stretching A linear stretching is the simplest way to map intensities from [ l 1 , l 2 ], l min ≤ l 1 ≤ l 2 ≤ l max into [ k 1 , k 2 ], when transforming ˆ I = ( D I , I ) into ˆ J = ( D I , J ).  k 1 , for l < l 1 ,   ( k 2 − k 1 ) = ( l 2 − l 1 ) ( l − l 1 ) + k 1 , for l 1 ≤ l < l 2 , k  k 2 , for l ≥ l 2 .  It is called ao, when k 2 = 2 b − 1, k 1 = 0, l 1 = l min , and normaliza¸ c˜ l 2 = l max ; negative, when k 2 = l min , k 1 = l max , l 1 = l min , and l 2 = l max ; window & level, when k 2 = 2 b − 1, k 1 = 0, and l 1 < l 2 , such that the level l 1 + l 2 affects brightness and the window l 2 − l 1 2 affects contrast; and Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  13. Linear Stretching A linear stretching is the simplest way to map intensities from [ l 1 , l 2 ], l min ≤ l 1 ≤ l 2 ≤ l max into [ k 1 , k 2 ], when transforming ˆ I = ( D I , I ) into ˆ J = ( D I , J ).  k 1 , for l < l 1 ,   ( k 2 − k 1 ) = ( l 2 − l 1 ) ( l − l 1 ) + k 1 , for l 1 ≤ l < l 2 , k  k 2 , for l ≥ l 2 .  It is called ao, when k 2 = 2 b − 1, k 1 = 0, l 1 = l min , and normaliza¸ c˜ l 2 = l max ; negative, when k 2 = l min , k 1 = l max , l 1 = l min , and l 2 = l max ; window & level, when k 2 = 2 b − 1, k 1 = 0, and l 1 < l 2 , such that the level l 1 + l 2 affects brightness and the window l 2 − l 1 2 affects contrast; and limiarization (binarization, thresholding), when k 2 = 2 b − 1, k 1 = 0, and l 1 = l 2 . Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  14. Dark image with low contrast (a) (b) (a) Image ˆ I of an MR slice of a breast with carcinoma and (b) its normalized histogram. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  15. After linear stretching (a) (b) (a) Image ˆ J after linear stretching and (b) the comparison between the previous and the resulting normalized histograms. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  16. Dark images in practice The presence of blood flow in MR can often create dark images. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  17. Dark images in practice Those brightest voxels from the blood flow can be easily detected based on the cumulative histogram l max � h ( l ′ ) , h a ( l ) = l ′ = l min which corresponds to the area below the normalized histogram h ( l ). An example of h a ( l ), when h ( l ) is the normalized histogram of the MR-breast slice. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  18. Dark images in practice In the case of the MR image of the brain, we may then assume that 2% of the brightest voxels are blood flow and suppress their intensities by linear stretching with l 2 as the highest value for h a ( l ) < 0 . 98, l 1 = l min , k 1 = 0, and k 2 = 2 b − 1. Another option is to interactively adjust the percentages of window and level in the user interface. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  19. Color Humans perceive colors — i.e., light with wavelengths in [0 . 4 µ m − 0 . 7 µ m ] — in different ways by their cone cells (photoreceptors). Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  20. Color Humans perceive colors — i.e., light with wavelengths in [0 . 4 µ m − 0 . 7 µ m ] — in different ways by their cone cells (photoreceptors). Most of the visible colors can be produced by a combination of monochromatic light in the wavelengths of the blue, red, and green. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  21. Color Humans perceive colors — i.e., light with wavelengths in [0 . 4 µ m − 0 . 7 µ m ] — in different ways by their cone cells (photoreceptors). Most of the visible colors can be produced by a combination of monochromatic light in the wavelengths of the blue, red, and green. One can also decompose a color into three independent components: intensity (brightness perception), hue (the most predominant color perception), and saturation (perception of color purity related to the white). Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  22. Color A color can then be represented in different color spaces : RGB, HSV, YCbCr, YCgCo, Lab, Luv, etc. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

  23. Color A color can then be represented in different color spaces : RGB, HSV, YCbCr, YCgCo, Lab, Luv, etc. Considering RGB and YCgCo, for instance, the second separates intensity in Y and hue with saturation in Cg and Co. Alexandre Xavier Falc˜ ao Volumetric Image Visualization

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