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University of Groningen

Scalable max-tree and alpha-tree algorithm for high resolution, multispectral, and extreme dynamic range images

You, Jiwoo; Wilkinson, M.H.F.; Trager, Scott

IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below.

Document Version

Publisher's PDF, also known as Version of record

Publication date: 2018

Link to publication in University of Groningen/UMCG research database

Citation for published version (APA):

You, J., Wilkinson, M. H. F., & Trager, S. (2018). Scalable max-tree and alpha-tree algorithm for high resolution, multispectral, and extreme dynamic range images. Poster session presented at XXX Canary Islands Winter School of Astrophysics, Tenerife, Spain.

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Kapteyn Astronomical Institute & Bernoulli Institute

[1] Teeninga, Paul, et al.: International Symposium on Mathematical Morphology and Its Applications to Signal and Image Processing (ISMM), pp. 157-168 (2015). [2] Moschini, U., Meijster A., and Wilkinson M.H.F.: IEEE transactions on pattern analysis and machine intelligence 40(3) 513–526 (2018)

[3] Ouzounis, G.K., and Soille P.: JRC Technical Reports, Joint Research Centre, European Commission (2012)

[4] Wilkinson M.H.F.: 2011 18th IEEE International Conference on Image Processing (ICIP), pp. 1021–1024 (2011)

The proposed

α–tree algorithm achieved 3x execution speed increase

The proposed

α–tree algorithm reduced the memory use by 41%

We modeled the

α–tree size using an exponential decay function

We will apply the

α–TSE to pilot max–tree of astronomical images in [2]

Alpha Tree Flooding Algorithm

▪ Algorithm design motivated from [2] and [4] with some modifications for α–trees

Alpha Tree Size Estimation (α–TSE)

The tree size can be easily estimated from pixel dissimilarity histogram (dhist)

D is a root mean squared deviation between dhist and flat histogram

We found that the tree size is an exponential decay function of D

𝐷 = σ𝑒∈𝐸 𝑑ℎ𝑖𝑠𝑡 𝑒

2 − |𝐸|

𝐸 − 1

𝑇𝑆𝐸 𝐷 = 𝑁𝑒−𝜋𝐷 N: Image sizeE: Set of neighbouring pixel pairs

The Test Dataset

▪ Manually collected 254 low dynamic range (8-bit) optical images

▪ Experiments conducted in both colour and grey-scale

▪ Results on grey-scale images are shown here

Partition Tree (Max tree, Alpha tree)

▪ Tree data structures used in morphological image filtering

▪ Connected morphological filters are very useful for faint object detection, as shown by [1] and [2]

▪ Alpha tree is useful in analysis of satellite or planetary images [3]

A Novel Fast, Memory Efficient Alpha Tree Algorithm

▪ The first Alpha tree flooding algorithm

▪ The first study to accurately estimate the partition tree size to increase memory efficiency

Execution Speed Improvement by Flooding

▪ The proposed algorithm was compared to Ouzounis–Soille’s [3]

▪ The proposed algorithm achieved 3x speed increase

The α–TSE Modeling

▪ The α–TSE model was optimized to maximize memory efficiency

▪ Confidence Interval (95%) of TSE model error was only 5.8% of the maximum tree size (N)

The α–TSE Performance

▪ The α–TSE reduced average memory usage by 41%

▪ Computation increase of α–TSE was only 0.3% (14.3 Mpix/s)

▪ The α–TSE performed better than other dynamic memory reallocation schemes

▪ Execution speed and memory usage in α–TSE were anti-correlated – Execution speed can be predicted using α–TSE

3x Execution Speed Increase

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