001     59280
005     20191029145035.0
024 7 _ |2 DOI
|a 10.1007/s11263-008-0145-5
024 7 _ |2 WOS
|a WOS:000259370500006
037 _ _ |a PreJuSER-59280
041 _ _ |a eng
082 _ _ |a 004
084 _ _ |2 WoS
|a Computer Science, Artificial Intelligence
100 1 _ |0 P:(DE-HGF)0
|a Preusser, T.
|b 0
245 _ _ |a Building blocks for computer vision with stochastic partial differential equations
260 _ _ |a Dordrecht [u.a.]
|b Springer Science + Business Media B.V
|c 2008
300 _ _ |a 375 - 405
336 7 _ |0 PUB:(DE-HGF)16
|2 PUB:(DE-HGF)
|a Journal Article
336 7 _ |2 DataCite
|a Output Types/Journal article
336 7 _ |0 0
|2 EndNote
|a Journal Article
336 7 _ |2 BibTeX
|a ARTICLE
336 7 _ |2 ORCID
|a JOURNAL_ARTICLE
336 7 _ |2 DRIVER
|a article
440 _ 0 |0 19561
|a International Journal of Computer Vision
|v 80
|x 0920-5691
|y 3
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a We discuss the basic concepts of computer vision with stochastic partial differential equations (SPDEs). In typical approaches based on partial differential equations (PDEs), the end result in the best case is usually one value per pixel, the "expected" value. Error estimates or even full probability density functions PDFs are usually not available. This paper provides a framework allowing one to derive such PDFs, rendering computer vision approaches into measurements fulfilling scientific standards due to full error propagation. We identify the image data with random fields in order to model images and image sequences which carry uncertainty in their gray values, e.g. due to noise in the acquisition process.The noisy behaviors of gray values is modeled as stochastic processes which are approximated with the method of generalized polynomial chaos (Wiener-Askey-Chaos). The Wiener-Askey polynomial chaos is combined with a standard spatial approximation based upon piecewise multi-linear finite elements. We present the basic building blocks needed for computer vision and image processing in this stochastic setting, i.e. we discuss the computation of stochastic moments, projections, gradient magnitudes, edge indicators, structure tensors, etc. Finally we show applications of our framework to derive stochastic analogs of well known PDEs for de-noising and optical flow extraction. These models are discretized with the stochastic Galerkin method. Our selection of SPDE models allows us to draw connections to the classical deterministic models as well as to stochastic image processing not based on PDEs. Several examples guide the reader through the presentation and show the usefulness of the framework.
536 _ _ |0 G:(DE-Juel1)FUEK407
|2 G:(DE-HGF)
|a Terrestrische Umwelt
|c P24
|x 0
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |2 WoSType
|a J
653 2 0 |2 Author
|a image processing
653 2 0 |2 Author
|a error propagation
653 2 0 |2 Author
|a random fields
653 2 0 |2 Author
|a polynomial chaos
653 2 0 |2 Author
|a stochastic partial differential equations
653 2 0 |2 Author
|a stochastic galerkin method
653 2 0 |2 Author
|a stochastic finite element method
700 1 _ |0 P:(DE-Juel1)129394
|a Scharr, H.
|b 1
|u FZJ
700 1 _ |0 P:(DE-Juel1)129347
|a Krajsek, K.
|b 2
|u FZJ
700 1 _ |0 P:(DE-HGF)0
|a Kirby, R.M.
|b 3
773 _ _ |0 PERI:(DE-600)1479903-0
|a 10.1007/s11263-008-0145-5
|g Vol. 80, p. 375 - 405
|p 375 - 405
|q 80<375 - 405
|t International journal of computer vision
|v 80
|x 0920-5691
|y 2008
856 7 _ |u http://dx.doi.org/10.1007/s11263-008-0145-5
909 C O |o oai:juser.fz-juelich.de:59280
|p VDB
913 1 _ |0 G:(DE-Juel1)FUEK407
|b Erde und Umwelt
|k P24
|l Terrestrische Umwelt
|v Terrestrische Umwelt
|x 0
914 1 _ |y 2008
915 _ _ |0 StatID:(DE-HGF)0010
|a JCR/ISI refereed
920 1 _ |0 I:(DE-Juel1)ICG-3-20090406
|d 31.10.2010
|g ICG
|k ICG-3
|l Phytosphäre
|x 1
970 _ _ |a VDB:(DE-Juel1)93275
980 _ _ |a VDB
980 _ _ |a ConvertedRecord
980 _ _ |a journal
980 _ _ |a I:(DE-Juel1)IBG-2-20101118
980 _ _ |a UNRESTRICTED
981 _ _ |a I:(DE-Juel1)IBG-2-20101118
981 _ _ |a I:(DE-Juel1)ICG-3-20090406


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21