Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/3658
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dc.contributor.authorBandyopadhyay, Sanmoyen_US
dc.contributor.authorDas, Saurabhen_US
dc.contributor.authorDatta, Abhirupen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-17T15:29:52Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-17T15:29:52Z-
dc.date.issued2020-
dc.identifier.citationBandyopadhyay, S., Das, S., & Datta, A. (2020). Simultaneous coronal hole segmentation from solar EUV images using the image co-segmentation technique. Paper presented at the 2020 33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020, doi:10.23919/URSIGASS49373.2020.9232314en_US
dc.identifier.isbn9.78946E+12-
dc.identifier.otherEID(2-s2.0-85096848130)-
dc.identifier.urihttps://doi.org/10.23919/URSIGASS49373.2020.9232314-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/3658-
dc.description.abstractAccurate detection of coronal holes (CHs) is an important issue in the domain of solar physics, since, CHs plays an vital role in controlling the overall space weather and generation of solar wind. In this paper a novel application of image co-segmentation (Co-seg) has been proposed for accurate detection of coronal hole simultaneously in two solar disk images of different band. For the task of Co-seg circular Hough transform inspired active contour method (ACM) have been proposed. Here the circular Hough transform has been introduced to setup the initial contours for the ACM based Co-seg. In later stage, the initiated contours has been evolved based on the energy function by incorporating the color features. At the final stage, when the contours do not deform any more is considered as the final contours position and the regions inside the contours is extracted as the CHs regions from both the images under consideration. The experiment has been conducted on few benchmark datasets and the corresponding results have been compared with the results of other existing techniques. The compared outcomes validate the performance of the applied technique in detection of coronal holes in solar disk. © 2020 URSI.en_US
dc.language.isoenen_US
dc.publisherInstitute of Electrical and Electronics Engineers Inc.en_US
dc.source2020 33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020en_US
dc.subjectHough transformsen_US
dc.subjectActive contour methoden_US
dc.subjectBenchmark datasetsen_US
dc.subjectCircular Hough transformsen_US
dc.subjectCo segmentationsen_US
dc.subjectColor featuresen_US
dc.subjectEnergy functionsen_US
dc.subjectInitial contouren_US
dc.subjectNovel applicationsen_US
dc.subjectImage segmentationen_US
dc.titleSimultaneous Coronal Hole Segmentation from Solar EUV Images using the Image Co-segmentation Techniqueen_US
dc.typeConference Paperen_US
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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