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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Bandyopadhyay, Sanmoy | en_US |
dc.contributor.author | Das, Saurabh | en_US |
dc.contributor.author | Datta, Abhirup | en_US |
dc.date.accessioned | 2022-03-17T01:00:00Z | - |
dc.date.accessioned | 2022-03-17T15:29:52Z | - |
dc.date.available | 2022-03-17T01:00:00Z | - |
dc.date.available | 2022-03-17T15:29:52Z | - |
dc.date.issued | 2020 | - |
dc.identifier.citation | Bandyopadhyay, 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/URSIGASS49373.2020.9232314 | en_US |
dc.identifier.isbn | 9.78946E+12 | - |
dc.identifier.other | EID(2-s2.0-85096848130) | - |
dc.identifier.uri | https://doi.org/10.23919/URSIGASS49373.2020.9232314 | - |
dc.identifier.uri | https://dspace.iiti.ac.in/handle/123456789/3658 | - |
dc.description.abstract | Accurate 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.iso | en | en_US |
dc.publisher | Institute of Electrical and Electronics Engineers Inc. | en_US |
dc.source | 2020 33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020 | en_US |
dc.subject | Hough transforms | en_US |
dc.subject | Active contour method | en_US |
dc.subject | Benchmark datasets | en_US |
dc.subject | Circular Hough transforms | en_US |
dc.subject | Co segmentations | en_US |
dc.subject | Color features | en_US |
dc.subject | Energy functions | en_US |
dc.subject | Initial contour | en_US |
dc.subject | Novel applications | en_US |
dc.subject | Image segmentation | en_US |
dc.title | Simultaneous Coronal Hole Segmentation from Solar EUV Images using the Image Co-segmentation Technique | en_US |
dc.type | Conference Paper | en_US |
Appears in Collections: | Department of Astronomy, Astrophysics and Space Engineering |
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