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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/11385
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dc.contributor.authorPasari, Sumanta-
dc.date.accessioned2023-08-14T09:39:08Z-
dc.date.available2023-08-14T09:39:08Z-
dc.date.issued2021-
dc.identifier.urihttps://ieeexplore.ieee.org/document/9792070-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/xmlui/handle/123456789/11385-
dc.description.abstractRidges and fractures along the interplate boundaries influence arc morphology and earthquake rupture propagation. The space-based interferometric synthetic aperture radar (InSAR) approach has been used to investigate tectonic deformation along the Delhi-Haridwar Ridge (DHR) in the Indo-Gangetic alluvial plain and below the Himalayan arc. The deformation rates are derived from InSAR data using 390 interferograms from 2017 to 2021. The InSAR line of sight velocity reveals prominent subsidence along the DHR, whereas the Himalayan arc surrounding DHR shows upliftment. In addition, continuous microseismicity and persistent subsidence along the DHR indicate aseismic creeping in this area, indicating an unfavorable condition for large rupture formation and propagation in the future.en_US
dc.language.isoenen_US
dc.publisherIEEEen_US
dc.subjectMathematicsen_US
dc.subjectInSARen_US
dc.subjectTectonic deformationen_US
dc.subjectInterferogramen_US
dc.subjectDelhi-Haridwar Ridgeen_US
dc.titleTectonic deformation along the Delhi-Haridwar Ridge revealed by InSAR observations: Preliminary resultsen_US
dc.typeArticleen_US
Appears in Collections:Department of Mathematics

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