Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456798/188
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dc.contributor.authorBharathi, Divya-
dc.contributor.authorSubrahmanyam, M.-
dc.contributor.authorRamesh, D. S.-
dc.contributor.authorRajendran, S.-
dc.date.accessioned2022-07-13T11:37:24Z-
dc.date.available2022-07-13T11:37:24Z-
dc.date.issued2020-
dc.identifier.citationCurrent Science, v. 119, 9en_US
dc.identifier.urihttp://library.iigm.res.in:8080/xmlui/handle/123456798/188-
dc.description.abstractNine total magnetic profiles in the S–N direction of the Central Indian Ocean (CIO) have been interpreted with spectral and Werner deconvolution techniques to obtain approximate depths to shallow (magnetic basement) and deeper (Curie isotherm) interfaces of the oceanic crust. From these preliminary depths, tentative crustal models for all these nine profiles are prepared. These tentative models of the area show varying thickness of the oceanic crust, supporting the deformation history. It is inferred from these tentative models that deformation extends beyond the zone identified south of 8°S latitude. There is good agreement between the spectral and Werner deconvolution depths.en_US
dc.language.isoenen_US
dc.subjectOceanic crusten_US
dc.subjectMagnetic anomalyen_US
dc.subjectDeformation zoneen_US
dc.subjectDeconvolution techniquesen_US
dc.subjectTentative modelen_US
dc.titleTentative model of crustal structure of the Central Indian Ocean deformation as inferred from spectral and Werner deconvolution techniques of magnetic dataen_US
dc.typeArticleen_US
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