Rock magnetic signatures of the dalma Formation in the Singhbhum mobile belt, Eastern India

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dc.contributor.author Chatterjee, Saurodeep
dc.contributor.author Basavaiah, N.
dc.contributor.author Mondal, Supriya
dc.contributor.author Gain, Debesh
dc.date.accessioned 2022-07-27T04:41:47Z
dc.date.available 2022-07-27T04:41:47Z
dc.date.issued 2021
dc.identifier.citation Journal of Geological Society of India, 97, 635–642 (2021). https://doi.org/10.1007/s12594-021-1738-7 en_US
dc.identifier.uri http://library.iigm.res.in:8080/xmlui/handle/123456798/204
dc.description.abstract Petrography and rock magnetic properties of the Dalma volcanics (DV) and associated meta-sediments of Singhbhum mobile belt (SMB) are presented to describe magnetic grain size and Fe-Ti oxide mineralogy of the volcano-sedimentary sequence. Petrography revealed the presence of Ti-magnetite, hematite, ilmenite and pyrite in quartz-biotite-sericite-muscovite schists, quartzites, and volcanic rocks. The average value of magnetic susceptibility (c) is 5.6 x 10-7 m3/kg, anhysteretic remanent magnetization (ARM) is 2.25 x 10-5Am2/kg, saturating isothermal remanent magnetization (SIRM) is 403.33 x 10-5 Am2/kg, soft IRM is 240.2 x 10-5 Am2/kg, hard IRM is 77.56 x 10-5 Am2/kg, and natural remanent magnetization (NRM) is 54.1 mA/m. The central tendency of the inter-parametric ratio ARM/c is 0.06 kAm-1, SIRM/c is 111.04 kAm-1 and S-ratio is 0.8. Based on results, magnetic mineralogy indicated that the bulk magnetic carrier is stable single domain (SSD) or pseudo single domain (PSD) grains of Fe-Ti oxides with minor iron sulphides such as pyrite, greigite and pyrrhotite. Petrography and rock magnetic studies suggest that the magnetic carriers are chiefly secondary in origin and the NRM is modified over time. en_US
dc.language.iso en en_US
dc.subject Rock magnetic signatures, Dalma formation, Singhbhum mobile belt, Eastern India en_US
dc.title Rock magnetic signatures of the dalma Formation in the Singhbhum mobile belt, Eastern India en_US
dc.type Article en_US


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