Rock and palaeomagnetic properties of randomly oriented basaltic blocks from lonar crater ejecta, India

dc.contributor.authorArif, Md.
dc.contributor.authorBasavaiah, N.
dc.contributor.authorMisra, S.
dc.date.accessioned2016-08-25T06:59:37Z
dc.date.accessioned2021-02-12T09:45:43Z
dc.date.available2016-08-25T06:59:37Z
dc.date.available2021-02-12T09:45:43Z
dc.date.issued2012
dc.description.abstractThe preliminary investigation of rock and palaeomagnetic properties of the basaltic blocks deposited within the continuous ejecta around the Lonar crater during impact shows that these ejecta basalts, in general, have low NRM/χ compared with the average unshocked basalt from the ESE of Lonar crater. These ejecta basalts also have low REM with few exceptions. The HC component of these ejecta basalts are random but showing a broad concentration around the average HC component of shocked basalts from around the crater rim suggesting influence of shock induced magnetic field beyond the modification stage of formation of the Lonar crater.en_US
dc.identifier.accession091240
dc.identifier.citationEuropean Planetary Science Congress 2012, v.7, EPSC2012-163, 2012en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/921
dc.language.isoenen_US
dc.subjectLonar crater ejectaen_US
dc.subjectPalaeomagnetic propertiesen_US
dc.subjectRocken_US
dc.titleRock and palaeomagnetic properties of randomly oriented basaltic blocks from lonar crater ejecta, Indiaen_US
dc.typeArticleen_US

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