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

Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/921

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DC Field	Value	Language
dc.contributor.author	Arif, Md.
dc.contributor.author	Basavaiah, N.
dc.contributor.author	Misra, S.
dc.date.accessioned	2016-08-25T06:59:37Z
dc.date.accessioned	2021-02-12T09:45:43Z	-
dc.date.available	2016-08-25T06:59:37Z
dc.date.available	2021-02-12T09:45:43Z	-
dc.date.issued	2012
dc.identifier.citation	European Planetary Science Congress 2012, v.7, EPSC2012-163, 2012	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/921	-
dc.description.abstract	The 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.language.iso	en	en_US
dc.subject	Lonar crater ejecta	en_US
dc.subject	Palaeomagnetic properties	en_US
dc.subject	Rock	en_US
dc.title	Rock and palaeomagnetic properties of randomly oriented basaltic blocks from lonar crater ejecta, India	en_US
dc.type	Article	en_US
dc.identifier.accession	091240
Appears in Collections:	UAS_Reprints

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