Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis

Wilkes Basin lies to the east of the Transantarctic Mountains. The origin of this sub-glacial basin is still controversial. Flexural uplift of the Transantarctic Mountains has been suggested as the geophysical process which generated the basin (Stern & ien Brink, 1989). Other studies proposed a...

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Main Authors: Piana Agostinetti, N., Roselli, P., Cattaneo, M., Amato, A.
Other Authors: Piana Agostinetti, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia, Roselli, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia, Cattaneo, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia, Amato, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia, Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia, Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Format: Other/Unknown Material
Language:English
Published: 2005
Subjects:
Online Access:http://hdl.handle.net/2122/3199
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spelling ftingv:oai:www.earth-prints.org:2122/3199 2023-05-15T13:51:39+02:00 Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis Piana Agostinetti, N. Roselli, P. Cattaneo, M. Amato, A. Piana Agostinetti, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia Roselli, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia Cattaneo, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia Amato, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia 2005-10 http://hdl.handle.net/2122/3199 en eng IASPEI-General Assembly http://hdl.handle.net/2122/3199 open receiver functios Antarctica 01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics Poster session 2005 ftingv 2022-07-29T06:04:42Z Wilkes Basin lies to the east of the Transantarctic Mountains. The origin of this sub-glacial basin is still controversial. Flexural uplift of the Transantarctic Mountains has been suggested as the geophysical process which generated the basin (Stern & ien Brink, 1989). Other studies proposed a continental rift structure for this region (Ferraccioli et al., 2001). The two models differ mainly in the crustal structure predicted beneath the basin. In the former, crustal thickning is expected to be originated from the high rigidity of the East Antarctic Craton lithosphere. Otherwise, the rift structure hypothesis is consistent with a broad crustal thinning. During the WIBEM 2003 campaign, we deployed five broadband seismic stations across the basin. We selected high signal/noise teleseismic recording to compute a data-set of receiver functions. We applied a classical inversion scheme, the Neighbourhood Algorithm, to our data-set. Here, two different and complementary studies are presented. We constrain the Moho geometry beneath the Wilkes Basin from the analysis of low-frequency P-to-S conversion at the base of the crust. Also, we investigate the nature of the basin mapping the presence of subglacial sediments using the P-to-S conversion at the ice-bedrock interface. Published Chile 3.3. Geodinamica e struttura dell'interno della Terra open Other/Unknown Material Antarc* Antarctic Antarctica Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Antarctic Transantarctic Mountains
institution Open Polar
collection Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia)
op_collection_id ftingv
language English
topic receiver functios
Antarctica
01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics
spellingShingle receiver functios
Antarctica
01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics
Piana Agostinetti, N.
Roselli, P.
Cattaneo, M.
Amato, A.
Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
topic_facet receiver functios
Antarctica
01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics
description Wilkes Basin lies to the east of the Transantarctic Mountains. The origin of this sub-glacial basin is still controversial. Flexural uplift of the Transantarctic Mountains has been suggested as the geophysical process which generated the basin (Stern & ien Brink, 1989). Other studies proposed a continental rift structure for this region (Ferraccioli et al., 2001). The two models differ mainly in the crustal structure predicted beneath the basin. In the former, crustal thickning is expected to be originated from the high rigidity of the East Antarctic Craton lithosphere. Otherwise, the rift structure hypothesis is consistent with a broad crustal thinning. During the WIBEM 2003 campaign, we deployed five broadband seismic stations across the basin. We selected high signal/noise teleseismic recording to compute a data-set of receiver functions. We applied a classical inversion scheme, the Neighbourhood Algorithm, to our data-set. Here, two different and complementary studies are presented. We constrain the Moho geometry beneath the Wilkes Basin from the analysis of low-frequency P-to-S conversion at the base of the crust. Also, we investigate the nature of the basin mapping the presence of subglacial sediments using the P-to-S conversion at the ice-bedrock interface. Published Chile 3.3. Geodinamica e struttura dell'interno della Terra open
author2 Piana Agostinetti, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia
Roselli, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Cattaneo, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia
Amato, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
format Other/Unknown Material
author Piana Agostinetti, N.
Roselli, P.
Cattaneo, M.
Amato, A.
author_facet Piana Agostinetti, N.
Roselli, P.
Cattaneo, M.
Amato, A.
author_sort Piana Agostinetti, N.
title Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
title_short Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
title_full Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
title_fullStr Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
title_full_unstemmed Moho-depth and subglacial sedimentary layer thickness in the Wilkes Basin from Receiver Function Analysis
title_sort moho-depth and subglacial sedimentary layer thickness in the wilkes basin from receiver function analysis
publishDate 2005
url http://hdl.handle.net/2122/3199
geographic Antarctic
Transantarctic Mountains
geographic_facet Antarctic
Transantarctic Mountains
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_relation IASPEI-General Assembly
http://hdl.handle.net/2122/3199
op_rights open
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