New geophysical views of Mt. Melbourne Volcano (East Antarctica)

AB: Mt. Melbourne volcano is located along the transition between the Transantarctic Mountains and the West Antarctic Rift System. Recent volcanic activity is suggested by the occurrence of blankets of pyroclastic pumice and scoria fall around the eastern and southern flanks of Mt Melbourne and by p...

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Main Authors: ARMADILLO, EGIDIO, BOZZO, EMANUELE, M. GAMBETTA, F. FERRACCIOLI, H. CORR
Other Authors: Armadillo, Egidio, M., Gambetta, F., Ferraccioli, H., Corr, Bozzo, Emanuele
Format: Conference Object
Language:English
Published: 2009
Subjects:
Online Access:http://hdl.handle.net/11567/241472
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spelling ftunivgenova:oai:iris.unige.it:11567/241472 2024-02-11T09:56:24+01:00 New geophysical views of Mt. Melbourne Volcano (East Antarctica) ARMADILLO, EGIDIO BOZZO, EMANUELE M. GAMBETTA F. FERRACCIOLI H. CORR Armadillo, Egidio M., Gambetta F., Ferraccioli H., Corr Bozzo, Emanuele 2009 ELETTRONICO http://hdl.handle.net/11567/241472 eng eng ispartofbook:Canadian Geophysical Union, Spring Meeting 2009 Canadian Geophysical Union, Spring Meeting 2009 firstpage:1 lastpage:1 http://hdl.handle.net/11567/241472 info:eu-repo/semantics/conferenceObject 2009 ftunivgenova 2024-01-17T17:35:39Z AB: Mt. Melbourne volcano is located along the transition between the Transantarctic Mountains and the West Antarctic Rift System. Recent volcanic activity is suggested by the occurrence of blankets of pyroclastic pumice and scoria fall around the eastern and southern flanks of Mt Melbourne and by pyroclastic layers interbedded with the summit snows. Geothermal activity in the crater area of Mount Melbourne may be linked to the intrusion of dykes within the last 200 years. Geophysical networks suggest that Mount Melbourne is a quiescent volcano, possibly characterised by slow internal dynamics. During the 2002-2003 Italian Antarctic campaign a high-resolution aeromagnetic survey was performed within the TIMM (Tectonics and Interior of Mt. Melbourne area) project. This helicopter-borne survey was flown at low-altitude and in drape-mode configuration (305 m above terrain) with a line separation less than 500 m. Our new high-resolution magnetic maps reveal the largely ice-covered magmatic and tectonic patters in the Mt. Melbourne volcano area. Additionally, in the frame of the UK-Italian ISODYN-WISE project (2005-06), an airborne ice-sounding radar survey was flown. We combine the sub-ice topography with images and models of the interior of Mt. Melbourne volcano, as derived from the high resolution aeromagnetic data and land gravity data. Our new geophysical maps and models also provide a new tool to study the regional setting of the volcano. In particular we re-assess whether there is geophysical evidence for coupling between strike-slip faulting, the Terror Rift, and Mount Melbourne volcano. Conference Object Antarc* Antarctic Antarctica East Antarctica Università degli Studi di Genova: CINECA IRIS Antarctic East Antarctica Transantarctic Mountains Mount Melbourne ENVELOPE(164.700,164.700,-74.350,-74.350)
institution Open Polar
collection Università degli Studi di Genova: CINECA IRIS
op_collection_id ftunivgenova
language English
description AB: Mt. Melbourne volcano is located along the transition between the Transantarctic Mountains and the West Antarctic Rift System. Recent volcanic activity is suggested by the occurrence of blankets of pyroclastic pumice and scoria fall around the eastern and southern flanks of Mt Melbourne and by pyroclastic layers interbedded with the summit snows. Geothermal activity in the crater area of Mount Melbourne may be linked to the intrusion of dykes within the last 200 years. Geophysical networks suggest that Mount Melbourne is a quiescent volcano, possibly characterised by slow internal dynamics. During the 2002-2003 Italian Antarctic campaign a high-resolution aeromagnetic survey was performed within the TIMM (Tectonics and Interior of Mt. Melbourne area) project. This helicopter-borne survey was flown at low-altitude and in drape-mode configuration (305 m above terrain) with a line separation less than 500 m. Our new high-resolution magnetic maps reveal the largely ice-covered magmatic and tectonic patters in the Mt. Melbourne volcano area. Additionally, in the frame of the UK-Italian ISODYN-WISE project (2005-06), an airborne ice-sounding radar survey was flown. We combine the sub-ice topography with images and models of the interior of Mt. Melbourne volcano, as derived from the high resolution aeromagnetic data and land gravity data. Our new geophysical maps and models also provide a new tool to study the regional setting of the volcano. In particular we re-assess whether there is geophysical evidence for coupling between strike-slip faulting, the Terror Rift, and Mount Melbourne volcano.
author2 Armadillo, Egidio
M., Gambetta
F., Ferraccioli
H., Corr
Bozzo, Emanuele
format Conference Object
author ARMADILLO, EGIDIO
BOZZO, EMANUELE
M. GAMBETTA
F. FERRACCIOLI
H. CORR
spellingShingle ARMADILLO, EGIDIO
BOZZO, EMANUELE
M. GAMBETTA
F. FERRACCIOLI
H. CORR
New geophysical views of Mt. Melbourne Volcano (East Antarctica)
author_facet ARMADILLO, EGIDIO
BOZZO, EMANUELE
M. GAMBETTA
F. FERRACCIOLI
H. CORR
author_sort ARMADILLO, EGIDIO
title New geophysical views of Mt. Melbourne Volcano (East Antarctica)
title_short New geophysical views of Mt. Melbourne Volcano (East Antarctica)
title_full New geophysical views of Mt. Melbourne Volcano (East Antarctica)
title_fullStr New geophysical views of Mt. Melbourne Volcano (East Antarctica)
title_full_unstemmed New geophysical views of Mt. Melbourne Volcano (East Antarctica)
title_sort new geophysical views of mt. melbourne volcano (east antarctica)
publishDate 2009
url http://hdl.handle.net/11567/241472
long_lat ENVELOPE(164.700,164.700,-74.350,-74.350)
geographic Antarctic
East Antarctica
Transantarctic Mountains
Mount Melbourne
geographic_facet Antarctic
East Antarctica
Transantarctic Mountains
Mount Melbourne
genre Antarc*
Antarctic
Antarctica
East Antarctica
genre_facet Antarc*
Antarctic
Antarctica
East Antarctica
op_relation ispartofbook:Canadian Geophysical Union, Spring Meeting 2009
Canadian Geophysical Union, Spring Meeting 2009
firstpage:1
lastpage:1
http://hdl.handle.net/11567/241472
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