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  5. High resolution aeromagnetic anomaly map of Mount Etna volcano, Southern Italy
 
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High resolution aeromagnetic anomaly map of Mount Etna volcano, Southern Italy

Author(s)
D'Ajello Caracciolo, F.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Nicolosi, I.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Carluccio, R.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Chiappini, S.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
De Ritis, R.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Giuntini, A.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Materni, V.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Messina, A.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Chiappini, M.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Language
English
Obiettivo Specifico
7A. Geofisica di esplorazione
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Journal of volcanology and geothermal research  
Issue/vol(year)
/277 (2014)
ISSN
0377-0273
Electronic ISSN
1872-6097
Publisher
Elsevier Science Limited
Pages (printed)
36-40
Date Issued
April 5, 2014
DOI
10.1016/j.jvolgeores.2014.03.008
URI
https://www.earth-prints.org/handle/2122/9017
Subjects
04. Solid Earth::04.05. Geomagnetism::04.05.04. Magnetic anomalies  
Subjects

Etna volcano

Magnetic anomalies

Aeromagnetism

potential fields

Fry analysis

Abstract
A high resolution aeromagnetic survey of Mount Etna Volcano was carried out by the Airborne Geophysics Science Team of Istituto Nazionale di Geofisica e Vulcanologia (INGV), aimed at producing the most detailed magnetic anomaly map existing so far for this area. Two datasets of the total intensity of the Earth's Magnetic Field were collected at different altitudes to take into account the huge topographic variations of Etna volcano, that reaches elevations above 3300 m asl. One level was flown at the altitude of 2200 m whereas a second one over the central part, at about 3500 m of altitude. Since the region is characterized by a large presence of strongly magnetized volcanic products, the survey was carried out acquiring profile lines only, in order to optimize the resources. From the residual magnetic anomaly analysis we inferred two main trending lineaments (− 35°N and 0°N) that are related to regional tectonic stress field and we interpret the main magnetic anomaly as the effect of thickness variation of magnetized volcanic products due to the complex pre-volcanic basement morphology of Etna.
Type
article
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D'AjelloCaracciolo2014.pdf

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1.88 MB

Format

Adobe PDF

Checksum (MD5)

499ecc0f46688c2204e4ccc08f718935

rome library|catania library|milano library|napoli library|pisa library|palermo library
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