Andrea Di Giulio

Prof. Andrea Di Giulio

orcid

Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 March 2019 in Earth-Science Reviews
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Journal Article
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PSPietro Sternai
Pietro Sternai
CSChristian Sue
Christian Sue
LHLaurent Husson
Laurent Husson
ESEnrico Serpelloni
Enrico Serpelloni
TBThorsten W. Becker
Thorsten W. Becker
SCSébastien Castelltort
Sébastien Castelltort

1 June 2015 in Geology
Verified
Journal Article
Closed access
MMMatteo Maino
Matteo Maino
LCLeonardo Casini
Leonardo Casini
ACAndrea Ceriani
Andrea Ceriani
ADAlessandro Decarlis
Alessandro Decarlis
AGAndrea Di Giulio
Andrea Di Giulio
FSFinlay M. Stuart
Finlay M. Stuart

25 January 2011 in Sedimentology
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Journal Article
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PRPaola Ronchi
Paola Ronchi
FJFlavio Jadoul
Flavio Jadoul
ACAndrea Ceriani
Andrea Ceriani
AGAndrea Di Giulio
Andrea Di Giulio
PSPaolo Scotti
Paolo Scotti
EMElisabetta Previde Massara
Elisabetta Previde Massara

1 August 2001 in International Journal of Earth Sciences
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Journal Article
Closed access
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AGAndrea Di Giulio
Andrea Di Giulio
BCBarbara Carrapa
Barbara Carrapa
RFRoberto Fantoni
Roberto Fantoni
LGLuciano Gorla
Luciano Gorla
AVAntonio Valdisturlo
Antonio Valdisturlo

1 October 2014 in Tectonophysics
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Journal Article
Closed access
GTGiovanni Toscani
Giovanni Toscani
LBLorenzo Bonini
Lorenzo Bonini
MAMohammad Irfan Ahmad
Mohammad Irfan Ahmad
DBDaniela Di Bucci
Daniela Di Bucci
AGAndrea Di Giulio
Andrea Di Giulio
CGCarla Galuppo
Carla Galuppo

1 July 2001 in Journal of Sedimentary Research
Verified
Journal Article
Closed access
IDI. Dunkl
I. Dunkl
AGAndrea Di Giulio
Andrea Di Giulio
JKJ. Kuhlemann
J. Kuhlemann
Fission track (FT) analyses on unannealed detrital minerals provide a powerful tool both for refining provenance models derived from traditional methods and for collecting information about erosion rates of the source area. Their power is increased if they are coupled with the study of zircon morphology. This combination of methods is applied to the Chattian-Aquitanian (25-23 Ma) Macigno turbidite complex. Basin-fill patterns and petrographical studies consistently identify the uplifting western Central Alps as the main source region for the Macigno Formation. Most zircon grains fall into a young age cluster (∼ 40-30 Ma), derived from a rapidly exhuming crystalline source region with a high cooling rate. Within this cluster, two age subgroups can be distinguished at 30 and 40 Ma. In the younger subgroup, the zircon morphology supports the presence of two main populations: (1) from igneous rocks (S-type euhedral zircons), which appear to be partly derived from airborne tuffs; and (2) from metasedimentary units. In huge volumes of these metamorphic rocks, mica Ar-Ar and zircon fission-track thermochronometers have been reset, because of high geothermal gradients in the vicinity of the Periadriatic intrusives in mid-Oligocene times. At the present surface of the Alps, zircon FT ages around and slightly less than 30 Ma are reported in the Sesia-Lanzo zone, the Gran Paradiso Massif, the Upper Pennine nappes, the Monte Rosa Massif, and the Dent Blanche complex. The older subgroup of the Tertiary zircons (40 Ma) may have been supplied by metamorphic and migmatitic rocks affected by an Eocene high-temperature phase. A Late Cretaceous age cluster (∼ 70-60 Ma) is related to cooling after the main Austroalpine metamorphic event at 110-100 Ma. Most of the recently exposed Austroalpine nappe complex displays mica cooling ages and zircon FT ages between 95-70 Ma and 99-55 Ma, respectively. Finally, an ill-defined Jurassic age cluster, with a mean in Late Jurassic times, is related to rift-shoulder heating of the Austroalpine/South-Alpine crystalline basement due to rifting of the Pennine oceanic domain. Presently, the Silvretta nappe complex, situated at the western termination of the Austroalpine realm, and the South-Alpine basement west of the Canavese Line, display similar zircon FT ages. Therefore, a westward continuation of the Silvretta complex prior to deep Neogene erosion is suggested.