Michela Giustiniani

Dr. Michela Giustiniani

Istituto Nazionale di Oceanografia e di Geofisica Sperimentale - OGS
orcid

Research Focus & Metrics

Academic Career Length

22Years (2005-Present)

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

Representative Publications

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22 April 2013 in Journal of the Geological Society
Verified
Journal Article
Closed access
RCRaimondo Catalano
Raimondo Catalano
VVVera Valenti
Vera Valenti
CACinzia Albanese
Cinzia Albanese
FAFlavio Accaino
Flavio Accaino
ASAttilio Sulli
Attilio Sulli
Michela GiustinianiMichela Giustiniani
Michela Giustiniani
Sicily is a thick orogenic wedge formed by (1) the foreland (African) and its Sicilian orogen and (2) the thick-skinned, Calabrian–Peloritani wedge. The crust under central Sicily, from the Tyrrhenian margin to the coastline of the Sicily Channel, has been investigated by the multidisciplinary (SI.RI.PRO.) research project. The project dealt with the nature and thickness of the crust and depth and geometry of the Moho, which is essential in formulating subduction models and improving the knowledge of African and Tyrrhenian–European lithospheres. The results resolve features such as (1) the main orogenic wedge, (2) the very steep, NW–SE-trending regional monocline suggesting inflection of the foreland crust, (3) the deep Caltanissetta synform imaged, for the first time, to about 25 km, and (4) the top of the crystalline basement and the inferred crust–mantle boundary. The SI.RI.PRO. transect confirmed that the NNW-dipping, autochthonous Iblean platform of SE Sicily and its basement extends all the way into central Sicily. Further NW, towards the NNW end of the transect, a large uplift involves the Iblean platform and its underlying basement. The associated gravity anomaly is interpreted as the southern wedge edge of the Tyrrhenian mantle that splits the subducting Iblean–Pelagian (African) continental slab from an overlying synformal stack of allochthonous thrust sheets. Supplementary materials: Additional data are available at www.geolsoc.org.uk/SUP18594 .

1 January 2020 in Marine and Petroleum Geology
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Journal Article
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TMTimothy A. Minshull
Timothy A. Minshull
HMHector Marin-Moreno
Hector Marin-Moreno
PBPeter Betlem
Peter Betlem
JBJoerg Bialas
Joerg Bialas
SBStefan Bünz
Stefan Bünz
Juan-Tomás VázquezJuan-Tomás Vázquez
Juan-Tomás Vázquez

1 July 2011 in Tectonophysics
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Journal Article
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FAFlavio Accaino
Flavio Accaino
RCRaimondo Catalano
Raimondo Catalano
LMLuigi Di Marzo
Luigi Di Marzo
Michela GiustinianiMichela Giustiniani
Michela Giustiniani
Umberta TinivellaUmberta Tinivella
Umberta Tinivella
PMPiero Manetti
Piero Manetti

24 March 2021 in Energies
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Journal Article
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AGAlberto Maria Gambelli
Alberto Maria Gambelli
Umberta TinivellaUmberta Tinivella
Umberta Tinivella
Rita GiovannettiRita Giovannetti
Rita Giovannetti
Beatrice CastellaniBeatrice Castellani
Beatrice Castellani
Michela GiustinianiMichela Giustiniani
Michela Giustiniani
FRFederico Rossi
Federico Rossi
Chemical composition in seawater of marine sediments, as well as the physical properties and chemical composition of soils, influence the phase behavior of natural gas hydrate by disturbing the hydrogen bond network in the water-rich phase before hydrate formation. In this article, some marine sediments samples, collected in National Antarctic Museum in Trieste, were analyzed and properties such as pH, conductivity, salinity, and concentration of main elements of water present in the sediments are reported. The results, obtained by inductively coupled plasma-mass spectrometry (ICP-MS) and ion chromatography (IC) analysis, show that the more abundant cation is sodium and, present in smaller quantities, but not negligible, are calcium, potassium, and magnesium, while the more abundant anion is chloride and sulfate is also appreciable. These results were successively used to determine the thermodynamic parameters and the effect on salinity of water on hydrates’ formation. Then, hydrate formation was experimentally tested using a small-scale apparatus, in the presence of two different porous media: a pure silica sand and a silica-based natural sand, coming from the Mediterranean seafloor. The results proved how the presence of further compounds, rather than silicon, as well as the heterogeneous grainsize and porosity, made this sand a weak thermodynamic and a strong kinetic inhibitor for the hydrate formation process.

1 January 2013 in Global and Planetary Change
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Journal Article
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Umberta TinivellaUmberta Tinivella
Umberta Tinivella
Michela GiustinianiMichela Giustiniani
Michela Giustiniani

1 September 2018 in Marine and Petroleum Geology
Verified
Journal Article
Closed access
DCDario Civile
Dario Civile
Emanuele LodoloEmanuele Lodolo
Emanuele Lodolo
FAFlavio Accaino
Flavio Accaino
RGRiccardo Geletti
Riccardo Geletti
MSMarcello Schiattarella
Marcello Schiattarella
LZLuigi Zampa
Luigi Zampa