Zobrazeno 1 - 10
of 105
pro vyhledávání: '"Luigi FERRANTI"'
Autor:
Giusy Lavecchia, Simone Bello, Carlo Andrenacci, Daniele Cirillo, Federico Pietrolungo, Donato Talone, Federica Ferrarini, Rita de Nardis, Paolo Galli, Joanna Faure Walker, Claudia Sgambato, Marco Menichetti, Carmelo Monaco, Salvatore Gambino, Giorgio De Guidi, Giovanni Barreca, Francesco Carnemolla, Fabio Brighenti, Salvatore Giuffrida, Claudia Pirrotta, Filippo Carboni, Luigi Ferranti, Luisa Valoroso, Giovanni Toscani, Massimiliano R. Barchi, Gerald Roberts, Francesco Brozzetti
Publikováno v:
Scientific Data, Vol 11, Iss 1, Pp 1-14 (2024)
Abstract QUIN database integrates and organizes structural-geological information from published and unpublished sources to constrain deformation in seismotectonic studies. The initial release, QUIN1.0, comprised 3,339 Fault Striation Pairs, mapped o
Externí odkaz:
https://doaj.org/article/3de0d7fdd42c4e50a7196e773078d3c0
Publikováno v:
Journal of Maps, Vol 13, Iss 2, Pp 227-238 (2017)
By using images acquired by the Mercury dual imaging system (MDIS) on-board the MESSENGER spacecraft during 2008–2015 and available DTMs, a new 1:3,000,000-scale geological map of the Shakespeare quadrangle of Mercury has been compiled. The quadran
Externí odkaz:
https://doaj.org/article/820e5996b5f84218ac44409879442d52
Geological cartography and structural analysis are essential for understanding Mercury’s geological history and tectonic processes. This work focuses on the Michelangelo quadrangle (H-12), located at latitudes 22.5°S-65°S and longitudes 180°E-27
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::94e17cab62dcd5a1a5324bfc03242813
https://doi.org/10.5194/egusphere-egu23-5378
https://doi.org/10.5194/egusphere-egu23-5378
Tolstoj quadrangle is located in the equatorial area of Mercury, between 22.5°N and 22.5°S of latitude and 144° and 216°E of latitude. In this work we present the preliminary results of a geological map (1:3M scale). The main basemap used for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::27c828a9b394366da83b6eac300ac27d
https://doi.org/10.5194/egusphere-egu23-12945
https://doi.org/10.5194/egusphere-egu23-12945
Introduction: The Michelangelo quadrangle of Mercury (H-12) encompasses the area between latitudes 22.5°S-65°S and longitudes 180°E-270°E. The first geological map of the H-12 quadrangle was produced by [1] at 1:5M scale using Mariner 10 data. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6afdf204d9c2e0d608aa808122d9559c
https://doi.org/10.5194/epsc2022-811
https://doi.org/10.5194/epsc2022-811
Gas leakage from deep geologic storage formations to the Earth’s surface is one of the main hazards in geological carbon sequestration and storage. Permeable sediment covers or natural and artificial pathways, such as faults and well structures, ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ebc0cdf1772d0db1d3ebb9e3c3ea26fc
https://doi.org/10.5194/egusphere-egu22-2440
https://doi.org/10.5194/egusphere-egu22-2440
Autor:
Jacopo Natale, Luigi Ferranti, Roberto Isaia, Camilla Marino, Marco Sacchi, Volkhard Spiess, Lena Steinmann, Stefano Vitale
Silicic calderas are volcanic systems whose unrest evolution is more unpredictable than other volcano types because they often do not culminate in an eruption. Their complex structure strongly influences the post-collapse volcano-tectonic evolution,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8c9c8a3aa24610783c9e5ce2403ef6d
http://hdl.handle.net/11588/876504
http://hdl.handle.net/11588/876504
Autor:
Jacopo Natale, Giovanni Camanni, Luigi Ferranti, Roberto Isaia, Marco Sacchi, Volkhard Spiess, Lena Steinmann, Stefano Vitale
Publikováno v:
Journal of Structural Geology. 163:104723
The structure of a caldera may influence its activity, making its understanding crucial for hazard assessment. Here, we analysed high-resolution seismic profiles in the Campi Flegrei (southern Italy) offshore sector. We recognized two main fault syst
Autor:
Luigi Ferranti, Gianluca Quarta, Paolo Orrù, Giovanni Scicchitano, Paolo Stocchi, Lucio Calcagnile, Fabrizio Antonioli, Marco Taviani, Giuseppe Mastronuzzi, Giovanni Scardino, Fabrizio Pepe, Carmelo Monaco
Publikováno v:
Water, Vol 13, Iss 2647, p 2647 (2021)
Water (Basel) 13 (2021). doi:10.3390/w13192647
info:cnr-pdr/source/autori:Antonioli F.; Calcagnile L.; Ferranti L.; Mastronuzzi G.; Monaco C.; Orru P.; Quarta G.; Pepe F.; Scardino G.; Scicchitano G.; Stocchi P.; Taviani M./titolo:New evidence of mis 3 relative sea level changes from the messina strait, Calabria (Italy)/doi:10.3390%2Fw13192647/rivista:Water (Basel)/anno:2021/pagina_da:/pagina_a:/intervallo_pagine:/volume:13
Water
Volume 13
Issue 19
Water (Basel) 13 (2021). doi:10.3390/w13192647
info:cnr-pdr/source/autori:Antonioli F.; Calcagnile L.; Ferranti L.; Mastronuzzi G.; Monaco C.; Orru P.; Quarta G.; Pepe F.; Scardino G.; Scicchitano G.; Stocchi P.; Taviani M./titolo:New evidence of mis 3 relative sea level changes from the messina strait, Calabria (Italy)/doi:10.3390%2Fw13192647/rivista:Water (Basel)/anno:2021/pagina_da:/pagina_a:/intervallo_pagine:/volume:13
Water
Volume 13
Issue 19
Investigation of sea-level positions during the highly-dynamic Marine Isotope Stage 3 (MIS 3: 29–61 kyrs BP) proves difficult because: (i) in stable and subsiding areas, coeval coastal sediments are currently submerged at depths of few to several t