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Sabatini volcanic field

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Series: GSA Special Papers
Published: 01 January 2006
DOI: 10.1130/2006.2408(06)
...RECENT GEOLOGICAL EVOLUTION OF THE ROMAN REGION The Roman territorial framework is mostly the product of recent geodynamic processes affecting the western Mediterranean area. Rome's foundations are mostly the products of the Quaternary explosive eruptions in two volcanic fields, the Sabatini...
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(A) Age of <span class="search-highlight">volcanic</span> activity for Albani Hills <span class="search-highlight">Volcanic</span> District (AHVD), Mou...
Published: 01 December 2011
Figure 6. (A) Age of volcanic activity for Albani Hills Volcanic District (AHVD), Mount Sabatini Volcanic District (MSVD), Phlegrean Fields (PF), and Mount Etna (Et) plotted on the sea-level curve of the past 1 m.y. (from Bintanja et al., 2005 ); red dashed lines indicate glacial maximum. (B
Journal Article
Journal: GSA Bulletin
Published: 01 March 2013
GSA Bulletin (2013) 125 (3-4): 556–577.
... of Latium, consisting of Vulsini, Vico, Monti Sabatini, and the Alban Hills, plus Roccamonfina. The angular coefficient of the parting line between the fields for lava flows of these two volcanic regions corresponds to a Nb/Zr ratio of ∼0.10, which represents a lower limit for the lava flows...
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Journal Article
Published: 01 April 2020
Earth Sciences History (2020) 39 (1): 28–63.
... of the Geological Committee of Italy carried out field surveys and produced modern, albeit low resolution geological maps of Monte Amiata volcanics ( Verri 1877 , 1878 , 1889 , 1903a ; Lotti 1878 , 1901 , 1910 , 1933 ; Sabatini 1899 , 1910 , 1911 , 1912 ). Prior to the early decades of the twentieth...
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Location map of the three study areas and of successive figures; catchment ...
Published: 01 December 2011
://srtm.csi.cgiar.org/ ). Green lines indicate the shelf break; light red areas indicate the main volcanic areas: MSVD—Mount Sabatini Volcanic District, AHVD—Albani Hills Volcanic District, RVC—Roccamonfina Volcanic Complex, PF—Phlegrean Fields, So-Ve—Somma-Vesuvius. Contour interval is 100 m, bold isobaths every 500 m.
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Zr/Y versus Nb/Y (A) and Th/Ta versus Nb/Zr (B) compositions of lava flows ...
Published: 01 March 2013
by a straight line (oblique dashed line in part A) from those of Latium, consisting of Vulsini, Vico, Monti Sabatini, and the Alban Hills, plus Roccamonfina. The angular coefficient of the parting line between the fields for lava flows of these two volcanic regions corresponds to a Nb/Zr ratio of ∼0.10, which
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Compositional <span class="search-highlight">fields</span> based on Zr&#x2F;Y versus Nb&#x2F;Y (A) and Th&#x2F;Ta versus Nb&#x2F;Zr (...
Published: 01 March 2013
of the Monti Sabatini (MS) Volcanic District ( Marra et al., 2011 , and references therein); (4) the Brown Leucitic Tuff and the White Trachytic Tuff pumices (RM) ( Luhr and Giannetti, 1987 ; Giannetti and Luhr, 1983 ); and (5) the average compositions for the Campanian volcanic products (CA), including lava
Journal Article
Published: 01 October 2016
Journal of Sedimentary Research (2016) 86 (10): 1208–1227.
... show that tectonism during middle–upper Pleistocene volcanic activity in the Sabatini, Cimini, and Vulsini volcanic complexes played a major role controlling stream-network reorganization in the Tiber drainage basin and resulted in enhanced volcaniclastic input from ash fall and recycling...
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Journal Article
Published: 01 June 2014
Italian Journal of Geosciences (2014) 133 (2): 169–186.
... crystal 40 Ar/ 39 Ar dating was performed yielding an age of 514±16 ka. Pollen analyses revealed the occurrence of warm and humid interglacial conditions that were correlated to MIS 13 on the basis of the age determination. The chemical compositions of glasses indicate that the Sabatinian volcanic field...
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Series: GSA Special Papers
Published: 01 January 2006
DOI: 10.1130/2006.2408(4.2)
... Albani ( Watkins et al., 2002 ) and the “Tufo Rosso a Scorie Nere” from the Sabatini volcanic field. Zeolitized ignimbrites can be local aquifers if they develop a good fracture network. The alteration of volcanic glass to halloysite may reduce the primary porosity of pyroclastic deposits, filling up...
Journal Article
Published: 01 December 2014
European Journal of Mineralogy (2014) 26 (6): 743–756.
... of the crystallization pressure of the OBI and the Roman Province literature clinopyroxenes can be outlined. Indeed, all the data fall in the low-pressure volcanic field at similar pressure value, and the differences among the Orvieto-Bagnoregio, Sabatini, the Alban Hills and Selva del Lamone - Commenda clinopyroxenes...
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Journal Article
Journal: Geosphere
Published: 01 December 2011
Geosphere (2011) 7 (6): 1284–1293.
...Figure 6. (A) Age of volcanic activity for Albani Hills Volcanic District (AHVD), Mount Sabatini Volcanic District (MSVD), Phlegrean Fields (PF), and Mount Etna (Et) plotted on the sea-level curve of the past 1 m.y. (from Bintanja et al., 2005 ); red dashed lines indicate glacial maximum. (B...
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Journal Article
Journal: Geology
Published: 01 March 2013
Geology (2013) 41 (3): 375–378.
... to the volcanic activity that has affected the coastal region of Latium since 500 ka (e.g., Cavinato et al., 1992 ; Karner et al., 2001 ). The overall picture highlights the likely presence of a crustal thermal bulge supposedly centered on the Sabatini Mounts volcanic complex ( Figs. 2 and 3...
FIGURES
Journal Article
Published: 01 January 2003
European Journal of Mineralogy (2003) 15 (1): 207–215.
... field crossed by the 2.5:1 line. Fig. 2. Diagram regarding hourglass catilli. Height/diameter ratio against height/width ratio of mount. Closed circles: millstones from Vesuvio: closed triangles: millstones from Orvieto. The volcanic rocks of the studied millstones can be grouped...
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Journal Article
Published: 01 April 2002
Mineralogical Magazine (2002) 66 (2): 287–299.
... quoted from the literature, we use the name given in the original paper, whether or not identification has been confirmed by XRD. The Greater Olkaria Volcanic Complex ( Clarke et al. , 1990 ) is a multicentred Quaternary volcanic field near Lake Naivasha (0°45′ S, 36°21′ E), in the south-central...
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Journal Article
Published: 01 December 2006
The Canadian Mineralogist (2006) 44 (6): 1367–1378.
... and PR-up, Table 1 ) were collected from the “upper pyroclastic flow” of the Sacrofano caldera in the Sabatini volcanic group ( De Rita et al . 1983 ). These samples, classified as “type-A holocrystalline ejecta”, were originally described by Della Ventura et al . (1992) . They are composed of K...
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Journal Article
Published: 01 October 2012
Italian Journal of Geosciences (2012) 131 (3): 389–402.
... mantling the epikarst surface of L’Aquila Breccia of picture C (S. Antonio site); this tephra can be assigned to the Ancient-Early activity of the Sabatini Volcanic District (0.4–0.8 Ma; S ottili et alii , 2004 ; 2010 ), so dating, as upper limit, the middle Pleistocene; E ) gravel of alluvial Vetoio...
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Journal Article
Published: 30 October 2018
Journal of Sedimentary Research (2018) 88 (10): 1238–1259.
... in the upstream Tiber river drainage basin, which has an area of 6077 km 2 . The downstream Tiber drainage basin, with area 5343 km 2 , exposes Oligocene to Pliocene fine-grained marine sediments, Jurassic to Miocene carbonate successions, and Plio-Pleistocene volcanic units of the Vulsini, Vico, Sabatini...
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Journal Article
Published: 01 January 2002
European Journal of Mineralogy (2002) 14 (1): 175–183.
.... Cenciaioli, pers.comm.; Santi et al. , in prep.) near the ancient Roman village of Otriculum along the River Tiber (Otricoli, Terni). The leucite phonolites from the Sabatini Volcanic District ( Conticelli et al. , 1997 ) and from Roccamonfina volcano ( Appleton, 1972 ) are incompatible as sources...
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Journal Article
Published: 02 December 2014
Bulletin of the Seismological Society of America (2015) 105 (1): 1–13.
... to halfway through the second century A.D. Online Material: Table of major‐element compositions, field photos, and Harker diagrams. MT1: Glass composition matches the tephra from the caldera‐forming Neapolitan Yellow Tuff eruption that occurred in the 160 km distant Campi Flegrei volcanic field. Its age...
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