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Sabatini District

The Sabatini Volcanic District developed between about 0.8-0.6 Ma and 40 ka over a wide area located just to the north of Rome. Volcanism was predominantly explosive and generated widespread pyroclastic deposits with only minor lava flows, which were emitted from a large number of centres including several calderas (e.g. De Rita et al. 1983, 1993). The vol-canism occurred along a zone of crosscutting NW-SE and NE-SW faults (Di Filippo 1993). The Sabatini rocks rest over the same type of sedimentary bedrocks as at Vico, as well over the acid volcanics of Tolfa-Manziana-Cerite complex of the Tuscany Province. [Pg.86]


Fig. 4.14. Schematic geological map of Sabatini district. Simplified after Conti-celli et al. (1997). Numbers indicate various activity phases. Vertically mled areas west of the Bracciano Lake are Tolfa-Manziana-Cerite outcrops. Fig. 4.14. Schematic geological map of Sabatini district. Simplified after Conti-celli et al. (1997). Numbers indicate various activity phases. Vertically mled areas west of the Bracciano Lake are Tolfa-Manziana-Cerite outcrops.
Conticelli S., Francalianci L., Manetti P., Cioni R., and Sbrana A. (1997) Petrology and geochemistry of the ultrapotassic rocks from the Sabatini volcanic district, central Italy the role of evolutionary process in the genesis... [Pg.1382]


See other pages where Sabatini District is mentioned: [Pg.86]    [Pg.87]    [Pg.87]    [Pg.89]    [Pg.86]    [Pg.87]    [Pg.87]    [Pg.89]    [Pg.333]    [Pg.1366]   


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District

Sabatini

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