2002
DOI: 10.1016/s0377-0273(01)00300-6
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Volcanological and petrological evolution of Marsili Seamount (southern Tyrrhenian Sea)

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Cited by 58 publications
(54 citation statements)
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“…Basaltic to rhyolitic lavas, dredged from the eastern and western seamounts, mostly belong to calc-alkaline and shoshonitic series, with compositional characteristics similar to the subaerial rocks of the Aeolian Islands. Mainly calc-alkaline rocks have been dredged at the Marsili volcano, sited in the central part of the Marsili backarc basin on a basaltic oceanic crust of 1.9-1.7 Ma (Trua et al, 2002, and references therein). Island-arc tholeiitic basalts have been only dredged from north Lametini and lowermost Aeolian slope.…”
Section: Introductionmentioning
confidence: 99%
“…Basaltic to rhyolitic lavas, dredged from the eastern and western seamounts, mostly belong to calc-alkaline and shoshonitic series, with compositional characteristics similar to the subaerial rocks of the Aeolian Islands. Mainly calc-alkaline rocks have been dredged at the Marsili volcano, sited in the central part of the Marsili backarc basin on a basaltic oceanic crust of 1.9-1.7 Ma (Trua et al, 2002, and references therein). Island-arc tholeiitic basalts have been only dredged from north Lametini and lowermost Aeolian slope.…”
Section: Introductionmentioning
confidence: 99%
“…Marsili seamount is a recent volcanic structure (1-0.1 Ma), mainly composed of basalts and, to a lesser extent, andesites and trachy-andesites with calc-alkaline affinity [32][33][34]. This structure has been interpreted as an inflated, small-scale spreading centre, since bio-and magneto-stratigraphic data show features comparable to those typical of mid-ocean ridges [35][36][37][38].…”
Section: Geothermal Potential Of Southern Tyrrhenian Basin and Marsilmentioning
confidence: 99%
“…The causes of the formation of the nearly 1500 km 3 structure have been deduced by its morphology and have been identified with the intense magma pulses originated from the subducted Ionian slab melting occurred about 0.7 My ago [9]. The basalt lava rocks composing the edifice belong mainly to the calc-alkaline and to the tholeitic magma series which, due to the quick cooling process after eruption, are characterised by a high degree of fracturing and vesicularity [10]. The submarine volcanic structure gets the maximum of heat anomaly flow of the whole Tyrrhenian Sea with values close to 250 mW/m 2 [3], but recent measurements report values up to 500 mW/m 2 within the crest's summit [11].…”
Section: -South Tyrrhenian Basin and Marsili Seamount Geophysicsmentioning
confidence: 99%