Thermochemical plumes form at the base of the lower mantle as a consequence of heat flow from the outer core and the presence of local chemical doping that decreases the melting temperature. Theoretical and experimental modelling of thermochemical plumes show that the diameter of a plume conduit remains practically constant during plume ascent. However, when the top of a plume reaches a refractory layer, whose melting temperature is higher than the melt temperature in the plume conduit, a mushroom-shaped plume head develops. Main parameters (melt viscosity, ascent time, ascent velocity, temperature differences in the plume conduit, and thermal power) are presented for a thermochemical plume ascending from the core-mantle boundary. In addition, the following relationships are developed: the pressure distribution in the plume conduit during the ascent of a plume, conditions for eruption-conduit formation, the effect of the P-T conditions and controls on the shape and size of a plume top, heat transfer between a thermochemical plume and the lithosphere (when the plume reaches the bottom of a refractory layer in the lithosphere), and eruption volume versus the time interval t(1) between plume formation and eruption. These relationships are used to determine thermal power and time t(1) for the Tunguska syneclise and the Siberian traps as a whole. The Siberian and other trap provinces are characterized by giant volumes of lavas and sills formed a very short time period. Data permit a model for superplumes with three stages of formation: early (variable picrites and alkali basalts), main (tholeiite plateau basalts), and final (ultrabasic and alkaline lavas and intrusions). These stages reflect the evolution of a superplume from the ascent of one or several independent plumes, through the formation of thick lenses of mantle melts underplating the lithosphere and, finally, intrusion and extrusion of differentiated mantle melts. Synchronous syenite-granite intrusions and bimodal volcanism abundant in the margins of the Siberian traps are the result of melting of the lower crust at depths of 65-70 km under the effect of plume melts. (c) 2007 Published by Elsevier B.V.
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Nanjing Univ, Dept Earth Sci, State Key Lab Mineral Deposits Res, Nanjing 210046, Jiangsu, Peoples R ChinaNanjing Univ, Dept Earth Sci, State Key Lab Mineral Deposits Res, Nanjing 210046, Jiangsu, Peoples R China
Wang, Qin
Bagdassarov, N.
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Goethe Univ Frankfurt, Inst Geosci, D-60438 Frankfurt, GermanyNanjing Univ, Dept Earth Sci, State Key Lab Mineral Deposits Res, Nanjing 210046, Jiangsu, Peoples R China
Bagdassarov, N.
Shatsky, V. S.
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Russian Acad Sci, Ap Vinogradov Geochem Inst, Siberian Branch, Ul Favorskogo 1A, Irkutsk 664033, Russia
Russian Acad Sci, Siberian Branch, VS Sobolev Inst Geol & Mineral, Pr Akad Koptyuga 3, Novosibirsk 630090, Russia
Novosibirsk State Univ, Ul Pirogova 2, Novosibirsk 630090, RussiaNanjing Univ, Dept Earth Sci, State Key Lab Mineral Deposits Res, Nanjing 210046, Jiangsu, Peoples R China