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Experimental and theoretical modeling of diamondiferous plumes. / Kirdyashkin, A. G.; Kirdyashkin, A. A.; Distanov, V. E. et al.

In: Geodynamics and Tectonophysics, Vol. 10, No. 2, 01.01.2019, p. 247-263.

Research output: Contribution to journalArticlepeer-review

Harvard

Kirdyashkin, AG, Kirdyashkin, AA, Distanov, VE & Gladkov, IN 2019, 'Experimental and theoretical modeling of diamondiferous plumes', Geodynamics and Tectonophysics, vol. 10, no. 2, pp. 247-263. https://doi.org/10.5800/GT-2019-10-2-0413

APA

Kirdyashkin, A. G., Kirdyashkin, A. A., Distanov, V. E., & Gladkov, I. N. (2019). Experimental and theoretical modeling of diamondiferous plumes. Geodynamics and Tectonophysics, 10(2), 247-263. https://doi.org/10.5800/GT-2019-10-2-0413

Vancouver

Kirdyashkin AG, Kirdyashkin AA, Distanov VE, Gladkov IN. Experimental and theoretical modeling of diamondiferous plumes. Geodynamics and Tectonophysics. 2019 Jan 1;10(2):247-263. doi: 10.5800/GT-2019-10-2-0413

Author

Kirdyashkin, A. G. ; Kirdyashkin, A. A. ; Distanov, V. E. et al. / Experimental and theoretical modeling of diamondiferous plumes. In: Geodynamics and Tectonophysics. 2019 ; Vol. 10, No. 2. pp. 247-263.

BibTeX

@article{82af97804f4a4b159535e16cbb6862d3,
title = "Experimental and theoretical modeling of diamondiferous plumes",
abstract = "We consider thermochemical mantle plumes with thermal power 1.6·1010 W<N<2.7·1010 W (relative thermal power 1.15<Ka<1.9) as plumes with an intermediate thermal power. Such plumes are formed at the core–mantle boundary beneath cratons in the absence of horizontal free‐convection mantle flows beneath them, or in the presence of weak horizontal mantle flows. A proposed scheme of convection flows in the conduit of a plume with an intermediate thermal power is based on laboratory and theoretical modeling data. A plume ascends (melts out) from the core-mantle boundary to critical depth xкр from which magma erupts on the Earth{\textquoteright}s surface. The magmatic melt erupts from the plume conduit onto the surface through the eruption conduit. The latter forms under the effect of superlithostatic pressure on the plume roof. While the thickness of the block above the plume roof decreases to a critical value xкр, the shear stress on its cylindrical surface reaches a critical value (strength limit) τкр.Rock fails in the vicinity of the cylindrical block and, as a consequence, the eruption conduit is formed. We estimate the height of the eruption conduit and the time for the plume to ascent to the critical depth xкр. The volume of erupted melt is estimated for kinematic viscosity of melt v=0.5–2 м2/с. The depth Δx from which the melt is transported to the surface is determined. Using the eruption volume, we obtain a relationship between the depth Δx and the plume conduit diameter for the above‐mentioned kinematic viscosities. In the case that the depth Δx is larger than 150 km, the melt from the plume conduit can transport diamonds to the Earth{\textquoteright}s surface. Thus, the plumes with an intermediate thermal power are diamondiferous. The melt flow structure at the plume conduit/eruption conduit interface is determined on the basis of the laboratory modeling data. The photographs of the simulated flow were obtained. The flow line velocities were measured in the main cylindrical conduit (plume conduit) and at the main conduit/eruption conduit interface. A stagnant area is detected in the 'conduit wall/plume roof{\textquoteright} interface zone. The melt flow in the eruption conduit was analyzed as a turbulent flow in the straight cylindrical conduit with diameter dк. According to the experimental modeling and theoretical data, the superlithostatic pressure in the plume conduit is the sum of the frictional pressure drop and the increasing dynamic pressure in the eruption conduit. A relationship between the melt flow velocity in the eruption conduit and superlithostatic pressure has been derived.",
keywords = "Eruption conduit, Flow velocity, Free-convection flows, Melt, Superlithostatic pressure, Thermal power, Thermochemical plume, thermochemical plume, thermal power, free-convection flows, melt, superlithostatic pressure, flow velocity, eruption conduit, MANTLE PLUMES, THERMAL POWER, KIMBERLITES, DIAMONDS",
author = "Kirdyashkin, {A. G.} and Kirdyashkin, {A. A.} and Distanov, {V. E.} and Gladkov, {I. N.}",
year = "2019",
month = jan,
day = "1",
doi = "10.5800/GT-2019-10-2-0413",
language = "English",
volume = "10",
pages = "247--263",
journal = "Geodynamics and Tectonophysics",
issn = "2078-502X",
publisher = "Institute of the Earth's Crust",
number = "2",

}

RIS

TY - JOUR

T1 - Experimental and theoretical modeling of diamondiferous plumes

AU - Kirdyashkin, A. G.

AU - Kirdyashkin, A. A.

AU - Distanov, V. E.

AU - Gladkov, I. N.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - We consider thermochemical mantle plumes with thermal power 1.6·1010 W<N<2.7·1010 W (relative thermal power 1.15<Ka<1.9) as plumes with an intermediate thermal power. Such plumes are formed at the core–mantle boundary beneath cratons in the absence of horizontal free‐convection mantle flows beneath them, or in the presence of weak horizontal mantle flows. A proposed scheme of convection flows in the conduit of a plume with an intermediate thermal power is based on laboratory and theoretical modeling data. A plume ascends (melts out) from the core-mantle boundary to critical depth xкр from which magma erupts on the Earth’s surface. The magmatic melt erupts from the plume conduit onto the surface through the eruption conduit. The latter forms under the effect of superlithostatic pressure on the plume roof. While the thickness of the block above the plume roof decreases to a critical value xкр, the shear stress on its cylindrical surface reaches a critical value (strength limit) τкр.Rock fails in the vicinity of the cylindrical block and, as a consequence, the eruption conduit is formed. We estimate the height of the eruption conduit and the time for the plume to ascent to the critical depth xкр. The volume of erupted melt is estimated for kinematic viscosity of melt v=0.5–2 м2/с. The depth Δx from which the melt is transported to the surface is determined. Using the eruption volume, we obtain a relationship between the depth Δx and the plume conduit diameter for the above‐mentioned kinematic viscosities. In the case that the depth Δx is larger than 150 km, the melt from the plume conduit can transport diamonds to the Earth’s surface. Thus, the plumes with an intermediate thermal power are diamondiferous. The melt flow structure at the plume conduit/eruption conduit interface is determined on the basis of the laboratory modeling data. The photographs of the simulated flow were obtained. The flow line velocities were measured in the main cylindrical conduit (plume conduit) and at the main conduit/eruption conduit interface. A stagnant area is detected in the 'conduit wall/plume roof’ interface zone. The melt flow in the eruption conduit was analyzed as a turbulent flow in the straight cylindrical conduit with diameter dк. According to the experimental modeling and theoretical data, the superlithostatic pressure in the plume conduit is the sum of the frictional pressure drop and the increasing dynamic pressure in the eruption conduit. A relationship between the melt flow velocity in the eruption conduit and superlithostatic pressure has been derived.

AB - We consider thermochemical mantle plumes with thermal power 1.6·1010 W<N<2.7·1010 W (relative thermal power 1.15<Ka<1.9) as plumes with an intermediate thermal power. Such plumes are formed at the core–mantle boundary beneath cratons in the absence of horizontal free‐convection mantle flows beneath them, or in the presence of weak horizontal mantle flows. A proposed scheme of convection flows in the conduit of a plume with an intermediate thermal power is based on laboratory and theoretical modeling data. A plume ascends (melts out) from the core-mantle boundary to critical depth xкр from which magma erupts on the Earth’s surface. The magmatic melt erupts from the plume conduit onto the surface through the eruption conduit. The latter forms under the effect of superlithostatic pressure on the plume roof. While the thickness of the block above the plume roof decreases to a critical value xкр, the shear stress on its cylindrical surface reaches a critical value (strength limit) τкр.Rock fails in the vicinity of the cylindrical block and, as a consequence, the eruption conduit is formed. We estimate the height of the eruption conduit and the time for the plume to ascent to the critical depth xкр. The volume of erupted melt is estimated for kinematic viscosity of melt v=0.5–2 м2/с. The depth Δx from which the melt is transported to the surface is determined. Using the eruption volume, we obtain a relationship between the depth Δx and the plume conduit diameter for the above‐mentioned kinematic viscosities. In the case that the depth Δx is larger than 150 km, the melt from the plume conduit can transport diamonds to the Earth’s surface. Thus, the plumes with an intermediate thermal power are diamondiferous. The melt flow structure at the plume conduit/eruption conduit interface is determined on the basis of the laboratory modeling data. The photographs of the simulated flow were obtained. The flow line velocities were measured in the main cylindrical conduit (plume conduit) and at the main conduit/eruption conduit interface. A stagnant area is detected in the 'conduit wall/plume roof’ interface zone. The melt flow in the eruption conduit was analyzed as a turbulent flow in the straight cylindrical conduit with diameter dк. According to the experimental modeling and theoretical data, the superlithostatic pressure in the plume conduit is the sum of the frictional pressure drop and the increasing dynamic pressure in the eruption conduit. A relationship between the melt flow velocity in the eruption conduit and superlithostatic pressure has been derived.

KW - Eruption conduit

KW - Flow velocity

KW - Free-convection flows

KW - Melt

KW - Superlithostatic pressure

KW - Thermal power

KW - Thermochemical plume

KW - thermochemical plume

KW - thermal power

KW - free-convection flows

KW - melt

KW - superlithostatic pressure

KW - flow velocity

KW - eruption conduit

KW - MANTLE PLUMES

KW - THERMAL POWER

KW - KIMBERLITES

KW - DIAMONDS

UR - http://www.scopus.com/inward/record.url?scp=85076591670&partnerID=8YFLogxK

UR - https://www.elibrary.ru/item.asp?id=38303710

U2 - 10.5800/GT-2019-10-2-0413

DO - 10.5800/GT-2019-10-2-0413

M3 - Article

AN - SCOPUS:85076591670

VL - 10

SP - 247

EP - 263

JO - Geodynamics and Tectonophysics

JF - Geodynamics and Tectonophysics

SN - 2078-502X

IS - 2

ER -

ID: 22999248