Geodynamic regimes of thermochemical mantle plumes

被引:12
|
作者
Kirdyashkin, A. A. [1 ,2 ]
Kirdyashkin, A. G. [1 ]
Distanov, V. E. [1 ]
Gladkov, I. N. [1 ]
机构
[1] Russian Acad Sci, Siberian Branch, VS Sobolev Inst Geol & Mineral, Pr Akad Koptyuga 3, Novosibirsk 630090, Russia
[2] Novosibirsk State Univ, Ul Pirogova 2, Novosibirsk 630090, Russia
关键词
thermochemical plume; thermal power; plume conduit; plume head; melt; intrusive bodies; diamondiferous plumes; batholiths; LARGE IGNEOUS PROVINCES; FLOOD BASALTS; LOWERMOST MANTLE; STARTING PLUMES; EVOLUTION; BOUNDARY; KIMBERLITES; DIAMONDS; DYNAMICS; CONDUIT;
D O I
10.1016/j.rgg.2016.05.003
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Laboratory and numerical experiments simulating the heat transfer and flow structure of thermochemical mantle plumes provide insights into the mechanisms of plume eruption onto the surface depending on the relative thermal power of plumes Ka = N/N-1, where N and N-1 are the heat transferred from the plume base to the plume conduit and the heat transferred from the plume conduit to the surrounding mantle, respectively, under steady thermal conduction. There are three main types of plumes according to the Ka criterion: (i) plumes with low thermal power (Ka < 1.15), which fail to reach the surface, (ii) plumes with intermediate thermal power (1.15 < Ka < 1.9), which occur beneath cratons and transport melts from depths below 150 km, where diamond is stable (diamondiferous plumes), and (iii) plumes with a mushroom-shaped head (1.9 < Ka < 10), which are responsible for large intrusive bodies, including batholiths. The volume of erupted melt and the depth from which the melt is transported to the surface are estimated for plumes of types (ii) and (iii). The relationship between the plume head area (along with the plume head diameter) and the relative thermal power is obtained. The relationship between the thickness of the block above the plume head and the relative thermal power is derived. On the basis of the results obtained, the geodynamic-regime diagram of thermochemical mantle plumes, including the plumes with Ka > 10, has been constructed. (C) 2016, V.S. Sobolev IGM, Siberian Branch of the RAS. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:858 / 867
页数:10
相关论文
共 50 条
  • [41] Narrow, Fast, and "Cool" Mantle Plumes Caused by Strain-Weakening Rheology in Earth's Lower Mantle
    Guelcher, A. J. P.
    Golabek, G. J.
    Thielmann, M.
    Ballmer, M. D.
    Tackley, P. J.
    GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS, 2022, 23 (10)
  • [42] Hotspots, mantle plumes and core heat loss
    Labrosse, S
    EARTH AND PLANETARY SCIENCE LETTERS, 2002, 199 (1-2) : 147 - 156
  • [43] Petrological evidence for secular cooling in mantle plumes
    Herzberg, Claude
    Gazel, Esteban
    NATURE, 2009, 458 (7238) : 619 - U83
  • [44] The Probability of Mantle Plumes in Global Tomographic Models
    Marignier, Augustin
    Ferreira, Ana M. G.
    Kitching, Thomas
    GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS, 2020, 21 (09)
  • [45] Surface subsidence caused by mantle plumes and volcanic loading in large igneous provinces
    Leng, Wei
    Zhong, Shijie
    EARTH AND PLANETARY SCIENCE LETTERS, 2010, 291 (1-4) : 207 - 214
  • [46] Mantle plumes, supercontinents, intracontinental rifting and mineral systems
    Pirajno, Franco
    Santosh, M.
    PRECAMBRIAN RESEARCH, 2015, 259 : 243 - 261
  • [47] Ridge-crossing mantle plumes and gaps in tracks
    Sleep, NH
    GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS, 2002, 3
  • [48] Thermochemical lithosphere differentiation and the origin of cratonic mantle
    Capitanio, Fabio A.
    Nebel, Oliver
    Cawood, Peter A.
    NATURE, 2020, 588 (7836) : 89 - +
  • [49] Lessons from Venus for understanding mantle plumes on Earth
    Ernst, RE
    Desnoyers, DW
    PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 2004, 146 (1-2) : 195 - 229
  • [50] Constraints on mantle plumes on Venus: Implications for volatile history
    Smrekar, Suzanne E.
    Sotin, Christophe
    ICARUS, 2012, 217 (02) : 510 - 523