What is a "Typical” Mantle Plume?

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Published in:Геофизический журнал
Date:2010
Main Authors: Harris, A., Kincaid, Ch.
Format: Article
Language:English
Published: Інститут геофізики ім. С.I. Субботіна НАН України 2010
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/103530
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:What is a "Typical” Mantle Plume? / A. Harris, Ch. Kincaid // Геофизический журнал. — 2010. — Т. 32, № 4. — С. 214. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Harris, A.
Kincaid, Ch.
author_facet Harris, A.
Kincaid, Ch.
citation_txt What is a "Typical” Mantle Plume? / A. Harris, Ch. Kincaid // Геофизический журнал. — 2010. — Т. 32, № 4. — С. 214. — англ.
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fulltext ������� ��� ����� ���� ��� ������������� �� !"# $ �% &' (�% �)�) What is a “Typical” Mantle Plume? A. Harris, Ch. Kincaid, 2010 University of Rhode Island, Graduate School of Oceanography, Narragansett, USA Process models for mantle plumes, and indeed arguments for the existence of mantle plumes, are largely based on expected characteristics for these upwelling features. Typically plume models have large heads (>500 km), moderately slender tails (~100 km), uniform compositions (lower to upper mantle/Lherzolite), and high excess temperatures (200 C or more). Here we present laboratory mod- els of mantle convection with recycled, chemically laminated lithosphere which reveal a diversity in size, composition, temperature and both surface geologi- cal and geophysical expressions. Results suggest there is no typical mantle plume, but rather a range in plume classes. Examples from within the differ- ent classes can readily explain the diversity in plume surface expressions, from large igneous provinces with associated tails (time progressive island chains), to headless plumes and large (or small) headed plumes with no tails. The traditional large headed, uniform composition, high excess tempera- ture plume was rarely seen in the 25 experiments conducted to date. Laboratory models utilized a glu- cose syrup (Ra=105 106) for a working fluid. Mix- tures of syrup and water were used to introduce density and viscosity contrasts between the ambi- ent fluid and a dyed, chilled and layered slab repre- senting recycled lithosphere. Generally, one layer of the slab was less dense than the ambient fluid (representing Harzburgite) and one layer was denser than the ambient fluid (representing Eclogite). A ther- mal boundary layer was developed at the base of a 20 20 15 cm tank by uniform basal heating. Inter- action between the slab layers and fluid within the thermal boundary layer had a strong influence over the distribution of thermochemical heterogeneity within upwelling plumes. A range of repeatable plume styles emerged from this study. One promi- nent plume style is characterized by upwellings growing shortly after slabs enter the thermal bound- ary layer. These plumes are Harzburgite-rich and range from cooler (~100 C) than ambient mantle to nearly equivalent with background temperature. Two common forms of chemical heterogeneity are seen, one in which these plumes have a thin (~10 km), Eclogite core. Plumes of this type that form from the edge of a slab pile have near perfect bilateral symmetry, containing half Harzburgite and half Lherzolite material from within the thermal bound- ary layer. Another common style of upwelling is re- corded over a range of parameter combinations and occurs well after recycled material has reached and spread within the thermal boundary layer. These are hotter plumes (~200—400 C excess temperature) with predictable distributions of both slab compo- nents (Harzburgite and Eclogite) and ambient ther- mal boundary layer material (Lherzolite). Length scales of thermochemical heterogeneity range from 1 km to >100 km depending on chemical density contrasts and local processes of instability forma- tion within the basal boundary layer. A number of cases from distinct upwelling classes are digitized and used to drive synthetic melting and seismic mod- els. Results show that more typical “plume-like” patterns can occur, but more commonly cases show extreme spatial and temporal discontinuities in melt production and seismic velocity patterns.
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institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 0203-3100
language English
last_indexed 2025-11-30T17:32:14Z
publishDate 2010
publisher Інститут геофізики ім. С.I. Субботіна НАН України
record_format dspace
spelling Harris, A.
Kincaid, Ch.
2016-06-19T11:48:22Z
2016-06-19T11:48:22Z
2010
What is a "Typical” Mantle Plume? / A. Harris, Ch. Kincaid // Геофизический журнал. — 2010. — Т. 32, № 4. — С. 214. — англ.
0203-3100
https://nasplib.isofts.kiev.ua/handle/123456789/103530
en
Інститут геофізики ім. С.I. Субботіна НАН України
Геофизический журнал
What is a "Typical” Mantle Plume?
Article
published earlier
spellingShingle What is a "Typical” Mantle Plume?
Harris, A.
Kincaid, Ch.
title What is a "Typical” Mantle Plume?
title_full What is a "Typical” Mantle Plume?
title_fullStr What is a "Typical” Mantle Plume?
title_full_unstemmed What is a "Typical” Mantle Plume?
title_short What is a "Typical” Mantle Plume?
title_sort what is a "typical” mantle plume?
url https://nasplib.isofts.kiev.ua/handle/123456789/103530
work_keys_str_mv AT harrisa whatisatypicalmantleplume
AT kincaidch whatisatypicalmantleplume