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Ascent and eruption of basaltic magma on the Earth and moon

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Ascent and eruption of basaltic magma on the Earth and moon. / Wilson, L.; Head, James W.
In: Journal of Geophysical Research, Vol. 86, No. B4, 10.04.1981, p. 2971-3001.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Wilson, L & Head, JW 1981, 'Ascent and eruption of basaltic magma on the Earth and moon', Journal of Geophysical Research, vol. 86, no. B4, pp. 2971-3001. https://doi.org/10.1029/JB086iB04p02971

APA

Wilson, L., & Head, J. W. (1981). Ascent and eruption of basaltic magma on the Earth and moon. Journal of Geophysical Research, 86(B4), 2971-3001. https://doi.org/10.1029/JB086iB04p02971

Vancouver

Wilson L, Head JW. Ascent and eruption of basaltic magma on the Earth and moon. Journal of Geophysical Research. 1981 Apr 10;86(B4):2971-3001. doi: 10.1029/JB086iB04p02971

Author

Wilson, L. ; Head, James W. / Ascent and eruption of basaltic magma on the Earth and moon. In: Journal of Geophysical Research. 1981 ; Vol. 86, No. B4. pp. 2971-3001.

Bibtex

@article{adb1e0468d9f40b5aecac0559b94e8cb,
title = "Ascent and eruption of basaltic magma on the Earth and moon",
abstract = "Geological and physical observations and constraints are applied to the development of a modelof the ascent and emplacement of basaltic magma on the earth and moon. Mathematical models of the nature and motion of gas/liquid mixtures are developed and show that gas exsolution from terrestrial and lunar magmas commonly only occurs at shallow depths (less than 2km); thus the ascent of bubble-free magma at depth can be treated separately from the complex motions caused by gas exsolution near the surface. Magma ascent is related to dike or conduit width; a lower limit to width is determined by the presence of a finite magma yield strength or by excessive magma cooling effects related to magma viscosity. For terrestrial basalts with negligible yield strengths and viscosities greater than 102Pa s, widths in the range 0.2-0.6m are needed to allow eruptions from between depths of 0.5-20km. Fissure widths of about 4m would be needed to account for the output rates estimated for the Columbia River flood basalt eruptions.-Authors",
author = "L. Wilson and Head, {James W.}",
year = "1981",
month = apr,
day = "10",
doi = "10.1029/JB086iB04p02971",
language = "English",
volume = "86",
pages = "2971--3001",
journal = "Journal of Geophysical Research",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "B4",

}

RIS

TY - JOUR

T1 - Ascent and eruption of basaltic magma on the Earth and moon

AU - Wilson, L.

AU - Head, James W.

PY - 1981/4/10

Y1 - 1981/4/10

N2 - Geological and physical observations and constraints are applied to the development of a modelof the ascent and emplacement of basaltic magma on the earth and moon. Mathematical models of the nature and motion of gas/liquid mixtures are developed and show that gas exsolution from terrestrial and lunar magmas commonly only occurs at shallow depths (less than 2km); thus the ascent of bubble-free magma at depth can be treated separately from the complex motions caused by gas exsolution near the surface. Magma ascent is related to dike or conduit width; a lower limit to width is determined by the presence of a finite magma yield strength or by excessive magma cooling effects related to magma viscosity. For terrestrial basalts with negligible yield strengths and viscosities greater than 102Pa s, widths in the range 0.2-0.6m are needed to allow eruptions from between depths of 0.5-20km. Fissure widths of about 4m would be needed to account for the output rates estimated for the Columbia River flood basalt eruptions.-Authors

AB - Geological and physical observations and constraints are applied to the development of a modelof the ascent and emplacement of basaltic magma on the earth and moon. Mathematical models of the nature and motion of gas/liquid mixtures are developed and show that gas exsolution from terrestrial and lunar magmas commonly only occurs at shallow depths (less than 2km); thus the ascent of bubble-free magma at depth can be treated separately from the complex motions caused by gas exsolution near the surface. Magma ascent is related to dike or conduit width; a lower limit to width is determined by the presence of a finite magma yield strength or by excessive magma cooling effects related to magma viscosity. For terrestrial basalts with negligible yield strengths and viscosities greater than 102Pa s, widths in the range 0.2-0.6m are needed to allow eruptions from between depths of 0.5-20km. Fissure widths of about 4m would be needed to account for the output rates estimated for the Columbia River flood basalt eruptions.-Authors

U2 - 10.1029/JB086iB04p02971

DO - 10.1029/JB086iB04p02971

M3 - Journal article

AN - SCOPUS:0019368359

VL - 86

SP - 2971

EP - 3001

JO - Journal of Geophysical Research

JF - Journal of Geophysical Research

SN - 0148-0227

IS - B4

ER -