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Volcanic input to the atmosphere from Alba Patera on Mars

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Volcanic input to the atmosphere from Alba Patera on Mars. / Wilson, Lionel; Mouginis-Mark, Peter J.
In: Nature, Vol. 330, No. 6146, 26.11.1987, p. 354-357.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Wilson, L & Mouginis-Mark, PJ 1987, 'Volcanic input to the atmosphere from Alba Patera on Mars', Nature, vol. 330, no. 6146, pp. 354-357. https://doi.org/10.1038/330354a0

APA

Vancouver

Wilson L, Mouginis-Mark PJ. Volcanic input to the atmosphere from Alba Patera on Mars. Nature. 1987 Nov 26;330(6146):354-357. doi: 10.1038/330354a0

Author

Wilson, Lionel ; Mouginis-Mark, Peter J. / Volcanic input to the atmosphere from Alba Patera on Mars. In: Nature. 1987 ; Vol. 330, No. 6146. pp. 354-357.

Bibtex

@article{9a26c88d6c76447ea8dae1b1ef33281b,
title = "Volcanic input to the atmosphere from Alba Patera on Mars",
abstract = "With the recent increased interest in the evolution of volcanism, tectonism and volatiles on Mars, several studies have been initiated to infer the mass of water vapour and carbon dioxide that might have been released from magmas erupted on the martian surface over geological time (see refs 1,2). Such studies are complementary to investigations of the global volatile inventory for Mars3,4, which trace a constant mass of volatiles to various sinks in the regolith, atmosphere and polar caps. Of necessity, these volatile distribution models are generalizations of Mars-wide averages. Here we present what we believe to be the first estimates for the amount of water vapour and/or carbon dioxide released, together with the corresponding release rates, from specific volcanic deposits on a relatively young martian volcanic construct (Alba Patera).",
author = "Lionel Wilson and Mouginis-Mark, {Peter J.}",
year = "1987",
month = nov,
day = "26",
doi = "10.1038/330354a0",
language = "English",
volume = "330",
pages = "354--357",
journal = "Nature",
issn = "0028-0836",
publisher = "Nature Publishing Group",
number = "6146",

}

RIS

TY - JOUR

T1 - Volcanic input to the atmosphere from Alba Patera on Mars

AU - Wilson, Lionel

AU - Mouginis-Mark, Peter J.

PY - 1987/11/26

Y1 - 1987/11/26

N2 - With the recent increased interest in the evolution of volcanism, tectonism and volatiles on Mars, several studies have been initiated to infer the mass of water vapour and carbon dioxide that might have been released from magmas erupted on the martian surface over geological time (see refs 1,2). Such studies are complementary to investigations of the global volatile inventory for Mars3,4, which trace a constant mass of volatiles to various sinks in the regolith, atmosphere and polar caps. Of necessity, these volatile distribution models are generalizations of Mars-wide averages. Here we present what we believe to be the first estimates for the amount of water vapour and/or carbon dioxide released, together with the corresponding release rates, from specific volcanic deposits on a relatively young martian volcanic construct (Alba Patera).

AB - With the recent increased interest in the evolution of volcanism, tectonism and volatiles on Mars, several studies have been initiated to infer the mass of water vapour and carbon dioxide that might have been released from magmas erupted on the martian surface over geological time (see refs 1,2). Such studies are complementary to investigations of the global volatile inventory for Mars3,4, which trace a constant mass of volatiles to various sinks in the regolith, atmosphere and polar caps. Of necessity, these volatile distribution models are generalizations of Mars-wide averages. Here we present what we believe to be the first estimates for the amount of water vapour and/or carbon dioxide released, together with the corresponding release rates, from specific volcanic deposits on a relatively young martian volcanic construct (Alba Patera).

U2 - 10.1038/330354a0

DO - 10.1038/330354a0

M3 - Journal article

AN - SCOPUS:0000809302

VL - 330

SP - 354

EP - 357

JO - Nature

JF - Nature

SN - 0028-0836

IS - 6146

ER -