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Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data

Research output: Contribution to Journal/Magazine › Journal article

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Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data. / Pavri, B.; Head, J. W.; Klose, K. B. et al.
In: Journal of Geophysical Research: Planets, Vol. 97, No. E8, 1992, p. 13445-13478.

Research output: Contribution to Journal/Magazine › Journal article

Harvard

Pavri, B, Head, JW, Klose, KB & Wilson, L 1992, 'Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data', Journal of Geophysical Research: Planets, vol. 97, no. E8, pp. 13445-13478. https://doi.org/10.1029/92JE01162

APA

Pavri, B., Head, J. W., Klose, K. B., & Wilson, L. (1992). Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data. Journal of Geophysical Research: Planets, 97(E8), 13445-13478. https://doi.org/10.1029/92JE01162

Vancouver

Pavri B, Head JW, Klose KB, Wilson L. Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data. Journal of Geophysical Research: Planets. 1992;97(E8):13445-13478. doi: 10.1029/92JE01162

Author

Pavri, B. ; Head, J. W. ; Klose, K. B. et al. / Steep-sided domes on Venus : characteristics, geologic setting, and eruption conditions from Magellan data. In: Journal of Geophysical Research: Planets. 1992 ; Vol. 97, No. E8. pp. 13445-13478.

Bibtex

@article{95cb465f15fc4917b78abd033c47a795,
title = "Steep-sided domes on Venus: characteristics, geologic setting, and eruption conditions from Magellan data",
abstract = "A survey of more than 95 percent of the Venus surface reveals 145 steep-sided domes which can be subdivided into a variety of morphologic forms, the most common being shaped like inverted bowls or flat-topped domes. Results of a preliminary analysis of the distribution and geologic setting of the domes are presented. The relation of the domes to analogous terrestrial features is examined, and possible models for their mode of emplacement are outlined.",
keywords = "Domes (Geology), Magellan Spacecraft (NASA), Planetary Geology, Satellite Imagery, Venus Surface, Data Flow Analysis, Planetary Structure, Rhyolite",
author = "B. Pavri and Head, {J. W.} and Klose, {K. B.} and L. Wilson",
year = "1992",
doi = "10.1029/92JE01162",
language = "English",
volume = "97",
pages = "13445--13478",
journal = "Journal of Geophysical Research: Planets",
issn = "2169-9100",
publisher = "Blackwell Publishing Ltd",
number = "E8",

}

RIS

TY - JOUR

T1 - Steep-sided domes on Venus

T2 - characteristics, geologic setting, and eruption conditions from Magellan data

AU - Pavri, B.

AU - Head, J. W.

AU - Klose, K. B.

AU - Wilson, L.

PY - 1992

Y1 - 1992

N2 - A survey of more than 95 percent of the Venus surface reveals 145 steep-sided domes which can be subdivided into a variety of morphologic forms, the most common being shaped like inverted bowls or flat-topped domes. Results of a preliminary analysis of the distribution and geologic setting of the domes are presented. The relation of the domes to analogous terrestrial features is examined, and possible models for their mode of emplacement are outlined.

AB - A survey of more than 95 percent of the Venus surface reveals 145 steep-sided domes which can be subdivided into a variety of morphologic forms, the most common being shaped like inverted bowls or flat-topped domes. Results of a preliminary analysis of the distribution and geologic setting of the domes are presented. The relation of the domes to analogous terrestrial features is examined, and possible models for their mode of emplacement are outlined.

KW - Domes (Geology)

KW - Magellan Spacecraft (NASA)

KW - Planetary Geology

KW - Satellite Imagery

KW - Venus Surface

KW - Data Flow Analysis

KW - Planetary Structure

KW - Rhyolite

U2 - 10.1029/92JE01162

DO - 10.1029/92JE01162

M3 - Journal article

VL - 97

SP - 13445

EP - 13478

JO - Journal of Geophysical Research: Planets

JF - Journal of Geophysical Research: Planets

SN - 2169-9100

IS - E8

ER -