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Lava thicknesses: Implications for rheological and crustal developmentThe morphology of a lava flow is strongly influenced by its rheological structure. The rheological structure is, in turn, dependent on numerous factors including: (1) bulk composition, (2) crystallingity, (3) vesicularity, and (4) crustal development. Identifying which of the latter factors are most significant, and hence most readily investigated by remote-sensing techniques, is necessary to clarify short-term objectives and expectations from the study of Martian lava flows. Insights into the rheological controls on flow morphology are provided by variations in thickness of undrained lava streams on Etna and Vesuvius, Southern Italy. Both pahoehoe and aa lavas were studied.
Document ID
19880021106
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kilburn, C. R. J.
(Consiglio Nazionale delle Ricerche Naples (Italy), United States)
Lopes, R. M. C.
(London Univ. Observatory, United Kingdom)
Date Acquired
September 5, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Lunar and Planetary Inst., NASA MEVTV Program Working Group Meeting: Volcanism on Mars
Subject Category
Geophysics
Accession Number
88N30490
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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