untitled
<OAI-PMH schemaLocation=http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd>
<responseDate>2018-01-15T15:40:40Z</responseDate>
<request identifier=oai:HAL:hal-00420888v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request>
<GetRecord>
<record>
<header>
<identifier>oai:HAL:hal-00420888v1</identifier>
<datestamp>2018-01-11</datestamp>
<setSpec>type:ART</setSpec>
<setSpec>subject:sdu</setSpec>
<setSpec>subject:sde</setSpec>
<setSpec>collection:CNRS</setSpec>
<setSpec>collection:SDE</setSpec>
<setSpec>collection:GM</setSpec>
<setSpec>collection:GIP-BE</setSpec>
<setSpec>collection:AGROPOLIS</setSpec>
<setSpec>collection:INSU</setSpec>
<setSpec>collection:B3ESTE</setSpec>
<setSpec>collection:UNIV-AG</setSpec>
<setSpec>collection:UNIV-MONTPELLIER</setSpec>
</header>
<metadata><dc>
<publisher>HAL CCSD</publisher>
<title lang=en>Geometry, displacement-length scaling, and extensional strain of normal faults on Mars with inferences on mechanical stratigraphy of the Martian crust</title>
<creator>Polit, Anjani T.</creator>
<creator>Schultz, Richard A.</creator>
<creator>Soliva, Roger</creator>
<contributor>Mackay School of Earth Sciences and Engineering, University of Nevada, Reno ; Université du Québec</contributor>
<contributor>Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<description>International audience</description>
<source>ISSN: 0191-8141</source>
<source>Journal of Structural Geology</source>
<publisher>Elsevier</publisher>
<identifier>hal-00420888</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-00420888</identifier>
<source>https://hal.archives-ouvertes.fr/hal-00420888</source>
<source>Journal of Structural Geology, Elsevier, 2009, 31 (7), pp.662-673. 〈10.1016/j.jsg.2009.03.016〉</source>
<identifier>DOI : 10.1016/j.jsg.2009.03.016</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/j.jsg.2009.03.016</relation>
<language>en</language>
<subject lang=en>Displacement-length scaling</subject>
<subject lang=en>Normal faults</subject>
<subject lang=en>Grabens</subject>
<subject lang=en>Mars</subject>
<subject lang=en>Fault restriction</subject>
<subject lang=en>segmented normal faults</subject>
<subject lang=en>thermal emission</subject>
<subject>[SDU.STU.TE] Sciences of the Universe [physics]/Earth Sciences/Tectonics</subject>
<subject>[SDE.MCG] Environmental Sciences/Global Changes</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>We measure throw distributions for graben-bounding normal faults from two areas on Mars to investigate fault growth, displacement-length (D-max-L) scaling, and extensional strain using a complementary suite of techniques. Faults in the northern plains are inferred to be restricted at 2-3 km depth, as shown by a transition from linear scaling, with D-max-L ratios of similar to 1 x 10(-3), to nonlinear scaling for faults >50 km long. On the Alba Patera volcano, faults conform to linear Dmax-L scaling, with a Dmax-L ratio of similar to 6 x 10(-3), consistent with more deeply penetrating faults that are not restricted at depth. These grabens accommodate larger extensional strains (similar to 0.84%) than the faults in the northern plains (similar to 0.23%), with a temporal change from regionally distributed to localized deformation and associated increases in D-max-L ratio extensional strain, and perhaps down-dip fault height. The results suggest that both spatial and temporal variations in extensional strain and displacement-length scaling relations, along with fault restriction, are recorded by Martian fault populations. (C) 2009 Elsevier Ltd. All rights reserved.</description>
<date>2009</date>
</dc>
</metadata>
</record>
</GetRecord>
</OAI-PMH>
