A Parametric Method to Model 3D Displacements Around Faults with Volumetric Vector Fields G
A parametric method to model 3D displacements around faults with volumetric vector fields G. Laurent, G. Caumon, A. Bouziat, M. Jessell To cite this version: G. Laurent, G. Caumon, A. Bouziat, M. Jessell. A parametric method to model 3D displace- ments around faults with volumetric vector fields. Tectonophysics, Elsevier, 2013, 590, pp.83-93. 10.1016/j.tecto.2013.01.015. hal-01301478 HAL Id: hal-01301478 https://hal.archives-ouvertes.fr/hal-01301478 Submitted on 23 Jul 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A parametric method to model 3D displacements around faults with volumetric vector fieldsI Gautier Laurenta,b,∗, Guillaume Caumona,b, Antoine Bouziata,b,1, Mark Jessellc, Gautier Laurenta,b,∗, Guillaume Caumona,b, Antoine Bouziata,b,1, Mark Jessellc aUniversit´ede Lorraine, CRPG UPR 2300, Vandoeuvre-l`es-Nancy,54501, France bCNRS, CRPG, UPR 2300, Vandoeuvre-l`es-Nancy, 54501, France cIRD, UR 234, GET, OMP, Universit´eToulouse III, 14 Avenue Edouard Belin, 31400 Toulouse, FRANCE Abstract This paper presents a 3D parametric fault representation for modeling the displacement field associated with faults in accordance with their geometry. The displacements are modeled in a canonical fault space where the near-field displacement is defined by a small set of parameters consisting of the maximum displacement amplitude and the profiles of attenuation in the surrounding space.
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