Smectite swelling in the Miura-Boso accretionary prism: Possible cause for incipient décollement zone formation

Tectonophysics

Volumn 494, Issue 1-2, 2010, Pages 75-84

  Kameda, Jun ^a   Yamamoto, Yuzuru ^b   Kimura, Gaku ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b JAPAN AGENCY FOR MARINE EARTH SCIENCE AND TECHNOLOGY   (Japan)

Author keywords

Accretionary prism; Clay minerals; D collement; Off scraping; Swelling pressure; XRD

Indexed keywords

ACCRETIONARY PRISM; COMBINED EFFECT; DEFORMATION STRUCTURE; EFFECTIVE PRESSURE; HIGH SWELLING; ILLITE-SMECTITE; MECHANICAL HETEROGENEITY; MINERAL COMPOSITION; MIXED LAYER; OFF-SCRAPING; PREFERRED ORIENTATIONS; SMECTITES; SPATIAL VARIATIONS; SWELLING PRESSURE; UPPER MIOCENE; XRD; XRD ANALYSIS;

CARBONATE MINERALS; CRYSTALLOGRAPHY; KAOLINITE; MINERALOGY; MINERALS; PRISMS; QUARTZ; SEDIMENTOLOGY; SILICATE MINERALS; SWELLING;

PRESSURE EFFECTS;

ACCRETIONARY PRISM; DECOLLEMENT; DEFORMATION MECHANISM; ILLITE; KAOLINITE; MINERALOGY; PLAGIOCLASE; PORE PRESSURE; PREFERRED ORIENTATION; PRESSURE EFFECT; PRESSURE FIELD; SILT; SMECTITE; SPATIAL VARIATION; SWELLING; X-RAY DIFFRACTION;

BOSO PENINSULA; CHIBA; HONSHU; JAPAN; KANAGAWA; KANTO; MIURA PENINSULA;

EID: 78650076143     PISSN: 00401951     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.tecto.2010.08.008     Document Type: Article

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