FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1994153906> ?p ?o ?g. }

• W1994153906 endingPage "19615" @default.
• W1994153906 startingPage "19599" @default.
• W1994153906 abstract "Anisotropy of anhysteretic remanence (AAR), scanning electron microscopy (SEM), and X ray pole figure goniometry studies of clay‐rich sediments were conducted to delineate the interactions between magnetite and clay particles which cause inclination shallowing during compaction. These studies used synthetic sediments composed of kaolinite or illite and two grain sizes of magnetite, 0.45 μm and 2–3 μm. Natural marine sediments which contained 40–50% clay were also used. The sediments were compacted by pressures as high as 0.157 MPa. The sediments' porosity decrease suggests that the compaction experiments model burial depths up to 400–500 m. The main result of this study is that inclination shallowing and void ratio versus pressure curves show two points where behavior changes. A rapid decrease in inclination and void ratio occurs up to a pressure of 0.02 MPa. This is accompanied by a magnetic intensity decrease of 20–30%. Compaction at pressures between 0.02 MPa and 0.05 MPa causes a further decrease in these parameters at moderate rates, while compaction at pressures above 0.05 MPa causes very little change. Percent magnetic anisotropy and X ray pole figure intensity ratio versus pressure curves show only one point where behavior changes at 0.05 MPa with a rapid increase at lower pressures and little change at higher pressures. A model to explain this behavior, based on the SEM observations as well as the magnetic anisotropy, pole figure, and inclination data, suggests that compaction up to 0.02 MPa causes a decrease in pore volume with little reorientation of clay particles. Some magnetic particles are firmly attached to clay particles, whereas other loosely attached particles are either randomized or subvertical ones are preferentially disturbed causing inclination shallowing and an intensity decrease. At pressures between 0.02 MPa and 0.05 MPa, magnetite particles have become firmly attached to clay particles and start to follow the reorientation of clay particles as the clay fabric develops. At 0.05 MPa there is a major change in the clay microstructure with a horizontal fabric becoming evident. Compaction at higher pressures causes little further volume loss and clay particle reorientation and hence little additional inclination shallowing. The randomization/disturbance process suggested by this model causes slightly more than half of the inclination shallowing observed in the samples studied, whereas magnetite‐clay attachment causes the remainder of the inclination decrease." @default.
• W1994153906 created "2016-06-24" @default.
• W1994153906 creator A5035123411 @default.
• W1994153906 creator A5062447455 @default.
• W1994153906 date "1992-12-10" @default.
• W1994153906 modified "2023-10-13" @default.
• W1994153906 title "Magnetic anisotropy, scanning electron microscopy, and X ray pole figure goniometry study of inclination shallowing in a compacting clay‐rich sediment" @default.
• W1994153906 cites W1964093890 @default.
• W1994153906 cites W1970083643 @default.
• W1994153906 cites W1971670411 @default.
• W1994153906 cites W1976283239 @default.
• W1994153906 cites W1987866994 @default.
• W1994153906 cites W1991996909 @default.
• W1994153906 cites W1994835033 @default.
• W1994153906 cites W2004335510 @default.
• W1994153906 cites W2011852791 @default.
• W1994153906 cites W2011903174 @default.
• W1994153906 cites W2012699280 @default.
• W1994153906 cites W2026865121 @default.
• W1994153906 cites W2029350478 @default.
• W1994153906 cites W2030699461 @default.
• W1994153906 cites W2035932459 @default.
• W1994153906 cites W2042633236 @default.
• W1994153906 cites W2049573671 @default.
• W1994153906 cites W2064165463 @default.
• W1994153906 cites W2069594081 @default.
• W1994153906 cites W2069668420 @default.
• W1994153906 cites W2076291288 @default.
• W1994153906 cites W2080128630 @default.
• W1994153906 cites W2081112390 @default.
• W1994153906 cites W2083614796 @default.
• W1994153906 cites W2107996333 @default.
• W1994153906 cites W2108851940 @default.
• W1994153906 cites W2110920310 @default.
• W1994153906 cites W2118204502 @default.
• W1994153906 cites W2126220006 @default.
• W1994153906 cites W2128987520 @default.
• W1994153906 cites W2147773116 @default.
• W1994153906 cites W2150123818 @default.
• W1994153906 cites W2152732732 @default.
• W1994153906 cites W2155640414 @default.
• W1994153906 cites W2155779249 @default.
• W1994153906 cites W2165075535 @default.
• W1994153906 cites W2169550127 @default.
• W1994153906 cites W2332488232 @default.
• W1994153906 cites W4247382079 @default.
• W1994153906 doi "https://doi.org/10.1029/92jb01589" @default.
• W1994153906 hasPublicationYear "1992" @default.
• W1994153906 type Work @default.
• W1994153906 sameAs 1994153906 @default.
• W1994153906 citedByCount "67" @default.
• W1994153906 countsByYear W19941539062012 @default.
• W1994153906 countsByYear W19941539062013 @default.
• W1994153906 countsByYear W19941539062014 @default.
• W1994153906 countsByYear W19941539062015 @default.
• W1994153906 countsByYear W19941539062017 @default.
• W1994153906 countsByYear W19941539062018 @default.
• W1994153906 countsByYear W19941539062019 @default.
• W1994153906 countsByYear W19941539062020 @default.
• W1994153906 countsByYear W19941539062021 @default.
• W1994153906 countsByYear W19941539062022 @default.
• W1994153906 countsByYear W19941539062023 @default.
• W1994153906 crossrefType "journal-article" @default.
• W1994153906 hasAuthorship W1994153906A5035123411 @default.
• W1994153906 hasAuthorship W1994153906A5062447455 @default.
• W1994153906 hasConcept C120665830 @default.
• W1994153906 hasConcept C121332964 @default.
• W1994153906 hasConcept C127313418 @default.
• W1994153906 hasConcept C151730666 @default.
• W1994153906 hasConcept C159985019 @default.
• W1994153906 hasConcept C164374781 @default.
• W1994153906 hasConcept C187320778 @default.
• W1994153906 hasConcept C192562407 @default.
• W1994153906 hasConcept C196715460 @default.
• W1994153906 hasConcept C199289684 @default.
• W1994153906 hasConcept C26771246 @default.
• W1994153906 hasConcept C2777781897 @default.
• W1994153906 hasConcept C2779899878 @default.
• W1994153906 hasConcept C60365795 @default.
• W1994153906 hasConcept C6648577 @default.
• W1994153906 hasConcept C8058405 @default.
• W1994153906 hasConcept C85725439 @default.
• W1994153906 hasConceptScore W1994153906C120665830 @default.
• W1994153906 hasConceptScore W1994153906C121332964 @default.
• W1994153906 hasConceptScore W1994153906C127313418 @default.
• W1994153906 hasConceptScore W1994153906C151730666 @default.
• W1994153906 hasConceptScore W1994153906C159985019 @default.
• W1994153906 hasConceptScore W1994153906C164374781 @default.
• W1994153906 hasConceptScore W1994153906C187320778 @default.
• W1994153906 hasConceptScore W1994153906C192562407 @default.
• W1994153906 hasConceptScore W1994153906C196715460 @default.
• W1994153906 hasConceptScore W1994153906C199289684 @default.
• W1994153906 hasConceptScore W1994153906C26771246 @default.
• W1994153906 hasConceptScore W1994153906C2777781897 @default.
• W1994153906 hasConceptScore W1994153906C2779899878 @default.
• W1994153906 hasConceptScore W1994153906C60365795 @default.
• W1994153906 hasConceptScore W1994153906C6648577 @default.
• W1994153906 hasConceptScore W1994153906C8058405 @default.

• next