Deutsch
 
Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
 ZurückNächste 
  Grain-size evolution in subducted oceanic lithosphere associated with the olivine-spinal transformation and ist effects on rheology

Riedel, M. R., Karato, S. (1997): Grain-size evolution in subducted oceanic lithosphere associated with the olivine-spinal transformation and ist effects on rheology. - Earth and Planetary Science Letters, 148, 27-43.
https://doi.org/10.1016/S0012-821X(97)00016-2

Item is

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Riedel, M. R.1, Autor              
Karato, S.2, Autor
2.1 Physics of Earthquakes and Volcanoes, 2.0 Physics of the Earth, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, Autor              
Affiliations:
10 Pre-GFZ, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146023              
2External Organizations, ou_persistent22              

Inhalt

einblenden:
ausblenden:
Schlagwörter: subduction zones; rheology; phase transitions; deep-focus earthquakes; grain size; kinetics
 DDC: 550 - Earth sciences
 Zusammenfassung: Abstract: We investigate the role of grain-size reduction during the olivine-spinal transformation on rheological properties of subducting slabs on the basis of a scaling model for micro structural development during nucleation and growth. In this model, the size of spinal grains nucleating at olivine grain-boundaries is controlled by the relative rates of nucleation and growth, taking into account the impingement through the collision of grains due to growth. When the volume fraction of spinal reaches a certain threshold value (critical volume fraction ~ 1 to 10 %, depending on the P,T conditions in the slab), the new phase will form a continuous film and will significantly reduce the strength of the two-phase aggregate if spinal grain-size is small. The size of spinal grains delta 0 at this stage is calculated and is shown to be highly sensitive to temperature. At relatively high temperatures (T > 1000 K), delta_0 shows an Arrhenius-type dependence on temperature, that is delta_0 ~ exp(-E* /RT) with E* ~ 400 kJ/mol, whereas a more complicated temperature dependence is found at low temperatures (T < 900 K), where a grain-size reduction of up to 4 orders in magnitude is possible. Strength profiles of slabs due to combined effects of temperatures and of grain-size reduction are calculated. It is shown that: (1) the strength of slabs will have an unusual temperature dependence through the temperature dependence of grain-size; and (2) a subducting slab has a complicated rheological structure containing a weak region below the tip of a metastable olivine-bearing wedge in a cold slab. Possible implications of these anomalous rheological structures of slabs on the dynamics of subduction are discussed including the mechanisms of deep earthquakes.

Details

einblenden:
ausblenden:
Sprache(n):
 Datum: 1997
 Publikationsstatus: Final veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: eDoc: 88
DOI: 10.1016/S0012-821X(97)00016-2
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Earth and Planetary Science Letters
Genre der Quelle: Zeitschrift, SCI, Scopus
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 148 Artikelnummer: - Start- / Endseite: 27 - 43 Identifikator: CoNE: https://gfzpublic.gfz-potsdam.de/cone/journals/resource/journals99