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- W1012471284 endingPage "214" @default.
- W1012471284 startingPage "181" @default.
- W1012471284 abstract "A non steady-state thermal model is proposed for the axial domain of spreading ridges, in which accretion is simulated as the superposition of seafloor spreading and thermal inputs which vary through time associated with magmato-tectonic cycles. Realistic time frequencies of accretion are tested for extreme cases of slow and fast spreading ridges. The thermal structure, melt fraction and crustal production are computed. For fast spreading ridges, the partial melt region is very wide and varies little through time; the associated crustal production is large and nearly constant. In contrast, melting zones beneath slow spreading ridges are narrow and waxing and waning through time; the associated crustal production decreases dramatically toward zero at the end of cycles. Our model reconciles opposing views on the geometry of the melting regions beneath spreading centres and their relationship to spreading rate. In addition, it accounts for the occurrence of mantle rock outcrops reported along the ridge axis and for the relationship between their relative abundance and axial segmentation." @default.
- W1012471284 created "2016-06-24" @default.
- W1012471284 creator A5029213050 @default.
- W1012471284 creator A5069428530 @default.
- W1012471284 date "1995-01-01" @default.
- W1012471284 modified "2023-09-25" @default.
- W1012471284 title "Non Steady-State Thermal Model of Spreading Ridges: Implications for Melt Generation and Mantle Outcrops" @default.
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