Other
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988e%26psl..87..127w&link_type=abstract
Earth and Planetary Science Letters (ISSN 0012-821X), vol. 87, no. 1-2, Jan. 1988, p. 127-136.
Other
3
Earth Crust, Earth Planetary Structure, Geotemperature, Himalayas, Planetary Evolution, Isostatic Pressure, Tectonics
Scientific paper
Present crustal evolution models fail to account for the generation of the large volumes of continental crust in the required time intervals. If the oceanic crust was appreciably thicker in the Archaean, as geothermal models would indicate, then oceanic crustal collision on the scale of the present-day Himalayan continental collision zone may have been a frequent occurrence in the Archaean, resulting in extensive partial melting of the hydrous underthrust oceanic crust to produce voluminous tonalite melts leaving a depleted stabilized basic residuum.
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