Granitic rocks are a major component of the continental crust and
the many and complex problems of their origin that have challenged
geologists over some 200 years still are presenting challenges
today. Current ideas of granite formation involve lower crustal
melting, segregation, ascent (as dykes or diapirs) and emplacement
in the upper crust.In this book we suggest an alternative model for
the origin of granite in terms of in-situ meltingintracrustal
convection that physically determines the process from partial
melting of mid-upper crustal rocks to formation of a convecting
magma layer. We illustrate the model using the geological,
geochemical and geophysical studies from Australia, North and South
America, Europe and China, and conclude that heat convection within
a crustal partial melting layer is essential for formation of
granite magma and that without convection, partial melting of rocks
produces migmatites rather than granites.
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