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The youngest Alpine magmatism (Miocene to Quaternary) in Western and Central Anatolia is represented by three coeval assemblages from West to East. They are the Western Anatolian Volcanic assemblage (...
The Alpine belt comprises several pieces of Pre-Mesozoic basement, which have received various imprints of the successive Paleozoic orogenic episodes. If Pre-Mesozoic palinspatic reconstructions are ...
To evaluate the origin and significance of microgranular enclaves hosted by granites, we present new data on two granitoid series belonging to the Los Pedroches Batholith (LPB), SW Iberian Massif, Spa...
Magmatic evolution of the Moon     Magmatic evolution  Moon  rock types  KREEP   Stage       font style='font-size:12px;'> 2012/4/1
Although incomplete because of the imperfect and somewhat random sampling of rock types by the Apollo and Luna missions (1969(R)C1976), the history of lunar magmatism has been reconstructe by numero...
Experiments on tonalite and granodiorite wereperformed at conditions ranging from 2.1 to 18kbar and 550 to 850°C to establish the magmatic stability field ofepidote as a function ofP, T,and f02. Atwat...

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