6. Величина и скорость производства магмы зависят от интенсивности флюидного потока и глубинной геодинамики мантийного клина, заметно возрастая в зонах растяжения.
Авторы крайне благодарны А.Колоскову, Г.Флерову, О.Волынцу, К.Ойстерхуз, П.Плечову и А.Максимову за продуктивное обсуждение материала и помощь в течение полевых работ. Эта работа была поддержана проектами DFG Wo362/15-1+2, INTAS No. 94-3129, грантами DFG-РФФИ No. 98-05-04103 и 00-0504000 и фондом Фольксвагена.
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