“…The assumptions of localized tectonic extension and repeated diking events likely contribute to heat preservation and construction of mush regions. There are relatively limited geophysical constraints on the expanse and residence time for lower crustal melt that focus on: 1) petrologic observations on exhumed lower crustal terrains that include for example Ivrea, North Italy (e.g., Sinigoi et al, 1994;Voshage et al, 1990;Wedepohl, 1995); Kohistan, Pakistan (e.g., Burg, 2011;Dhuime et al, 2009;Jagoutz et al, 2007;Jagoutz and Schmidt, 2012); Fraser and Musgrave Ranges, Australia (e.g., Fletcher et al, 1991;White et al, 1999); Sierra Nevada and Peninsular Ranges, California (e.g., DePaolo, 1981a;Pickett and Saleeby, 1993); Fiordland, New Zealand (e.g., Klepeis et al, 2003) and 2) seismic studies exemplified by Main Ethiopian Rift (e.g., Keranen et al, 2004) and Western United States (e.g., McCarthy and Thompson, 1988). However, while useful, these observations provide a limited picture of the temporal history of lower crustal magmas.…”