“…Grain-scale to mesoscale melt topology studies mostly focus on anatectic high-temperature-medium-pressure regions that commonly show protracted episodes of melting (e.g., Sawyer, 2001;Brown and Solar, 1999;Hasalová et al, 2008aHasalová et al, , 2008bKisters et al, 2009;Bonamici and Duebendorfer, 2010;Sawyer, 2014;Kisters, 2012, 2016). In contrast, petrostructural studies of migmatitic UHP terranes have aimed to identify the incipient melting reactions close to the UHP conditions (e.g., Gordon et al, 2013;Chen et al, 2013Ganzhorn et al, 2014;Zhang et al, 2015;Stepanov et al, 2016), and rather neglected the grain-scale melt topology and deformation mechanisms with respect to the kinematic framework of their host.…”