Fig. 4: Chemical distribution of Fe/Ni/Co.
From: Pinpointing the thermal history of lunar basaltic meteorites in a nutshell
a TEM-EDS (Kα) Ni map and Fe/Ni/Co profiles (AA’) of the bleb shown in Fig. 1 illustrating the smooth compositional gradient from the core to the rim, disrupted only by retained fcc grains and the abrupt step between the core and the intermediate band (IB). The large white frame indicates the location of Fig. 1c. b Close-up Ni map and Fe/Ni/Co profiles showing the concentrations across the interface between two bcc grains of the core (BB’), and across the core and the intermediate band (CC’).
