Skip to main content
. Author manuscript; available in PMC: 2020 Aug 14.
Published in final edited form as: J Geophys Res Planets. 2017 Nov 21;122(12):2469–2488. doi: 10.1002/2017JE005331

Figure 4.

Figure 4.

Fourier transforms of EXAFS spectra, uncorrected for phase shift (ΔR) and offset for clarity. Modeled fits to the EXAFS spectra (gray series) were calculated using the R range from 1 to 3.4 Å. For each composition, dotted lines corresponding to positions of Fe-O and Fe-(Fe,Mg,Al,Si) shells in untreated smectite are included for reference. k3-weighted EXAFS spectra (prior to Fourier transform) are displayed in Figure S2.