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We present postprocess AGB nucleosynthesis models with different C-pocket internal structures to better explain zirconium isotope measurements in mainstream presolar SiC grains by Nicolussi et al. (1997) and Barzyk et al. (2007). We show that higher-than-solar Zr/Zr ratios can be predicted by adopting a C-pocket with a flat C profile, instead of the previous decreasing-with-depth C profile. The improved agreement between grain data for zirconium isotopes and AGB models provides additional support for a recent proposal of a flat C profile based on barium isotopes in mainstream SiC grains by Liu et al. (2014).

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