Investigating how the cutoff energy $E_{rm cut}$ varies with X-ray flux and photon index $Gamma$ in individual AGNs opens a new window to probe the yet unclear coronal physics. So far $E_{rm cut}$ variations have only been detected in several AGNs but different patterns have been reported. Here we report new detections of $E_{rm cut}$ variations in two Seyfert galaxies with multiple NuSTAR exposures. While in NGC 3227 $E_{rm cut}$ monotonically increases with $Gamma$, the $E_{rm cut}$-$Gamma$ relation exhibits a $Lambda$ shape in SWIFT J2127.4+5654 ($E_{rm cut}$ increasing with $Gamma$ at $Gamma$ $lesssim$ 2.05, but reversely decreasing at $Gamma$ $gtrsim$ 2.05), indicating more than a single underlying mechanism is involved. Meanwhile both galaxies show softer spectra while they brighten in X-ray, a common phenomenon in Seyfert galaxies. Plotting all 7 AGNs with $E_{rm cut}$ variations ever reported with NuSTAR observations in the $E_{rm cut}$-$Gamma$ diagram, we find they could be unified with the $Lambda$ pattern. Although the sample is small and SWIFT J2127.4+5654 is the only source with $Gamma$ varying across the break point thus the only one exhibiting the complete $Lambda$ pattern in a single source, the discoveries shed new light on the coronal physics in AGNs. Possible underlying physical mechanisms are discussed.
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