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A spatially homogeneous and anisotropic Bianchi type I universe is studiedwith the interacting holographic and new agegraphic scalar fields models ofdark energy.  Given, the framework of the anisotropic model, both the dynamics andpotential of these scalar field models according to the evolutionary behaviorof both dark energy models are reconstructed. We also investigate thecosmological evolution of interacting dark energy models, and compare it withobservational data and schematic diagram.  In order to do so, we focus on observational determinations of the expansionhistory $H(z)$. Next, we evaluate effects of anisotropy on various topics, suchas evolution of the growth of perturbations in the linear regime, statefinderdiagnostic, Sandage-Loeb (SL) test and distance modulus from holographic andnew agegraphic dark energy models and compare the results with standard FRW and$\Lambda$CDM and $w$CDM models.  Our numerical result show the effects of the interaction and anisotropy onthe evolutionary behavior the new agegraphic scalar field models

Effects of low anisotropy on interacting holographic and new agegraphic scalar fields models of dark energy