  Recent observations of cosmic rays (CRs) have revealed a two-component
anomaly in the spectra of primary and secondary particles, as well as their
ratios, prompting investigation into their common origin. In this study, we
incorporate the identification of slow diffusion zones around sources as a
common phenomenon into our calculations, which successfully reproduces all
previously described anomalies except for the positron spectrum. Crucially, our
research offers a clear physical picture of the origin of CR: while high-energy
($\textrm{>200~GV}$, including the knee) particles are primarily produced by
fresh accelerators and are confined to local regions, low energy
($\textrm{<200~GV}$) components come from distant sources and travel through
the outer diffusive zone outside of the galactic disk. This scenario can be
universally applied in the galactic disk, as evidenced by ultra-high energy
diffuse $\rm\gamma$-ray emissions detected by the AS$\rm\gamma$ experiment.
Furthermore, our results predict that the spectrum of diffuse $\rm\gamma$-ray
is spatial-dependent, resting with local sources, which can be tested by LHAASO
experiment.
