  The local sources, such as Geminga SNR, may play important role for the
anomaly of proton, electron and anisotropy in the past works. In fact, there
exists twelve SNRs around solar system within $1$ kpc. One question is that can
other SNRs also possibly contribute the spectra of nuclei and electron and
explain the special structure of anisotropy? In this work, under the
spatial-dependent propagation, we systematically study the contribution of all
local SNRs within 1 kpc around solar to the spectra of nuclei and electron, as
well as the energy dependence of anisotropy. As a result, only Geminga,
Monogem, and Vela SNRs have quantitive contribution to the nuclei and electron
spectra and anisotropy. Here, Geminga SNR is the sole optimal candidate and
Monogem SNR is controversial due to the tension of anisotropy between model
calculation and observations. The Vela SNR contributes a new spectral structure
beyond TeV energy, hinted by HESS, VERITAS, DAMPE and CALET measurements. More
interesting is that the electron anisotropy satisfies the Fermi-LAT limit below
TeV energy, but rises greatly and reaches $10\%$ at several TeV. This new
structure will shed new light to check our model. We hope that the new
structure of electron spectrum and anisotropy can be observed by space-borne
DAMPE and HERD and ground-based HAWC and LHAASO experiments in the near future.
