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

Statistically study the optimal local sources for cosmic ray nuclei and electron