  We study the model-independent traversable wormholes from cosmological
reconstruction based on Gaussian processes (GP). Using a combination of Union
2.1 SNe Ia data, the latest observational Hubble parameter data and recent
Planck's shift parameter, we find that our GP method can give a tighter
constraint on the normalized comoving distance, its derivatives and the dark
energy equation of state than the previous work \cite{1}. Subsequently, two
specific traversable wormhole solutions are obtained, i.e., the cases of a
constant redshift function and a linear shape function. We find that, with
decreasing cosmic acceleration, the traversal velocity $v$ of the former case
increases and the amounts of exotic matter $I_V$ of the latter case decreases.
