  Magnetic reconnection has been extensively shown to be a promising approach
to extract spinning black hole energy. In this paper, we focus on extracting
spinning wormhole energy via such mechanism. The study shows that it is indeed
possible to extract rotating energy from a spinning wormhole with small
regularization parameter $\ell$ of the central singularity. The efficiency and
power of the energy extraction are also evaluated. Quite different from the
Kerr black hole, the spin of the wormhole can take arbitrarily large value.
However, the increasing of wormhole spin not always improves the efficiency and
power of energy extraction. By further comparing with the Kerr black hole, we
find the wormhole is more efficient when the magnetic reconnection happens
within radial distance $r/M<1$. These studies reveal the features of extracting
spinning wormhole energy, and more underlying properties are expected to be
disclosed for the horizonless objects.
