  Commonly used boundary conditions in reconstructing $f(T)$ gravity from
holographic Ricci dark energy model (RDE) are found to cause some problem, we
therefore propose new boundary conditions in this paper. By reconstructing
$f(T)$ gravity from the RDE with these new boundary conditions, we show that
the new ones are better than the present commonly used ones since they can give
the physically expected information, which is lost when the commonly used ones
are taken in the reconstruction, of the resulting $f(T)$ theory. Thus, the new
boundary conditions proposed here are more suitable for the reconstruction of
$f(T)$ gravity.
