In this paper finite-difference second-order accurate direct simulatio
ns have been used to investigate how the helicity density fluctuations
change when a turbulent pipe rotates about its axis. In this case the
rotation axis is parallel to the near wall vortical structures which
play a fundamental role on the wall friction and turbulence production
. The helicity density is the trace of the tensor gamma(ij)'=(upsilon(
i)'omega(j)') whose elements form the components of v' x omega'. When
the momentum equations are written in rotational form the turbulence e
nergy production term splits into two parts, one related to the convec
tion of the large scales and the other related to the energy cascade t
o the small scales. From data of direct simulations the changes of the
turbulent production term profile with the rotation have been explain
ed by the pdf of the v' x omega' components. The links between the cha
nges on the pdf of the v' x omega' and the modifications of the vortic
al structures have been also investigated. The joint pdf of the dissip
ation with the helicity density has shown that the dissipation is high
ly correlated with regions of very low helicity density in the non-rot
ating pipe. When the pipe rotates the helicity density increases and t
he dissipation decreases. Since a drag reduction is one of the results
of the background rotation, in this paper, it has been speculated tha
t the alignment between velocity and vorticity could be a common featu
re in drag reducing flows. (C) 1997 American Institute of Physics.