The evolution of a single hairpin vortex-like structure in the mean turbule
nt field of a low-Reynolds-number channel flow is studied by direct numeric
al simulation. The structure of the initial three-dimensional vortex is ext
racted from the two-point spatial correlation of the velocity field by line
ar stochastic estimation given a second-quadrant ejection event vector. Ini
tial vortices having vorticity that is weak relative to the mean vorticity
evolve gradually into omega-shaped vortices that persist for long times and
decay slowly. As reported in Zhou, Adrian & Balachandar (1996), initial vo
rtices that exceed a threshold strength relative to the mean flow generate
new hairpin vortices upstream of the primary vortex. The detailed mechanism
s for this upstream process are determined, and they are generally similar
to the mechanisms proposed by Smith et al. (1991), with some notable differ
ences in the details. It has also been found that new hairpins generate dow
nstream of the primary hairpin, thereby forming, together with the upstream
hairpins, a coherent packet of hairpins that propagate coherently. This is
consistent with the experimental observations of Meinhart & Adrian (1995).
The possibility of autogeneration above a critical threshold implies that
hairpin vortices in fully turbulent fields may occur singly, but they more
often occur in packets. The hairpins also generate quasi-streamwise vortice
s to the side of the primary hairpin legs. This mechanism bears many simila
rities to the mechanisms found by Brooke & Hanratty (1993) and Bernard, Tho
mas & Handler (1993). It provides a means by which new quasi-streamwise vor
tices, and, subsequently, new hairpin vortices can populate the near-wall l
ayer.