Circulation of perivisceral fluid in the sea urchin Lytechinus variegatus

The principal driving mechanism of perivisceral-fluid circulation was investigated in the echinoid Lytechinus variegatus by metal-clad hot-wire anemometry. Analysis of 23 flow profiles from 13 individuals collected from 1 to 3 m water depth at Tarpon Springs and Sarasota, Florida (USA) in 1984 indicates that for this species, the ciliated epithelium is an ineffective driving mechanism for mixing of the perivisceral fluid. Instead, the Aristotle's lantern is the major driving force of circulation of the perivisceral fluid, with velocity fluctuations of 1.5 mm s^-1 amplitude in the cavity center during intermittent periods of activity. These fluctuations rapidly decay as the ciliated surfaces are approached. Spectral analysis of velocity time-series reveals predominant energy-containing velocity fluctuations between 0.007 and 0.05 Hz. The circulation, which can be described as non-turbulent forced mixing, has revealed four different flow patterns which appear to be correlated with specific animal activities. A modified eddydiffusion model predicts that oxygen transport through the cavity over a 2 cm path length requires more than 20 h. Calculation of the oxygen flux to a ripe ovary suggests that supply does not meet ovarian oxygen demand in this case. Alternative pathways of oxygen transport invoking advection in perivisceral-fluid eddies and along the ciliated coelomic surfaces are compatible with the observed flow patterns and lead to much shorter oxygen-transport time scales of the order of 1 to 10 min.