Vertical Nitrate Flux Induced by Kelvin-Helmholtz Billows Over a Seamount in the Kuroshio

Kelvin-Helmholtz (KH) billows can facilitate microscale turbulent mixing around seamounts in the Kuroshio. This study sought to describe the influence of billow intensity (i.e., intermittent and small and steady and large billows) on vertical nitrate fluxes. KH billows led to turbulent kinetic energy dissipation rates [epsilon = O (10(-7) to 10(-6)) W kg(-1)] and eddy diffusivities [K-rho = O (10(-4) to 10(-3)) m(2) s(-1)] that were significantly stronger than those outside the billow depths. The mean nitrate flux estimated using K-rho in the billow depths had a maximal value of 10.0 mmol m(-2) day(-1), which was much higher than estimates for the open ocean. The nitrate flux associated with the shallow KH billows at two vertical levels contributed to enrich the subsurface phytoplankton maximum, while the deeper billows closer to the summit were found to induce a large amount of nitrate flux from the deeper to the subsurface water. This study showed that KH billows make important contributions to seamount ecosystems, particularly in the cycling and vertical mixing of nutrients to make them available for potential downstream transport.

Automated summary

The study shows that Kelvin-Helmholtz billows play a significant role in influencing vertical nitrate fluxes and promoting microscale turbulent mixing around seamounts in the Kuroshio. Billow intensity affects nitrate fluxes, with higher values found in the billow depths contributing to the growth of phytoplankton communities. The depth and proximity of the billows to the seafloor also impact the distribution of nitrate fluxes.