Journal Highlights

What Happens When Ocean Eddies Hit a Wall?

Editors’ Highlight—Observing subsurface changes of two anticyclonic eddies passing over the Izu-Ogasawara Ridge

This study examines how submarine ridges create subsurface changes to ocean eddies. Looking specifically at two anticyclonic eddies in the North Pacific that migrate westward and encounter the Izu-Ogasawara Ridge, the authors analyze daily temperature and salinity data collected from Iridium Argo floats. Their analysis identifies changes in eddy vertical structure and diapycnal mixing as the eddies pass over the ridge. Mesoscale eddies play an important role in the mixing and redistribution of heat, salt and carbon, and also effect large-scale circulation and climate, so a better understanding of subsurface eddy-bathymetry interactions is valuable for climate research and forecasting.

From Research Spotlights—What Happens When Ocean Eddies Hit a Wall?

A new study tracks two ocean eddies passing over the Pacific Ocean’s Izu-Ogasawara Ridge. 

Spanning tens to hundreds of kilometers, mesoscale eddies spiral and swirl across the ocean, transporting just as much water as wind or deeper currents. Although scientists have long studied them from above by satellite, their 3-D motion is more difficult to track as they move over the seafloor and encounter undersea mountains and ravines. 

To observe these hidden dynamics, scientists deploy buoyant bobbers called Argo floats, which trail sensors at different depths. Now, by dropping 17 Argo floats into a clockwise eddy east of Japan, Xu et al. have captured what happens when such an eddy hits the Izu-Ogasawara Ridge, a stretch of undersea mountains roughly north of the Marianas Trench

The authors dropped the floats in the southwest moving eddy in March 2014. Several of the floats remained caught in the eddy for months, until the vortex reached the Izu-Ogasawara Ridge in late September and finally dissipated. Several other floats escaped the first eddy and got trapped in a second one, farther east. When this eddy encountered the ridge, it passed over it, and the floats became entrained in the current for nearly a year, until the current diminished in May 2015. 

In total, the team collected more than 5000 data points on the two eddies, monitoring their structure and movement down to more than 1000 meters deep. As both eddies hit the ridge, they “domed up,” increasing in diameter, the team reports. 

The eddies formed underwater structures known as Taylor columns, a phenomenon in fluid dynamics that occurs when rotating fluids encounter an obstacle and form a column of stagnant water above it. Despite all the turbulence happening deep underwater, the upper 200 meters of ocean remained largely unperturbed as the eddies hit the ridge, the team found. 

The authors note that studying the dynamics of such eddies could help scientists better predict how they distribute heat, salt, and carbon throughout the globe.

-- Emily Underwood, Freelance Writer,


Recent Highlights Across AGU Publications Earth & Space Science News

View more Earth and space science news from Eos

Download the App

New Android App Available!

Google Play Store Logo

Download the Geophysical Research Letters app from the Google Play Store

iOS App for iPad or iPhone


Download the Geophysical Research Letters app from the Apple store

AGU Career Center

AGU Unlocked

Featured Special Collection

Early Results: Juno at Jupiter 

Early results from Juno's mission at Jupiter including approach to Jupiter and the first perijove pass (PJ1). Juno's scientific objectives include the study of Jupiter's interior, atmosphere and polar magnetosphere with the goal of understanding Jupiter's origin, formation and evolution. This collection of papers provides early results from Juno's measurements of the gravity and magnetic fields, deep atmospheric microwave sounding, infrared, visible and ultraviolet images/spectra and an array of fields and particles instruments as well as context for the early results with respect to current theory and models of Jupiter's formation and evolution. Topics include both Juno - Jupiter related theoretical models and data analysis as well as collaborative observations made from Earth based assets.