WASHINGTON - Scientists have discovered a striking similarity between certain ocean currents on Earth and the bands that characterize the surface of large, gaseous planets like Jupiter. Boris Galperin of the University of South Florida's College of Marine Science in Saint Petersburg and colleagues in the United States, Israel, and Japan report their findings later this month in Geophysical Research Letters, published by the American Geophysical Union.

"The banded structure of Jupiter has long been a subject of fascination and intensive research," says Galperin, a physical oceanographer who analyzes turbulence theory and applies theory and numerical modeling to analyze planetary processes. "The visible bands on Jupiter are formed by clouds moving along a stable set of alternating flows."

Galperin and his colleagues have discovered that oceans on Earth also harbor stable alternating bands of current that, when modeled, are similar to the bands on Jupiter, due to the same kinds of "jets." "We think this resemblance is more than just visual," says Galperin. "The energy spectrum of the oceanic jets obeys a power law that fits the spectra of zonal flows on the outer planets."

The observation begs the question of whether these similar phenomena are rooted in similar physical forces. "To answer this question," says Galperin, "one needs to determine what physical processes govern the large-scale dynamics in both systems."

According to Galperin, there is a similarity in the forcing agents for planetary and oceanic circulations. The study maintains that both sets of zonal jets -- the ocean's bands of currents and the bands of Jupiter's clouds - are the result of an underlying turbulent flow regime common in nature.

Comparing the energy spectra on giant planets and in Earth's oceans can yield valuable information about the transport properties of the oceans, says Galperin, especially about the strongest currents in the mid-depth ocean. "The implications of these findings for climate research on Earth and the designs of future outer space observational studies are important," he says.

The study was funded by the U.S. Army Research Office and the Israel Science Foundation.

Notes for Journalists

Journalists (only) may obtain a pdf copy of this paper upon request to Harvey Leifert: hleifert@agu.org. Please provide your name, name of publication, phone, and email address. The paper and this press release are not under embargo.

Title: "The ubiquitous zonal jets in the atmosphere of giant planets and Earth's oceans"

Authors:
  • Boris Galperin, College of Marine Science, University of South Florida, St. Petersburg, Florida, USA
  • Hideyuki Nakano, Oceanographic Research Department, Meteorological Research Institute, Tsukuba, Ibaraki, Japan
  • Huei-Ping Huang, Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York, USA
  • Semion Sukorianski, Department of Mechanical Engineering/Perlstone Center for Aeronautical Engineering Studies, Ben-Gurion University of the Negev, Beer-Sheva, Israel

Citation: Galperin, B., H. Nakano, H-P. Huang, and S. Sukorianski (2004), The ubiquitous zonal jets in the atmosphere of giant planets and Earth's oceans, Geophys. Res. Lett., 31 [To come], doi:10/1029/2004GL 019691.

Contact information for authors:
Boris Galperin: +1 (727) 553-1249 or bgalperin@marine.usf.edu
[NOTE: Prof. Galperin will be in the United Kingdom from June 21 through July 31. He will be checking his e-mail there. To call him in the U.K., please contact Randolph Fillmore at USF (phone and e-mail address are at top of this press release).]
Hideyuki Nakano: +81 29 853 8538 hnakano@mri jma.go.jp
Huei Ping Huang: +1 (845) 365 8582 or huei@ldeo.columbia.edu
Semion Sukorianski: +972 8 6477096 or semion@bgumail.bgu.ac.il

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