Article Type:
Research Article

Lagrangian Observations of the Circulation in the Northern Gulf of California

M. F. Lavín Departamento de Oceanografía Física, CICESE, Ensenada, Baja California, Mexico

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R. Durazo Facultad de Ciencias Marinas, UABC, Ensenada, Baja California, Mexico

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E. Palacios Departamento de Oceanografía Física, CICESE, Ensenada, Baja California, Mexico

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M. L. Argote Departamento de Oceanografía Física, CICESE, Ensenada, Baja California, Mexico

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L. Carrillo Departamento de Oceanografía Física, CICESE, Ensenada, Baja California, Mexico

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Print Publication:
01 Oct 1997
DOI:
https://doi.org/10.1175/1520-0485(1997)027<2298:LOOTCI>2.0.CO;2
Page(s):
2298–2305
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Abstract

ARGOS drifters deployed in the Northern Gulf of California in September 1995 showed the presence of a cyclonic gyre, while a second deployment in March 1996 revealed an anticyclonic gyre. A circulation pattern consisting of a seasonally reversing gyre had been proposed before on the basis of satellite images, geostrophic calculations, and numerical models, but so far no direct observations have been made to test its existence. In September the gyre was cyclonic, baroclinic, very well defined, stable, and strong; its mean speed and rotation time were 0.3 m s−1 and ∼7 days. In March the gyre had the same mean speed, but it was anticyclonic and displaced to the northwest of the summer position. The March gyre has barotopic and baroclinic characteristics, but the observed speeds are stronger than in numerical simulations. These data and a data bank analysis suggest that the summer gyre is a persistent summer feature, but the winter–spring situation remains ill-defined and requires further research.

Corresponding author address: Dr. Miguel F. Lavín, CICESE-Oceanography, P.O. Box 434844, San Diego, CA 92143-4844.

Abstract

ARGOS drifters deployed in the Northern Gulf of California in September 1995 showed the presence of a cyclonic gyre, while a second deployment in March 1996 revealed an anticyclonic gyre. A circulation pattern consisting of a seasonally reversing gyre had been proposed before on the basis of satellite images, geostrophic calculations, and numerical models, but so far no direct observations have been made to test its existence. In September the gyre was cyclonic, baroclinic, very well defined, stable, and strong; its mean speed and rotation time were 0.3 m s−1 and ∼7 days. In March the gyre had the same mean speed, but it was anticyclonic and displaced to the northwest of the summer position. The March gyre has barotopic and baroclinic characteristics, but the observed speeds are stronger than in numerical simulations. These data and a data bank analysis suggest that the summer gyre is a persistent summer feature, but the winter–spring situation remains ill-defined and requires further research.

Corresponding author address: Dr. Miguel F. Lavín, CICESE-Oceanography, P.O. Box 434844, San Diego, CA 92143-4844.

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