On the Validity of the Sverdrup Balance in the Atlantic NECC
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The Mean Flow Field of the Tropical Atlantic Ocean
Deep-Sea Research II 46 (1999) 279—303 The mean flow field of the tropical Atlantic Ocean Lothar Stramma*, Friedrich Schott Institut fu( r Meereskunde, an der Universita( t Kiel, Du( sternbrooker Weg 20, 24105 Kiel, Germany Received 26 August 1997; received in revised form 31 July 1998 Abstract The mean horizontal flow field of the tropical Atlantic Ocean is described between 20°N and 20°S from observations and literature results for three layers of the upper ocean, Tropical Surface Water, Central Water, and Antarctic Intermediate Water. Compared to the subtropical gyres the tropical circulation shows several zonal current and countercurrent bands of smaller meridional and vertical extent. The wind-driven Ekman layer in the upper tens of meters of the ocean masks at some places the flow structure of the Tropical Surface Water layer as is the case for the Angola Gyre in the eastern tropical South Atlantic. Although there are regions with a strong seasonal cycle of the Tropical Surface Water circulation, such as the North Equatorial Countercurrent, large regions of the tropics do not show a significant seasonal cycle. In the Central Water layer below, the eastward North and South Equatorial undercurrents appear imbedded in the westward-flowing South Equatorial Current. The Antarcic Intermediate Water layer contains several zonal current bands south of 3°N, but only weak flow exists north of 3°N. The sparse available data suggest that the Equatorial Intermediate Current as well as the Southern and Northern Intermediate Countercurrents extend zonally across the entire equatorial basin. Due to the convergence of northern and southern water masses, the western tropical Atlantic north of the equator is an important site for the mixture of water masses, but more work is needed to better understand the role of the various zonal under- and countercur- rents in cross-equatorial water mass transfer. -
Fronts in the World Ocean's Large Marine Ecosystems. ICES CM 2007
- 1 - This paper can be freely cited without prior reference to the authors International Council ICES CM 2007/D:21 for the Exploration Theme Session D: Comparative Marine Ecosystem of the Sea (ICES) Structure and Function: Descriptors and Characteristics Fronts in the World Ocean’s Large Marine Ecosystems Igor M. Belkin and Peter C. Cornillon Abstract. Oceanic fronts shape marine ecosystems; therefore front mapping and characterization is one of the most important aspects of physical oceanography. Here we report on the first effort to map and describe all major fronts in the World Ocean’s Large Marine Ecosystems (LMEs). Apart from a geographical review, these fronts are classified according to their origin and physical mechanisms that maintain them. This first-ever zero-order pattern of the LME fronts is based on a unique global frontal data base assembled at the University of Rhode Island. Thermal fronts were automatically derived from 12 years (1985-1996) of twice-daily satellite 9-km resolution global AVHRR SST fields with the Cayula-Cornillon front detection algorithm. These frontal maps serve as guidance in using hydrographic data to explore subsurface thermohaline fronts, whose surface thermal signatures have been mapped from space. Our most recent study of chlorophyll fronts in the Northwest Atlantic from high-resolution 1-km data (Belkin and O’Reilly, 2007) revealed a close spatial association between chlorophyll fronts and SST fronts, suggesting causative links between these two types of fronts. Keywords: Fronts; Large Marine Ecosystems; World Ocean; sea surface temperature. Igor M. Belkin: Graduate School of Oceanography, University of Rhode Island, 215 South Ferry Road, Narragansett, Rhode Island 02882, USA [tel.: +1 401 874 6533, fax: +1 874 6728, email: [email protected]]. -
The Decadal Mean Ocean Circulation and Sverdrup Balance
Journal of Marine Research, 69, 417–434, 2011 The decadal mean ocean circulation and Sverdrup balance by Carl Wunsch1 ABSTRACT Elementary Sverdrup balance is tested in the context of the time-average of a 16-year duration time-varying ocean circulation estimate employing the great majority of global-scale data available between 1992 and 2007. The time-average circulation exhibits all of the conventional major features as depicted both through its absolute surface topography and vertically integrated transport stream function. Important small-scale features of the time average only become apparent, however, in the time-average vertical velocity, whether near the surface or in the abyss. In testing Sverdrup balance, the requirement is made that there should be a mid-water column depth where the magnitude of the vertical velocity is less than 10−8 m/s (about 0.3 m/year displacement). The requirement is not met in the Southern Ocean or high northern latitudes. Over much of the subtropical and lower latitude ocean, Sverdrup balance appears to provide a quantitatively useful estimate of the meridional transport (about 40% of the oceanic area). Application to computing the zonal component, by integration from the eastern boundary is, however, precluded in many places by failure of the local balances close to the coasts. Failure of Sverdrup balance at high northern latitudes is consistent with the expected much longer time to achieve dynamic equilibrium there, and the action of other forces, and has important consequences for ongoing ocean monitoring efforts. 1. Introduction The very elegant and powerful theories of the time-mean ocean circulation, treated as a laminar flow, remain of intense interest, despite the widespread recognition that the oceanic kinetic energy is dominated by the time variability. -
The Evolution and Demise of North Brazil Current Rings*
VOLUME 36 JOURNAL OF PHYSICAL OCEANOGRAPHY JULY 2006 The Evolution and Demise of North Brazil Current Rings* DAVID M. FRATANTONI Department of Physical Oceanography, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts PHILIP L. RICHARDSON Department of Physical Oceanography, Woods Hole Oceeanographic Institution, and Associated Scientists at Woods Hole, Woods Hole, Massachusetts (Manuscript received 27 May 2004, in final form 26 October 2005) ABSTRACT Subsurface float and surface drifter observations illustrate the structure, evolution, and eventual demise of 10 North Brazil Current (NBC) rings as they approached and collided with the Lesser Antilles in the western tropical Atlantic Ocean. Upon encountering the shoaling topography east of the Lesser Antilles, most of the rings were deflected abruptly northward and several were observed to completely engulf the island of Barbados. The near-surface and subthermocline layers of two rings were observed to cleave or separate upon encountering shoaling bathymetry between Tobago and Barbados, with the resulting por- tions each retaining an independent and coherent ringlike vortical circulation. Surface drifters and shallow (250 m) subsurface floats that looped within NBC rings were more likely to enter the Caribbean through the passages of the Lesser Antilles than were deeper (500 or 900 m) floats, indicating that the regional bathymetry preferentially inhibits transport of intermediate-depth ring components. No evidence was found for the wholesale passage of rings through the island chain. 1. Introduction ration from the NBC, anticyclonic rings with azimuthal speeds approaching 100 cm sϪ1 move northwestward a. Background toward the Caribbean Sea on a course parallel to the The North Brazil Current (NBC) is an intense west- South American coastline (Johns et al. -
Annual Cycle and Variability of the North Brazil Current
JANUARY 1998 JOHNS ET AL. 103 Annual Cycle and Variability of the North Brazil Current W. E. J OHNS AND T. N . L EE Rosenstiel School of Marine and Atmospheric Science, University of Miami, Miami, Florida R. C. BEARDSLEY,J.CANDELA, AND R. LIMEBURNER Woods Hole Oceanographic Institution, Woods Hole, Massachusetts B. CASTRO Instituto Oceanogra®co Universidade SaÄo Paulo, SaÄo Paulo, Brazil (Manuscript received 18 October 1996, in ®nal form 5 June 1997) ABSTRACT Current meter observations from an array of three subsurface moorings located on the Brazil continental slope near 48N are used to describe the annual cycle and low-frequency variability of the North Brazil Current (NBC). The moored array was deployed from September 1989 to January 1991, with further extension of the shallowest mooring, located over the 500-m isobath near the axis of the NBC, through September 1991. Moored current measurements were also obtained over the adjacent shelf for a limited time between February and May 1990. The NBC has a large annual cycle at this latitude, ranging from a maximum transport of 36 Sv (Sv [ 106 m3 s21) in July±August to a minimum of 13 Sv in April±May, with an annual mean transport of approximately 26 Sv. The mean transport is dominated by ¯ow in the upper 150 m, and the seasonal cycle is contained almost entirely in the top 300 m. Transport over the continental shelf is 3±5 Sv and appears to be fairly constant throughout the year, based on the available current meter records and shipboard ADCP surveys. The NBC transport cycle is in good agreement with linear wind-driven models and appears to be in near-equilibrium with remote wind stress curl forcing across the tropical Atlantic for much of the year. -
(Potential) Vorticity: the Swirling Motion of Geophysical Fluids
(Potential) vorticity: the swirling motion of geophysical fluids Vortices occur abundantly in both atmosphere and oceans and on all scales. The leaves, chasing each other in autumn, are driven by vortices. The wake of boats and brides form strings of vortices in the water. On the global scale we all know the rotating nature of tropical cyclones and depressions in the atmosphere, and the gyres constituting the large-scale wind driven ocean circulation. To understand the role of vortices in geophysical fluids, vorticity and, in particular, potential vorticity are key quantities of the flow. In a 3D flow, vorticity is a 3D vector field with as complicated dynamics as the flow itself. In this lecture, we focus on 2D flow, so that vorticity reduces to a scalar field. More importantly, after including Earth rotation a fairly simple equation for planar geostrophic fluids arises which can explain many characteristics of the atmosphere and ocean circulation. In the lecture, we first will derive the vorticity equation and discuss the various terms. Next, we define the various vorticity related quantities: relative, planetary, absolute and potential vorticity. Using the shallow water equations, we derive the potential vorticity equation. In the final part of the lecture we discuss several applications of this equation of geophysical vortices and geophysical flow. The preparation material includes - Lecture slides - Chapter 12 of Stewart (http://www.colorado.edu/oclab/sites/default/files/attached- files/stewart_textbook.pdf), of which only sections 12.1-12.3 are discussed today. Willem Jan van de Berg Chapter 12 Vorticity in the Ocean Most of the fluid flows with which we are familiar, from bathtubs to swimming pools, are not rotating, or they are rotating so slowly that rotation is not im- portant except maybe at the drain of a bathtub as water is let out. -
Arxiv:1809.01376V1 [Astro-Ph.EP] 5 Sep 2018
Draft version March 9, 2021 Typeset using LATEX preprint2 style in AASTeX61 IDEALIZED WIND-DRIVEN OCEAN CIRCULATIONS ON EXOPLANETS Weiwen Ji,1 Ru Chen,2 and Jun Yang1 1Department of Atmospheric and Oceanic Sciences, School of Physics, Peking University, 100871, Beijing, China 2University of California, 92521, Los Angeles, USA ABSTRACT Motivated by the important role of the ocean in the Earth climate system, here we investigate possible scenarios of ocean circulations on exoplanets using a one-layer shallow water ocean model. Specifically, we investigate how planetary rotation rate, wind stress, fluid eddy viscosity and land structure (a closed basin vs. a reentrant channel) influence the pattern and strength of wind-driven ocean circulations. The meridional variation of the Coriolis force, arising from planetary rotation and the spheric shape of the planets, induces the western intensification of ocean circulations. Our simulations confirm that in a closed basin, changes of other factors contribute to only enhancing or weakening the ocean circulations (e.g., as wind stress decreases or fluid eddy viscosity increases, the ocean circulations weaken, and vice versa). In a reentrant channel, just as the Southern Ocean region on the Earth, the ocean pattern is characterized by zonal flows. In the quasi-linear case, the sensitivity of ocean circulations characteristics to these parameters is also interpreted using simple analytical models. This study is the preliminary step for exploring the possible ocean circulations on exoplanets, future work with multi-layer ocean models and fully coupled ocean-atmosphere models are required for studying exoplanetary climates. Keywords: astrobiology | planets and satellites: oceans | planets and satellites: terrestrial planets arXiv:1809.01376v1 [astro-ph.EP] 5 Sep 2018 Corresponding author: Jun Yang [email protected] 2 Ji, Chen and Yang 1. -
Ocean Circulation and Climate: a 21St Century Perspective
Chapter 13 Western Boundary Currents Shiro Imawaki*, Amy S. Bower{, Lisa Beal{ and Bo Qiu} *Japan Agency for Marine–Earth Science and Technology, Yokohama, Japan {Woods Hole Oceanographic Institution, Woods Hole, Massachusetts, USA {Rosenstiel School of Marine and Atmospheric Science, University of Miami, Miami, Florida, USA }School of Ocean and Earth Science and Technology, University of Hawaii, Honolulu, Hawaii, USA Chapter Outline 1. General Features 305 4.1.3. Velocity and Transport 317 1.1. Introduction 305 4.1.4. Separation from the Western Boundary 317 1.2. Wind-Driven and Thermohaline Circulations 306 4.1.5. WBC Extension 319 1.3. Transport 306 4.1.6. Air–Sea Interaction and Implications 1.4. Variability 306 for Climate 319 1.5. Structure of WBCs 306 4.2. Agulhas Current 320 1.6. Air–Sea Fluxes 308 4.2.1. Introduction 320 1.7. Observations 309 4.2.2. Origins and Source Waters 320 1.8. WBCs of Individual Ocean Basins 309 4.2.3. Velocity and Vorticity Structure 320 2. North Atlantic 309 4.2.4. Separation, Retroflection, and Leakage 322 2.1. Introduction 309 4.2.5. WBC Extension 322 2.2. Florida Current 310 4.2.6. Air–Sea Interaction 323 2.3. Gulf Stream Separation 311 4.2.7. Implications for Climate 323 2.4. Gulf Stream Extension 311 5. North Pacific 323 2.5. Air–Sea Interaction 313 5.1. Upstream Kuroshio 323 2.6. North Atlantic Current 314 5.2. Kuroshio South of Japan 325 3. South Atlantic 315 5.3. Kuroshio Extension 325 3.1. -
Geophysical Fluid Dynamics, Nonautonomous Dynamical Systems, and the Climate Sciences
Geophysical Fluid Dynamics, Nonautonomous Dynamical Systems, and the Climate Sciences Michael Ghil and Eric Simonnet Abstract This contribution introduces the dynamics of shallow and rotating flows that characterizes large-scale motions of the atmosphere and oceans. It then focuses on an important aspect of climate dynamics on interannual and interdecadal scales, namely the wind-driven ocean circulation. Studying the variability of this circulation and slow changes therein is treated as an application of the theory of nonautonomous dynamical systems. The contribution concludes by discussing the relevance of these mathematical concepts and methods for the highly topical issues of climate change and climate sensitivity. Michael Ghil Ecole Normale Superieure´ and PSL Research University, Paris, FRANCE, and University of California, Los Angeles, USA, e-mail: [email protected] Eric Simonnet Institut de Physique de Nice, CNRS & Universite´ Coteˆ d’Azur, Nice Sophia-Antipolis, FRANCE, e-mail: [email protected] 1 Chapter 1 Effects of Rotation The first two chapters of this contribution are dedicated to an introductory review of the effects of rotation and shallowness om large-scale planetary flows. The theory of such flows is commonly designated as geophysical fluid dynamics (GFD), and it applies to both atmospheric and oceanic flows, on Earth as well as on other planets. GFD is now covered, at various levels and to various extents, by several books [36, 60, 72, 107, 120, 134, 164]. The virtue, if any, of this presentation is its brevity and, hopefully, clarity. It fol- lows most closely, and updates, Chapters 1 and 2 in [60]. The intended audience in- cludes the increasing number of mathematicians, physicists and statisticians that are becoming interested in the climate sciences, as well as climate scientists from less traditional areas — such as ecology, glaciology, hydrology, and remote sensing — who wish to acquaint themselves with the large-scale dynamics of the atmosphere and oceans. -
The Sargassum Invasion of the Eastern Caribbean and Dynamics of the Equatorial North Atlantic
The Sargassum Invasion of the Eastern Caribbean and Dynamics of the Equatorial North Atlantic Invasión de Sargazo en el Caribe Oriental y la Dinámica en la Zona Ecuatorial del Atlántico Norte L'Invasion de Sargasse dans les Caraïbes Orientales et leur Dynamique dans la Partie Nord de l'Atlantique Ėquatorial DONALD R. JOHNSON1*, DONG S. KO2, JAMES S. FRANKS1, PAULA MORENO1, and GUILLERMO SANCHEZ-RUBIO1 1Center for Fisheries Research and Development, Gulf Coast Research Laboratory, University of Southern Mississippi, Ocean Springs, Mississippi 39564 USA. *[email protected]. [email protected]. [email protected]. [email protected]. 2Ocean Dynamics and Prediction Branch, Naval Research Laboratory, Stennis Space Center, Mississippi 39529 USA. [email protected]. EXTENDED ABSTRACT In the spring and summer of 2011, unprecedented quantities of pelagic sargassum came ashore on many islands of the eastern Caribbean (Figure 1), seriously affecting fishery and tourism industries. Concurrently, pelagic sargassum also washed ashore in massive amounts along the coasts of western Africa (Sierra Leone and Benin) and was spotted in large mats by aircraft off northern Brazil (Széchy et al. 2012). Two species were identified in the invasion: Sargassum natans and Sargassum fluitans, both of which coexist throughout the North Atlantic with large mats and long lines commonly found in the Sargasso Sea (Winge 1923) and in the northern Gulf of Mexico (Comyns et al. 2002). Using satellite tracked mixed- layer drifters during 2010 and 2011 we were unable to connect the Caribbean invasion to the central North Atlantic and the Sargasso Sea. However, from archived results of a numerical circulation model (HYCOM), back-tracking from where landfalls were reported suggested that the sargassum may have bloomed in the north equatorial recirculation region (NERR) where conditions in the spring/summer of 2010 were conducive to growth and consolidation. -
Atlantic Ocean Equatorial Currents
188 ATLANTIC OCEAN EQUATORIAL CURRENTS ATLANTIC OCEAN EQUATORIAL CURRENTS S. G. Philander, Princeton University, Princeton, Centered on the equator, and below the westward NJ, USA surface Sow, is an intense eastward jet known as the Equatorial Undercurrent which amounts to a Copyright ^ 2001 Academic Press narrow ribbon that precisely marks the location of doi:10.1006/rwos.2001.0361 the equator. The undercurrent attains speeds on the order of 1 m s\1 has a half-width of approximately Introduction 100 km; its core, in the thermocline, is at a depth of approximately 100 m in the west, and shoals to- The circulations of the tropical Atlantic and PaciRc wards the east. The current exists because the west- Oceans have much in common because similar trade ward trade winds, in addition to driving divergent winds, with similar seasonal Suctuations, prevail westward surface Sow (upwelling is most intense at over both oceans. The salient features of these circu- the equator), also maintain an eastward pressure lations are alternating bands of eastward- and west- force by piling up the warm surface waters in the ward-Sowing currents in the surface layers (see western side of the ocean basin. That pressure force Figure 1). Fluctuations of the currents in the two is associated with equatorward Sow in the thermo- oceans have similarities not only on seasonal but cline because of the Coriolis force. At the equator, even on interannual timescales; the Atlantic has where the Coriolis force vanishes, the pressure force a phenomenon that is the counterpart of El Ninoin is the source of momentum for the eastward Equa- the PaciRc. -
Brazil Shelf LME (Sea Around Us 2006)
Sustainable Management of the Shared Living Marine Resources of the Caribbean Sea Large Marine Ecosystem (CLME) and Adjacent Regions Caribbean Large Marine Ecosystem Regional Transboundary Diagnostic Analysis - DRAFT - May 2011 Table of contents 1. EXECUTIVE SUMMARY ...................................................................................................... 8 2. INTRODUCTION .................................................................................................................. 16 2.1. BACKGROUND TO THE CLME REGION ............................................................................ 16 2.1.1. Global and regional significance of the CLME .............................................................. 16 2.1.2. Purpose of the Transboundary Diagnostic Analysis ...................................................... 18 2.2. STRUCTURE OF REGIONAL TDA ...................................................................................... 19 3. METHODOLOGY ................................................................................................................. 20 3.1. INTRODUCTION ................................................................................................................ 20 3.2. SUMMARY OF THE PRELIMINARY TDA (2007) ................................................................ 20 3.3. APPROACH ADOPTED FOR THE CLME TDA .................................................................... 21 3.3.1. Background ....................................................................................................................