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JOURNALOFGEOPHYSICALRESEARCH,VOL.X,XXXX,DOI:10.1029/2016JGRXXXXX,2016 The life cycle of a coherent Lagrangian Agulhas ring Y. Wang1, F. J. Beron-Vera2 and M. J. Olascoaga1 Abstract. We document the long-term evolution of an Agulhas ring detected from satel- lite altimetry using a technique from nonlinear dynamical systems that enables objec- tive (i.e., observer-independent) eddy framing. Such objectively detected eddies have La- grangian (material) boundaries that remain coherent (unfilamented) over the detection period. The ring preserves a quite compact material entity for a period of about 2 years even after most initial coherence is lost within 5 months after detection. We attribute 6 this to the successive development of short-term coherent material boundaries around 1 the ring. These boundaries provide effective short-term shielding for the ring, which pre- 0 vents a large fraction of the ring’s interior from being mixed with the ambient turbu- 2 lent flow. We show that such coherence regain events cannot be inferred from Eulerian n analysis. This process is terminated by a ring-splitting event which marks the ring demise, a near the South American coast. The genesis of the ring is characterized by a ring-merging J event away from the Agulhas retroflection, followed by a 4-month-long partial coherence 7 stage, scenario that is quite different than a simple current occlusion and subsequent eddy pinch off. ] h p 1. Introduction the Cape Basin, which is in line with the fast decay of the - o ring’s SSH anomaly amplitude. Beyond the Walvis Ridge a a The long-term ability of Agulhas rings detected from large fraction of the ring (about 6×104 km3, correspond- . satellitealtimetrymeasurementsofseasurfaceheight(SSH) ing to a 2-km-deep, 200-km-diameter ring) is observed to s to maintain Lagrangian (i.e., material) coherence has been preserve a compact Lagrangian entity far beyond the the- c i demonstrated using satellite ocean color imagery [Lehahn oretical Lagrangian coherence horizon. This is shown to s et al., 2011]. This suggests a long-term transport ability becausedbysuccessiveshort-termcoherenceregainevents. y for such rings, which has been the subject of recent inves- Demise of the ring eventually occurs, triggered by a ring h tigation using nonlinear dynamical systems techniques that splitting event, after a rapid decay of the area enclosed by p enable objective (i.e., observer-independent) framing of La- theshort-termcoherentLagrangianloopsthatprovidedthe [ grangiancoherence. Usingtheovertwo-decade-longaltime- interiorfluidshieldingfromturbulentmixingwiththeambi- 1 tryrecord,Wangetal.[2015]foundthatlong-lived(ofupto entfluidalongtheringpath. Notalloftheseaspectsofthe v atleast1yearofduration)ringshavesmall(about50kmin evolution of the ring are inferable from Eulerian analysis of 0 diameter)coherentLagrangiancores,suggestingafastdecay SSH, which although signals coherence gain upon crossing 6 fortherings. Ontheotherhand,theyfoundthatsuchcores theWalvisRidge,suggestsslowdecaythereafter. Itisnoted 5 carry a small (about 30%) fraction of water traceable into finally that even if this behavior generalizes to all Agulhas 1 the Indian Ocean. The two findings together question the rings,whichneedstobeverified,theirlong-rangetransport 0 long-range ability of rings in transporting Agulhas leakage. ability is still limited. . In turn, Froyland et al. [2015] found that the rings decay The rest of the paper is organized as follows. Geodesic 1 slowly, enabling long-range Agulhas leakage transport, and eddy detection is briefly reviewed in Section 2, which con- 0 thatthisisinferablefromtheEulerianfootprintsoftherings tains basic information of the altimetry dataset and some 6 on SSH. numerical details. The life cycle of the ring is described 1 The goal of the present paper is to bridge the gap be- in Sections 3–5. Implications for transport are discussed in : tweentheaboveseeminglycontradictingresultsbycarrying Section 6. Finally, Section 7 includes concluding remarks. v out a detailed objective investigation of the genesis, evolu- i X tion, and decay of the ring priorly investigated by Froyland et al. [2015]. This is done using Haller and Beron-Vera’s 2. Geodesic eddy detection r [2013; 2014] technique, which enables optimal detection of a rings with Lagrangian boundaries that exhibit no signs of We are concerned with fluid regions enclosed by excep- filamentation over the coherence assessment time interval. tional material loops that defy the exponential stretching Lagrangian coherence is found to emerge quite sponta- that a typical loop will experience in turbulent flow. As neouslyfromturbulence,processthatdiffersfromtheideal- Haller and Beron-Vera [2013, 2014] have shown, such loops ized scenario in which an Agulhas ring forms as a result of have small annular neighborhoods exhibiting no leading- the occlusion of, and subsequent pinch off from, the Agul- order variation in averaged material stretching. hasretroflection. Thisinitialcoherenceisrapidlylostwithin 1DepartmentofOceanSciences,RosenstielSchoolofMarineandAtmosphericScience,UniversityofMiami,Miami,Florida, USA. 2DepartmentofAtmosphericSciences,RosenstielSchoolofMarineandAtmosphericScience,UniversityofMiami,Miami, Florida,USA. Copyright2016bytheAmericanGeophysicalUnion. 0148-0227/16/2016JGRXXXXX$9.00 1 X - 2 WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING Morespecifically,solvingthisvariationalproblemreveals 2013,2014;Beron-Veraetal.,2015;Wangetal.,2015;Kar- that the loops in question are uniformly stretching: any of rasch et al.,2014]andasoftwaretoolisnowavailable[Onu their subsets are stretched by the same factor λ under ad- et al., 2015]. Here we set the grid width of the computa- vection by the flow from time t to time t. The time t tionaldomainto0.1kmcontainingthering,whichenabled 0 0 positionsofλ-stretchingmaterialloopsturnouttobelimit us to push the Lagrangian coherence detectability horizon cycles of one of the following two equations for parametric close to 1.5 years. All integrations were carried out using a curves s(cid:55)→x (s): step-adaptingfourth/fifth-orderRunge–Kuttamethodwith 0 interpolations done with a cubic method. (cid:115) (cid:115) dx λ (x )−λ2 λ2−λ (x ) ds0 = λ (x2 )0−λ (x )ξ1(x0)± λ (x )−1λ (0x )ξ2(x0). 3. Lagrangian coherence detection 2 0 1 0 2 0 1 0 (1) Here λ (x ) < λ2 < λ (x ), where {λ (x )} and {ξ (x )}, Webeginbyapplyinggeodesiceddydetectionont0 =31 1 0 2 0 i 0 i 0 March 1999, date by which the ring in question is in a suf- satisfying ficiently mature Lagrangian coherence stage. On that date 1 the ring is found inside the region indicated by the square 0<λ1(x0)≡ λ (x ) <1, ξi(x0)·ξj(x0)=δij i,j =1,2, in the left panel of Fig. 1a. Geodesic eddy detection was 2 0 carried out over t through t = t +T for Lagrangian co- (2) 0 0 herence time scale T increasing from 30 d in steps of 30 d are eigenvalues and (normalized) eigenvectors, respectively, out to 480 d, the longest T from which it was possible to of the Cauchy–Green tensor, extract a coherent Lagrangian eddy boundary. This is a very long Lagrangian coherence time scale, consistent with Ct (x ):=DFt (x )(cid:62)DFt (x ), (3) t0 0 t0 0 t0 0 thestatementabovethattheringisinamatureLagrangian coherencestageonthedetectiondate. Infact,buildingma- an objective (i.e., independent of the observer) measure of terial coherence takes a few months, as we show in Section material deformation, where Ft : x (cid:55)→ x(t;x ,t ) is the t0 0 0 0 5. Application of geodesic eddy detection as just described flow map that takes time t positions to time t positions of 0 resulted in a nested family of Lagrangian boundaries with fluid particles, which obey coherence time scale increasing inward. Theextractedboundariesareindicatedinredonthede- dx =v(x,t), (4) tection date in Fig. 1a (the right panel shows a blow-up dt of the region indicated by the rectangle in the left panel). For each T considered there is a nested family of λ-loops; where v(x,t) is a divergenceless two-dimensional velocity the loop shown is the outermost one in each family. For field. T between 30 and 210 d the loops have λ = 1; for T in- Limitcyclesof (1)eithergroworshrinkunderchangesin creasing from 210 d, λ increases from 1.05 to 1.75. Thus λ,formingsmoothannularregionsofnonintersectingloops. as T increases the largest fluid area enclosed by a coherent The outermost member of such a band of material loops material loop shrinks and the ability of a loop to reassume is observed physically as the boundary of a coherent La- itsinitialarclengthdiminishes,reflectingthattheringturns grangian eddy. Limit cycles of (1) tend to exist only for unstable after a sufficiently long time. λ ≈ 1. Material loops characterized by λ = 1 resist the The outer, shorter-lived boundaries provide a shield to universallyobservedmaterialstretchinginturbulence: they the inner, longer-lived boundaries surrounding the core of reassume their initial arclength at time t. This conser- the coherent Lagrangian ring. This is evident in the suc- vation of arclength, along with enclosed area preservation cessive advected images of the boundaries under the flow. (whichholdsbyassumption),producesextraordinarycoher- These are shown in Figs. 1b–f on selected dates over more ence[Beron-Veraetal.,2013]. Finally,limitcyclesof (1)are than 2 years of evolution (an animation including monthly (null) geodesics of the generalized Green–Lagrange tensor snapshots is supplied as supporting information Movie 1 at Ct (x )−λ2Id, which must necessarily contain degenerate https://www.dropbox.com/s/s6qr2bkrqtiltkr/SI1.mov?dl=0). pot0ints0ofCt (x )whereitseigenvectorfieldisisotropic. For An advected boundary is depicted red when it is within t0 0 this reason the above procedure is known as geodesic eddy its theoretical Lagrangian coherence horizon and light blue detection. when is beyond it. As expected, no noticeable signs of fila- The specific form of the velocity field considered here is mentation are observed up to that time scale. The filamen- given by tation observed beyond the coherence horizon reveals that v(x,t)= g∇⊥η(x,t), (5) theevolutionoftheringischaracterizedbyadecayprocess f Fig. 1g shows the area enclosed by the largest coherent Lagrangianboundaryasafunctionofthegeographicallon- where g is the acceleration of gravity, f stands for Corio- gitudetakenbytheringasittranslateswestward. Notethe lis parameter, and η(x,t) is the SSH, taken as the sum of a drop,nearlyexponential,beforetheringreachestheWalvis (steady)meandynamictopographyandthe(transient)alti- Ridgeandtheslowdecaythereafter. Indeed,withinthefirst metricSSHanomaly. Themeandynamictopographyiscon- 5monthstheareachangesfromabout4.5×104 to7.5×103 structedfromsatellitealtimetrydata,in-situmeasurements, km2 (or the mean diameter from roughly 240 to 100 km), and a geoid model [Rio and Hernandez, 2004]. The SSH yetoverthefollowing11monthstheareadecaysveryslowly anomalyisprovidedweeklyona0.25◦-resolutionlongitude– atarateofnomorethan15km2d−1untilvanishing. Nearly latitude grid. This is referenced to a 20-year (1993–2012) 90% of the ring interior loses its initial material coherence mean, obtained from the combined processing of data col- prior to crossing the Walvis Ridge. lected by altimeters on the constellation of available satel- Therapiddecayofthering’smaterialcoherenceisnotre- lites [Le Traon et al., 1998]. flectedinthetopologyofthetotalaltimetricSSHfield,but Forthepurposeofthepresentinvestigationwehavecho- isaccompaniedbyasimilarrapiddecayintheSSHanomaly sen to focus on the ring detected and tracked by Froyland amplitude. ThisisillustratedinFig.2,whichdepictsinstan- et al. [2015] over the period 1999–2001. This ring was con- taneous total SSH field streamlines (a) and maximum SSH sideredbyWangetal.[2015]intheircoherenttransportcal- anomaly (b) in the domains occupied by the ring indicated culations. The numerical implementation of geodesic eddy inFigs.1a–f. Firstnotethatthestreamlinesareclosedboth detection is documented at length [Haller and Beron-Vera, beforeandaftertheringcrossestheWalvisRidge,signaling WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING X - 3 Figure 1. (a) Nested family of coherent Lagrangian ring boundaries extracted from altimetry-derived velocity by applying geodesic eddy detection on t = 31 March 1999 inside the region indicated by a 0 rectangle. Each member of the family has a different Lagrangian coherence time scale T ranging from 30 d (outermost) to 480 d (innermost) in steps of 30 d. Selected isobaths (in km) are indicated in gray. Theoutsetisablowupoftheindicatedregion. (b–f)Advectedimagesundertheflow(i.e.,evolution)of thecoherentLagrangianeddyboundariesin(a)onselecteddates. Anadvectedboundaryisdepictedred whenitiswithinitstheoreticalLagrangiancoherencehorizonandinabluetonewhenisbeyondit. The boundary from an additional detection from t with T =65 d is depicted green over the whole tracking 0 process. (g) As a function of longitude, area of the largest domain enclosed by advected boundaries within their theoretical Lagrangian coherence horizon. acoherenteddyfromanEulerianperspective. Furthermore, region filled with streamlines dominates over the transla- the tangential geostrophic velocity at the periphery of the X - 4 WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING Figure 2. (a) Streamlines of the altimetric sea surface height (SSH) field in each rectangular region indicated in (a–f). (b) As a function of longitude, maximum SSH anomaly associated with the ring. tional speed of the region, indicating an eddy capable of stretchesawayfrom,norspiralsinto,theringcore. The65- maintainingacoherentstructure[Flierl,1981]. Second,the dboundaryenclosesabout55%ofthefluidenclosedbythe anomaly falls from about 35 cm in March 1999 to nearly 30-d material boundary on 31 March 1999. Any boundary 20 cm in August 1999, before the ring reaches the Walvis larger than the 65-d boundary is found to develop long fil- Ridge. Similar behavior for other altimetry-tracked rings aments far to the east of the ring as it translates westward within the western Cape Basin was reported by Schouten beyond 2 months or so. Effectively, however, about 70% of et al. [2000]. the fluid enclosed by the 30-d boundary is actually seen to However, a change in SSH anomaly does not necessarily evolve quite coherently for about 2 years. This conclusion implyacorrespondingchangeinmaterialcoherence. Infact, follows from tracking passive tracers lying in between the theamplitudeoftheSSHanomalyrecoverspasttheWalvis 30- and 65-d boundaries. Ridge, reachinginNovember1999almost90%ofitsampli- The enduring Lagrangian coherence of the ring is ex- tudeinMarch1999. BeyondNovember1999,theamplitude plained as a consequence of successive short-term La- of the SSH anomaly falls again, at a rate of about 0.9 cm grangian coherence regain events. To illustrate this, in Fig. month−1. But meanwhile the ring interior loses material 3a we show (in green) selected advected positions of the coherence gradually with no interruption. 65-d boundary. Overlaid on each we depict (in red) a 30- AnincreaseintheSSHamplitudemayneverthelessbein- d boundary identified on the date when the advected 65- dicativeofinteractionwiththebottomtopography. deSteur d boundary is shown. (An animation including monthly and van Leeuwen’s [2009] numerical experiments reveal an snapshots is supplied as supporting information Movie 2 at upward transfer of kinetic energy accompanied by an in- https:/www.dropbox.com/s/tl4f5h8n3upuy9j/SI2.mov?dl=0) creaseoftheSSHamplitudewhenabarocliniceddycrosses For nearly 2 years the advected 65-d boundary is instanta- a meridional ridge. A large vertical extent for the ring can neously closely shadowed by a 30-d boundary, which pro- thusbeexpected, giventhatthecharacteristicdepthofthe vides an effective short-term shield to mixing of the fluid WalvisRidgeisover2km[Byrne et al.,1995]. Suchalarge near and inside the advected 65-d boundary with the am- vertical extent is in line too with in-situ hydrographic ob- bient fluid stirred by turbulence. Furthermore, because a servations [van Aken et al., 2003]. shielding boundary is the outermost member of a nested family of coherent material loops that fill up the ring in- terior, the ring core remains impermeable over such an ex- 4. Enduring Lagrangian coherence tendedperiodaswell. Thisismanifestedbytheincapability ofthe65-dboundarytopenetratetheringcorebyspiralling While filamentation of the ring is observed starting 30 inward. Suchalong-lastingtangentialfilamentationisfound d after detection on 31 March 1999, a large fraction of the toapplyto65-dthrough120-dboundaries. Inotherwords, ring’sfluidpreservesastrikinglycompactentityover2years thematerialbeltdelimitedbythe65-and120-dboundaries of evolution. This is manifested in the evolution of the ma- provides a thick barrier that provides isolation for the fluid terialloopindicatedingreeninFig.1. Thisloopistheout- inside the 120-d boundary. This accounts for 27% of the ermost of a nested family of arclength-reassuming (λ = 1) total fluid trapped inside the ring, which has a diameter of loopsobtainedfromaT =65dcalculation. Beyonditsthe- about 120 km. oretical coherence horizon and for nearly 2 years, this 65- Beyond approximately 2 years filamentation of the ad- d boundary develops only tangential filamentation. More vected65-dboundaryceasestobetangential,signalingmore specifically, even after formal coherence is lost, it neither intense mixing with the ambient fluid. Consistent with this WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING X - 5 Figure 3. (a) In green, advected images on selected dates of the third-to-outermost material loop in Fig. 1a, corresponding to the Lagrangian ring boundary with coherence time scale T = 65 d. In red, shielding boundaries detected from 30- or 15-d integration from the dates shown. (b) Area enclosed by the short-time shielding boundaries as a function of their geographic longitude location. the 30-d boundaries start to shrink, loosing their shielding 480-d boundary on 31 March 1999). By 30 January 1999, power, until no 30-d boundary can be detected (Fig. 3b no boundary with T = −30 d could be extracted, so we shows the area enclosed by the shielding boundaries as a switched to T = −15 d and reduced the detection step to function of longitude position taken). This happens on 19 two weeks. This led to the isolation of 2 boundaries with May 2001. Beyond this date only a 15-d boundary can be T =−30don31and1March1999,and6boundarieswith extracted. Eventuallyby3June2001noshort-termbound- T =−15dfrom30January1999backto16November1998 aryispossibletobeidentified,theringdetectedon31March every 15 d. 1999losesLagrangianentitycompletely,andcanbedeclared Figure4depictsonselecteddatesthesebackwardbound- dead, prior to reaching the South American coast. aries (in red) overlaid on the backward-advected images of Not surprising due to the observer-dependent nature of the forward boundaries extracted on 31 March 1999 (light Euleriananalysis,thedemiseoftheLagrangianringcannot blue). Thebackwardboundaryon31March1999issmaller be inferred from the inspection of the topology of the SSH than the outermost forward boundary on that date, which field. In fact, a compact region of closed SSH streamlines provides only partial shielding for the ring when advected existsevenwhentheringhasvigorouslyfilamented(cf.left- in backward time. Note the filaments stretching away from most SSH contours in Fig. 2a and Fig. 1f). Also, that the the ring into the South Atlantic. areaenclosedbytheshieldingboundarieshasshrunkconsid- A closer look reveals that some filaments spiral inward erablybyFebruary2001explainswhyFroyland et al.[2015] to the center of the ring. This is evident from the inspec- could not extract any coherent sets beyond February 2001. tionofthebackward-advectedimagesof120-dboundaryon ThustheslowdecayreportedbyFroyland et al.[2015]is attributed to the occurrence of successive coherence regain 31 March 1999 (depicted in dark blue in Fig. 4 on selected events. ThisenduringLagrangiancoherenceisnotinferable dates). The inward spiraling of this boundary happens at from a direct application of geodesic eddy detection on a least up to 16 December 1998. fixed date as done in Wang et al. [2015]. Revealing it re- Theshieldingboundariesshrinkconsiderablypast16De- quiresonetoapplyitonsuccessivedates. Theimplications cember1998,andfilamentationofthe120-dboundaryturns of slowly decaying rings for transport are discussed in Sec- both inward and outward spiraling. By 16 November 1998 tion 6 below. the shielding boundary has shrunk considerably and a part ofthe120-dboundaryisseentospiralintoaswirlingstruc- ture from which neither forward- nor backward-time coher- 5. Genesis ent material loops are possible to extract. On 1 November Anattemptwasmadetootoshedlightonthegenesispro- 1998the120-dboundarytakesahighlyconvolutedfilamen- cessoftheringbyapplyingagaingeodesiceddydetectionon tal structure. t =31March1999,butinbackwardtime.1 Thisprocedure The genesis process thus resembles the demise stage but 0 enabledisolatingcoherentLagrangianeddyboundariesonly in reversed time. The ring in question is seen to be the re- with T >−60 d. Because the short-termed forward bound- sult of a ring-merging event rather than a simple occlusion arieswerefoundtoprovideshieldingfortheringoveralong of,andsubsequentpinchofffrom,theAgulhasretroflection time scale, we set T = −30 d and performed the analy- [Dencausseetal.,2010;Pichevinetal.,1999]. Suchamerg- sisaroundthebackward-advectedlocationsoftheringcore ing event occurs right within Cape Cauldron, a highly tur- (taken as the center of mass of the fluid lying inside the bulent region well separated from the Agulhas retroflection X - 6 WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING Figure 4. Backward-advected images on selected dates of the ring boundaries in Fig. 1 corresponding to several Lagrangian coherence time scales (all depicted light blue, except the 120-d boundary, shown indarkblue)withtheshort-termshieldingboundaryobtainedfrombackward-timeintegrationfromthe date indicated overlaid (red). [Boebel et al.,2003]. Thisisconsistentwiththeobservation 6. Implications for transport made by Wang et al. [2015] that material Agulhas rings An important question is how material coherence regain are organized from incoherent fluid away from the Agulhas events affect the conclusions of Wang et al. [2015] if they retroflection. Furthermore, quite a good deal of the fluid were to be verified for all Agulhas rings. A quick compu- tation reveals that rings would carry yearly about 6 Sv (1 (morethan75%asalongbackwardadvectionreveals)that Sv = 106 m3s−1) across the South Atlantic. This rough ends up forming the ring comes from the South Atlantic. estimate follows from assuming that annually about 3 co- WANG,BERON-VERA&OLASCOAGA: THELIFECYCLEOFANAGULHASRING X - 7 herentmaterialringsareformed[Wang et al.,2015],andas [2015]conclusionsaboutthelimitedabilityofAgulhasrings inferred for the ring investigated here, the diameter of the tocarryAgulhasleakageacrosstheSouthAtlanticwouldre- ringsisabout240km,thecoherenceresponseatthesurface mainvalidasthesecorrectedtransportestimateswouldstill extends down to 2 km, and 70% of the ring fluid on the be much smaller than reported leakage estimates. The con- detectiondateiscarriedwellacrossthesubtropicalgyre. If tributionofcoherentLagrangianAgulhasringstothetrans- we further assume that about 25% of the ring contents are portofsaltisalsosmallerthanestimatesbypreviousstudies traceableintotheIndianOcean,asisapplicabletothering [vanBallegooyenetal.,1994;LutjeharmsandCooper,1996] investigatedhere,thentheAgulhasleakagetrappedinrings suggesting that over 95% (more than 70×1012 kg year−1) which is able to traverse the South Atlantic would amount of interbasin salt flux is attributable to rings. Neverthe- to up to 1.5 Sv. less, the excess salt associated with a coherent Lagrangian Overall, the transport results of Wang et al. [2015] may ringmaybetoolargetobeneglected, whichdeservestobe beunderestimatedbyoneorderofmagnitude. Butthemain investigated in more detail. conclusions of Wang et al. [2015] should remain unaltered Acknowledgments. Thealtimeterproductswereproduced because Agulhas leakage estimates are still almost an order by SSALTO/DUCAS and distributed by AVISO with sup- of magnitude bigger [e.g., Richardson, 2007]. On the other port from CNES (http://www.aviso.oceanobs). Our work was hand, there is large uncertainty around the behavior of the supported by NASA through grant NNX14AI85G and NOAA rings below the surface. For instance, according to numer- throughtheClimateObservationsandMonitoringProgram. ical simulations the vertical structure of a ring may decay muchfasterthanitssurfacesignature[deSteuretal.,2004]. Notes Moreover,Wang et al.[2015]showedthatonlyaverysmall fraction of fluid trapped inside rings detected over the last 1. Allofthebackward-timeintegrationresultsreportedaresuch twodecadesiseventuallypickedupbytheNorthBrazilCur- thatatleast90%reversibilityoftheinitialtracerpositionsis rent. ThuswhilecoherentLagrangianAgulhasringsprovide guaranteed. adirectroutefortheAgulhasleakageacrossthesubtropical gyre, most of it may be advected incoherently. The genesis of coherent material rings in the Cape Caul- dronalsoimpliesaverydistinctprocessoftransportofsalt References by these rings. In particular, while previous observations suggestthatAgulhasringsaresheddirectlyfromtheAgul- Beron-Vera, F. J., Y. Wang, M. J. Olascoaga, G. J. Goni, and hasretroflectionandexperienceturbulentmixingthereafter G. Haller (2013), Objective detection of oceanic eddies and [Boebel et al., 2003; Schouten et al., 2000; Schmid et al., theAgulhasleakage,J. Phys. Oceanogr.,43,1426–1438. 2003], mixing of the Agulhas leakage with its surrounding Beron-Vera, F. J., M. J. Olascoaga, G. Haller, M. Farazmand, occurs before a coherent material ring is actually born. As J. Trin˜anes, and Y. Wang (2015), Dissipative inertial trans- aresult,althougharingmaypossesssustainedmaterialco- port patterns near coherent Lagrangian eddies in the ocean, Chaos,25,087,412,doi:10.1063/1.4928693. herence, it will contain a considerable amount of Atlantic Boebel,O.,J.R.E.Lutjeharms,C.Schmid,W.Zenk,T.Rossby, water as well [Wang et al., 2015]. However, the amount of and C. Barron (2003), The Cape Cauldron: a regime of tur- salt eventually trapped in rings should not be considered bulentinter-oceanexchange,Deep-Sea Res. II,50,57–86. to be small. Indeed, hydrographic records show that the Byrne, D. A., A. L. Gordon, and W. F. Haxby (1995), Agulhas salt anomaly associated with a mature coherent Agulhas eddies: A synoptic view using Geosat ERM data, J. Phys. ring (180-km diameter and 1.6-km depth) can be as high Oceanogr.,25,902–917. as 8.4×1012 kg [Schmid et al., 2003]. A quick computa- de Steur, L., and P. J. van Leeuwen (2009), The influence of tion, then, reveals that the ring in the present study may bottom topography on the decay of modeled Agulhas rings, transport approximately 10×1012 kg of excess salt across Deep-Sea Res. I,56,471–494. deSteur,L.,P.J.vanLeeuwen,andS.S.Drijfhout(2004),Tracer theSouthAtlantic,roughly15%ofthetotalannualIndian– leakage from modeled Agulhas rings, J. Phys. Oceanogr., 34, Atlantic Ocean salt flux [Lutjeharms and Cooper, 1996]. 1387–1399. Dencausse,G.,M.Arhan,andS.Speich(2010),Spatio-temporal characteristicsoftheAgulhasCurrentretroflection,Deep Sea 7. Concluding remarks Res. I,57,1392–1405. Flierl,G.(1981),Particlemotionsinlarge-amplitudewavefields, Application of geodesic eddy detection on a recently in- Geophys. Astrophys. Fluid Dyn.,18,39–74. vestigated Agulhas ring has allowed us to explain its en- Froyland,G.,C.Horenkamp,V.Rossi,andE.vanSebille(2015), during Lagrangian coherence when detected from altimetry StudyinganAgulhasring’slong-termpathwayanddecaywith using a probabilistic method [Froyland et al., 2015] as a re- finite-timecoherentsets,Chaos,0,0–0. sultofthesuccessiveoccurrenceofcoherenceregainevents. Haller, G., and F. J. Beron-Vera (2013), Coherent Lagrangian These events are characterized by the formation of coher- vortices: The black holes of turbulence, J. Fluid Mech., 731, R4,doi:10.1017/jfm.2013.391. ent material loops around the ring, preventing the fluid Haller,G.,andF.J.Beron-Vera(2014),Addendumto‘Coherent trapped from mixing with the ambient fluid. These short- Lagrangian vortices: The black holes of turbulence’, J. 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