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Ring shedding

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This is an old revision of this page, as edited by WikiDan61 (talk | contribs) at 19:58, 19 May 2021 (Cleaned up per comment given earlier. Prep for publication.). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

  • Comment: This draft is good, and just about ready for publication, but it needs some minor tweaks:
  • Comment: I have removed the image after trying a few searches (google, bing, yandex) and was not able to source it.  A S U K I T E  18:26, 19 May 2021 (UTC)
  • Comment: CommanderWaterford I would argue that the unsourced image is a reason not to approve. I wouldn't suggest deleting the article for the missing source, but I would remove the image if it cannot be properly sourced. WikiDan61ChatMe!ReadMe!! 15:56, 19 May 2021 (UTC)

Ring shedding is a phenomenon in ocean currents where circle or ring-shaped eddies separate from the current. The rings are independent water current systems and can persist for several months and occur in most ocean basins[1]. The separated rings can have both warm or cold cores and play a role in the thermohaline circulation, interocean mixing, and nutrient supply for algae and bacteria.

Process of ring shedding

Ring shedding often takes place in the retroflection region, where the current loops back. The turbulent and dynamic nature of the ocean causes the current loop to sometimes close onto itself and separate ("shed") from the current.[2][3][4] This results in an independent ring current that drifts away from the main current. The exact timing of ring shedding is often unclear and the process behind it is still an active topic of research. The topography of the ocean floor and incoming eddies from upstream regions could play a role in ring shedding.[4][5] Other research indicates that ring shedding is driven by barotropic instabilities.[4][6][7] When the retroflection region destabilizes, the loop can separate from the current, forming a ring.[7]

Characteristics and observation

The process of ring shedding was first described by Fuglisteri in 1972, who observed rings in the Gulf Stream.[2] Since then, ring shedding has been observed in most ocean basins. Typically, the rings have a diameter of 100 to 400 kilometres (62 to 249 miles), a depth of up to 1,500 metres (4,900 feet), and a temperature anomaly of a few degrees Celsius.[1] The rings drift slowly (0 to 5 kilometres (0.0 to 3.1 miles) per day) until they either decay or are reabsorbed by their parent current.[8]

There are two main types of rings: cold core rings and warm core rings. The warm cores rings are easy to observe; due to their temperature anomaly satellites can detect them with infrared images.[1] Since warm water expands, these warm core rings also have elevated local sea levels and can hence also be observed by buoys or satellites using radar altimeters to map the topography of the ocean.[1][4][9]

Cold core rings are more difficult to observe as their initial colder surface is warmed by solar radiation. However, under the surface the colder water temperatures persist longer and deeper, allowing measurement and observation using vertical ocean profiles of temperature and salinity.[1]

Occurrence

Kuroshio

The Kuroshio current is a western boundary current in the Northeast Pacific Ocean. In 1994, ring shedding was first observed where the Kuroshio current loops into the South China Sea.[10][11] The observed current ring was a warm core, anticyclonic ring with a diameter of about 150 kilometres (93 mi) and detached from the Kuroshio in the Luzon Strait. The ring had a current speed of about 1 metre per second (3.3 ft/s) near the surface. The ring had positive temperature anomalies up until a depth of 1 kilometre (0.62 mi).

Gulf Stream

In the Gulf Stream ring shedding takes place at two locations: in the Gulf of Mexico and along the eastern coast of the United States.[1] The Loop current, as its name suggests, loops into the Gulf of Mexico. At the point of retroflection, ring shedding results in both warm core anticyclonic and cold core cyclonic rings.[1][4] These rings can have diameters up to 400 kilometres (250 mi) and reach depths of 1,500 metres (4,900 ft).[1] The frequency of the ring shedding in the Loop current has a high interannual variability.[12][13] However, a shift in the regime of ring shedding has been observed. During the period 1980–1999, there were on average 18 rings shed in the Gulf of Mexico per year, whereas the average between 2000 and 2017 was 33 rings per year.[6] The underlying geophysical reason for this shift in regime around 2000 is still a topic of debate.

Further down the Gulf Stream, along the eastern coast of the United States, ring shedding also takes place, albeit much less frequently. Here only warm core, anticyclonic rings with a diameter of typically 100 to 200 kilometres (62 to 124 mi) are formed.[1] These rings only occur once or twice a year and most of them drift slowly westwards until they are reabsorbed by the Gulf Stream after several months.

Agulhas current

The Agulhas current flows alongside the coast of southeast Africa until it retroflects at the tip of South Africa. Ring shedding occurs in this retroflection region.[1][3][7][9] The rings are warm core and anticyclonic, with a frequency of 4-6 rings per year.[1][9][5] However, the shedding of rings happens very irregularly and long periods of almost half a year without any rings occur.[5] The Agulhas rings transport warm and salty water to the Southern Atlantic Ocean. The water from the Agulhas rings can be up to 5 °C (41 °F) warmer than the water in the Southern Atlantic.[1] The rings from the Agulhas current transport about 5 Sverdrup to the Atlantic Ocean, thereby playing an important role in thermohaline circulation.[3] The exact cause of ring shedding in the Agulhas retroflection region is still unclear. One possible cause is incoming eddies from upstream regions.[5] A second proposed explanation is that the ring shedding is caused by barotropic instabilities in the Agulhas retroflection region.[7]

Effects

Thermohaline circulation

Ring shedding might play an important role in thermohaline circulation, depending on the location. The movement of the Agulhas rings are paired with leakage of warm and saline Indian Ocean water in the Southern Atlantic Ocean.[7] These rings move in the northwest direction in the Atlantic Ocean and are important for the renewal of North Atlantic Deep Water.[3]

Iron supply

Cold core rings in the Gulf Stream have higher iron concentrations than the other subtropical water in the Northern Atlantic. The rings transport iron-rich water from the continental slope to other parts of the Northern Atlantic.[14] For cyanobacteria, this incoming flux of iron is very important, as they require high iron concentrations to live in these parts of the Atlantic Ocean.

References

  1. ^ a b c d e f g h i j k l "Wind Driven Surface Currents: Rings". NASA. Retrieved 18 May 2021.{{cite web}}: CS1 maint: url-status (link)
  2. ^ a b Fuglister, F (1972). "Cyclonic rings formed by the Gulf Stream 1965-66". Studies in Physical Oceanography. New York: Gordon and Breach: 137–168.
  3. ^ a b c d Lutjeharms, J; Gordon, A (1987). "Shedding of an Agulhas ring observed at sea". Nature. 325: 138–140. doi:10.1038/325138a0.
  4. ^ a b c d e Chérubin, L; Morel, Y; Chassignet, E (2006). "Loop Current Ring Shedding: The Formation of Cyclones and the Effect of Topography". Journal of Physical Oceanography. 36(4): 569–591. doi:10.1175/JPO2871.1.
  5. ^ a b c d Schouten, M; de Ruijter, W; Van Leeuwen, P (2002). "Upstream control of Agulhas Ring shedding". Journal of Geophysical Research Atmospheres. 107(8). doi:10.1029/2001JC000804.
  6. ^ a b Gangopadhyay, A; Gawarkiewicz, G (2019). "An Observed Regime Shift in the Formation of Warm Core Rings from the Gulf Stream". Scientific Reports. 9. doi:10.1038/s41598-019-48661-9.
  7. ^ a b c d e Weijer, W; Zharkov, V; et al. (2013). "Agulhas ring formation as a barotropic instability of the retroflection". Geophysical research letters.
  8. ^ Richardson, P (1980). "Gulf Stream Ring Trajectories". Journal of Physical Oceanography. 10(1): 90–104. doi:10.1175/1520-0485(1980)010<0090:GSRT>2.0.CO;2.
  9. ^ a b c Feron, R; De Ruijter, W; Oskam, D (1992). "Ring shedding in the Agulhas Current System". Journal of Geophysical Research Oceans. 97: 9467–9477. doi:10.1029/92JC00736.
  10. ^ Li, L; Dowlin, W; Su, J (September 1998). "Anticyclonic rings from the Kuroshio in the South China Sea". Deep Sea Research Part I Oceanographic Research Papers. 45(9): 1469–1482. doi:10.1016/S0967-0637(98)00026-0.
  11. ^ Hu, J; Kawamura, H; Hong, H; et al. (2000). "A Review on the Currents in the South China Sea: Seasonal Circulation, South China Sea Warm Current and Kuroshio Intrusion". Journal of Oceanography. 56(6): 607–624. doi:10.1023/A:1011117531252 – via ResearchGate.
  12. ^ Silver, A; Gangopadhyay, A; et al. (2021). "Interannual and seasonal asymmetries in Gulf Stream Ring Formations from 1980 to 2019". Scientific Reports. 11. doi:10.1038/s41598-021-81827-y.
  13. ^ Sasaki, Y (2016). "Interannual variability of ring formations in the Gulf Stream region". American Geophysical Union. OCean Science Meeting 2016. Bibcode:2016AGUOSPO11C..05S.
  14. ^ Conway, T; Palter, J; de Souza, G (2018). "Gulf Stream rings as a source of iron to the North Atlantic subtropical gyre". Nature Geoscience. 11(8). doi:10.1038/s41561-018-0162-0.
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