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Spirals on the sea
Munk, W. (2001). Spirals on the sea. Sci. Mar. (Barc.) 65(S2): 193-198. https://dx.doi.org/10.3989/scimar.2001.65s2193
In: Scientia Marina (Barcelona). Consejo Superior de Investigaciones Científicas. Institut de Ciènces del Mar: Barcelona. ISSN 0214-8358; e-ISSN 1886-8134, meer
Ook verschenen in:
Gili, J.-M.; Pretus, J.L.; Packard, T.T. (Ed.) (2001). A Marine Science Odyssey into the 21st Century: 36th European Marine Biology Symposium, Maó (Menorca), 17-22 September 2001. European Marine Biology Symposia, 36. Scientia Marina (Barcelona), 65(Suppl. 2). 326 pp. https://dx.doi.org/10.3989/scimar.2001.65s2, meer
Peer reviewed article  

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Trefwoord
    Marien/Kust
Author keywords
    Remote sensing, air-sea boundary, frontal formation, mixing

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  • Munk, W.

Abstract
    Spiral eddies were first seen in the sun glitter on the Apollo Mission 30 years ago; they have since been recorded on SAR missions and in the infrared. The spirals are globally distributed, 10-25 km in size and overwhelmingly cyclonic. They have not been explained. Under light winds favorable to visualization, linear surface features with high surfactant density and low surface roughness are of common occurrence. We have proposed that frontal formations concentrate the ambient shear and prevailing surfactants. Horizontal shear instabilities ensue when the shear becomes comparable to the coriolis frequency. The resulting vortices wind the liner features into spirals. The hypothesis needs to be tested by prolonged measurements and surface truth. Spiral eddies are a manifestation of a sub-mesoscale oceanography associated with upper ocean stirring; dimensional considerations suggest a horizontal diffusivity of order 103 m2 s-1.

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