2012
DOI: 10.1038/ncomms1836
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Abyssal undular vortices in the Eastern Mediterranean basin

Abstract: Abyssal temperature and velocity observations performed within the framework of the neutrino mediterranean observatory, a project devoted to constructing a km 3 -scale underwater telescope for the detection of high-energy cosmic neutrinos, demonstrate cross-fertilization between subnuclear physics and experimental oceanography. Here we use data collected south of sicily in the Ionian abyssal plain of the Eastern mediterranean (Em) basin to show for the first time that abyssal vortices exist in the Em, at depth… Show more

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Cited by 27 publications
(39 citation statements)
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“…Expressed another way, rotation is more likely where vent orifices are larger and flow velocity smaller. A plume similar to that observed by Rubino et al (2012) with an average velocity value U ~10 cm/s, diameter of emissions L ~1.5 km, and f ~2π/24/hr. has an R o value of ~0.9.…”
Section: Vortex Tube Propellantsupporting
confidence: 73%
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“…Expressed another way, rotation is more likely where vent orifices are larger and flow velocity smaller. A plume similar to that observed by Rubino et al (2012) with an average velocity value U ~10 cm/s, diameter of emissions L ~1.5 km, and f ~2π/24/hr. has an R o value of ~0.9.…”
Section: Vortex Tube Propellantsupporting
confidence: 73%
“…During the LGM, the GHSZ was over ~500 m thick in the vicinity of the vortices reported by Rubino et al (2012) whereas the present GHSZ is only ~200 to 300 m thick (Praeg et al, 2011). As it can be expected that most of the NGH will be in the lower third of the GHSZ, large volumes of NGH have been, and probably continue to be, converted to constituent gas and water.…”
Section: Discussion and Conceptual Modelmentioning
confidence: 69%
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