Year: 2026
Type: article
Abstract: Turbulence is indispensable to redistribute nutrients for all life forms larger than microbial, on land and in the ocean. Yet, the development of deep‐sea turbulence was not studied in three dimensions to date. As a disproportionate laboratory, an array of nearly 3,000 high‐resolution temperature sensors had been installed for three years on the flat 2,500‐m deep bottom of the Mediterranean Sea. The time series from the half‐cubic hectometer mooring‐array allows for the creation of unique movies of deep‐sea water motions. Although temperature differences are typically 0.001°C, variable convection‐turbulence is observed as expected from geothermal heating through the flat seafloor. During about 40% of the time, an additional turbulence, 3 times stronger in magnitude, is observed from slantwise advected warmer waters to pass in turbulent clouds. Besides turbulent clouds and seafloor heating, movies also reveal weakly turbulent interfacial‐wave breakdown that commonly occurs in the open ocean far away from boundaries.
Source: Geophysical Research Letters
DOI: 10.1029/2025gl119998
Authors: Hans van Haren, KM3NeT collaboration
Institution: Royal Netherlands Institute for Sea Research
Language: English
Subfield: Oceanography
Field: Earth and Planetary Sciences
Domain: Physical Sciences
SDG: Life below water
Open Access status: gold
Estimated APC paid: $3,190
Funders: Arab Fund for Economic and Social Development, European Commission, Fundacja na rzecz Nauki Polskiej, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Generalitat Valenciana, Khalifa University of Science, Technology and Research, Agentúra na Podporu Výskumu a Vývoja, ESI Group, European Regional Development Fund, Agencia Estatal de Investigación
Awards: G120905174, G1422035950, G2262748287, G2489860800, G338497233, G3480869486, Skúmanie vlastností a interakcií neutrín pomocou reaktorových, atmosférických, astrofyzikálnych neutrín a atómového jadra, G3590787598, G3681454997, G4016415828, G4042783231, G425668148, G434337789, G4414191887, G451917667, G5967599077, G6948331134, Chemical Elements as Tracers of the Evolution of the Cosmos - Infrastructures for Nuclear Astrophysics, G7084143925, G7830810647, G8114839858, G8219391473
OpenAlex ID: W7125109906
