Ocean bubbles under high wind conditions – Part 1: Bubble distribution and development
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Published:2022-05-03
Issue:3
Volume:18
Page:565-586
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ISSN:1812-0792
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Container-title:Ocean Science
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language:en
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Short-container-title:Ocean Sci.
Author:
Czerski HelenORCID, Brooks Ian M.ORCID, Gunn Steve, Pascal Robin, Matei Adrian, Blomquist ByronORCID
Abstract
Abstract. The bubbles generated by breaking waves are of considerable
scientific interest due to their influence on air–sea gas transfer, aerosol
production, and upper ocean optics and acoustics. However, a detailed
understanding of the processes creating deeper bubble plumes (extending 2–10 m below the ocean surface) and their significance for air–sea gas
exchange is still lacking. Here, we present bubble measurements from the
HiWinGS expedition in the North Atlantic in 2013, collected during several
storms with wind speeds of 10–27 m s−1. A suite of instruments was used
to measure bubbles from a self-orienting free-floating spar buoy: a
specialised bubble camera, acoustical resonators, and an upward-pointing
sonar. The focus in this paper is on bubble void fractions and plume
structure. The results are consistent with the presence of a heterogeneous
shallow bubble layer occupying the top 1–2 m of the ocean, which is regularly
replenished by breaking waves, and deeper plumes which are only formed from
the shallow layer at the convergence zones of Langmuir circulation. These
advection events are not directly connected to surface breaking. The void
fraction distributions at 2 m depth show a sharp cut-off at a void fraction
of 10−4.5 even in the highest winds, implying the existence of
mechanisms limiting the void fractions close to the surface. Below wind
speeds of 16 m s−1 or a wind-wave Reynolds number of RHw=2×106, the probability distribution of void fraction at 2 m
depth is very similar in all conditions but increases significantly above
either threshold. Void fractions are significantly different during periods
of rising and falling winds, but there is no distinction with wave age.
There is a complex near-surface flow structure due to Langmuir circulation,
Stokes drift, and wind-induced current shear which influences the spatial
distribution of bubbles within the top few metres. We do not see evidence
for slow bubble dissolution as bubbles are carried downwards, implying that
collapse is the more likely termination process. We conclude that the
shallow and deeper bubble layers need to be studied simultaneously to link
them to the 3D flow patterns in the top few metres of the ocean. Many open
questions remain about the extent to which deep bubble plumes contribute to
air–sea gas transfer. A companion paper (Czerski et al.,
2022) addresses the observed bubble size distributions and the processes
responsible for them.
Funder
Natural Environment Research Council National Science Foundation
Publisher
Copernicus GmbH
Subject
Cell Biology,Developmental Biology,Embryology,Anatomy
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