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 metres 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 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, 2021) addresses the observed bubble size distributions and the processes responsible for them.

Highlights

  • 35 The bubbles generated by breaking waves are an important feature of the ocean surface

  • Extrapolating the observed bubble size distribution to 1 μm in radius suggests that the maximum possible contribution to the total volume from bubbles below 20 μm is extremely small, while the small number of bubbles larger than ~100 μm reaching the depth of 320 the resonator make a negligible contribution to the total void fraction; a direct comparison between the two instruments is appropriate

  • The results are consistent with a two-stage formation 640 mechanism for deep bubble plumes

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Summary

Introduction

35 The bubbles generated by breaking waves are an important feature of the ocean surface. It has been suggested that the deeper plumes are formed by advection of smaller bubbles downwards rather than being the direct consequence of a breaking waves (Zedel and Farmer, 1991; Thorpe et al, 2003), but there has been little in situ data available to explore those processes. This question is very relevant to the uptake of less soluble gases like oxygen, as well as for acoustical and optical studies. Studies either focus on processes very close to the surface (usually laboratory studies), or the deeper plumes observed at sea using upward-looking sonar, but rarely both at the same time

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