Published in

Wiley, Journal of Geophysical Research. Oceans, 3(119), p. 2066-2080, 2014

DOI: 10.1002/2013jc009459

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Autonomous observations of solar energy partitioning in first-year sea ice in the Arctic Basin

This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

A Spectral Radiation Buoy (SRB) was developed to autonomously measure the spectral incident, reflected, and transmitted spectral solar radiation (350 to 800 nm) above and below sea ice. The SRB was deployed on drifting first-year sea ice near the North Pole in mid-April 2012, together with velocity and ice mass balance buoys. The buoys drifted southward and reached Fram Strait after approximately seven months, covering a complete melt season. At the SRB site, snow melt started on 10 June, and had completely disappeared by 14 July. Surface albedo was above 0.85 until snow melt onset and decreased rapidly with the progression of snow melt. Albedo was lowest on 14 July, when the observed surface was likely a mixture of bare ice and melt pond(s). The transmitted irradiance measured under the ice was largest in July, with a monthly average of 20 W m-2, compared to less than 0.3 W m-2 pre-melt. Under-ice irradiance peaked on 19–20 July, with a daily average around 35 W m-2. From mid-April to mid-September, the solar energy transmitted through the ice into the ocean contributed about two thirds of the energy required for the observed bottom melt (0.49 m). The energy absorbed by the ice after snow melt was enough to melt an additional 0.1 m of ice. Solar energy incident on open water and melt ponds provided significant additional heating, indicating solar heating could explain all of the observed bottom melt in this region in summer 2012.