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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Thin (~ 100 m) supercooled liquid water (SLW, water staying in liquid phase below 0 °C) clouds have been detected, analysed, and modelled over the Dome C (Concordia, Antarctica) station during the austral summer 2018–2019 using observations and meteorological analyses. The SLW clouds were observed at the top of the planetary boundary layer and the SLW content was always strongly underestimated by the model indicating an incorrect simulation of the surface energy budget of the Antarctic Plateau.
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ACP | Articles | Volume 20, issue 7
ACP | Articles | Volume 20, issue 7
Atmos. Chem. Phys., 20, 4167–4191, 2020
https://doi.org/10.5194/acp-20-4167-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Chem. Phys., 20, 4167–4191, 2020
https://doi.org/10.5194/acp-20-4167-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
ACP | Articles | Volume 20, issue 7

Research article 07 Apr 2020

Research article | 07 Apr 2020

Supercooled liquid water cloud observed, analysed, and modelled at the top of the planetary boundary layer above Dome C, Antarctica

Philippe Ricaud et al.

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Short summary
Thin (~ 100 m) supercooled liquid water (SLW, water staying in liquid phase below 0 °C) clouds have been detected, analysed, and modelled over the Dome C (Concordia, Antarctica) station during the austral summer 2018–2019 using observations and meteorological analyses. The SLW clouds were observed at the top of the planetary boundary layer and the SLW content was always strongly underestimated by the model indicating an incorrect simulation of the surface energy budget of the Antarctic Plateau.
Read more
Citation
Altmetrics
Final-revised paper
Preprint
Atmospheric Chemistry and Physics

An interactive open-access journal of the European Geosciences Union

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