Atmos. Chem. Phys., 17, 5221–5237, 2017 www.atmos-chem-phys.net/17/5221/2017/ doi:10.5194/acp-17-5221-2017 © Author(s) 2017. CC Attribution 3.0 License. Genesis of diamond dust, ice fog and thick cloud episodes observed and modelled above Dome C, Antarctica Philippe Ricaud1, Eric Bazile1, Massimo del Guasta2, Christian Lanconelli3,a, Paolo Grigioni4, and Achraf Mahjoub1 1Météo-France/CNRM, CNRS UMR 3589, 42 avenue Gaspard Coriolis, 31057 Toulouse, France 2INO-CNR, Via Madonna del Piano 10, 50019, Sesto Fiorentino, Italy 3Institute of Atmospheric Sciences and Climate (ISAC), Consiglio Nazionale delle Ricerche, via Gobetti 101, 40129 Bologna, Italy 4ENEA, Lungotevere Thaon di Revel, 76-00196 Roma, Italy anow at: Joint Research Center, Institute for Environment and Sustainability (IES), Land Resource Management Unit (H05), via Fermi, 21027 Ispra (VA), Italy Correspondence to: Philippe Ricaud (
[email protected]) Received: 12 September 2016 – Discussion started: 15 September 2016 Revised: 31 March 2017 – Accepted: 31 March 2017 – Published: 21 April 2017 Abstract. Episodes of thick cloud and diamond dust/ice fog are detected during the warm and wet periods (24–26 March were observed during 15 March to 8 April 2011 and 4 to 2011 and 4 March 2013) with high depolarization ratios 5 March 2013 in the atmosphere above Dome C (Concor- (greater than 30 %) from the surface to 5–7 km above the dia station, Antarctica; 75◦060 S, 123◦210 E; 3233 m a.m.s.l.). ground associated with precipitation of ice particles and the The objectives of the paper are mainly to investigate the presence of a supercooled liquid water (depolarization less processes that cause these episodes based on observations than 10 %) clouds.