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significant (>0.01 g m −3 ) LWCs reached right up to cloud top at ~4 km. It may be significant that close to the region where the highest concentration of columns were observed, larger supercooled drops (greater than 80- μ m diameter) were present in concentrations of up to ~150 L −1 , the concentrations of drizzle fell to ~1–30 L −1 in regions where columnar crystals were in concentrations of ~80 L −1 ( Fig. 9a ). Crawford et al. (2011) showed the importance of warm rain processes leading to the
significant (>0.01 g m −3 ) LWCs reached right up to cloud top at ~4 km. It may be significant that close to the region where the highest concentration of columns were observed, larger supercooled drops (greater than 80- μ m diameter) were present in concentrations of up to ~150 L −1 , the concentrations of drizzle fell to ~1–30 L −1 in regions where columnar crystals were in concentrations of ~80 L −1 ( Fig. 9a ). Crawford et al. (2011) showed the importance of warm rain processes leading to the
. For further details of these instruments and the processing of the data, the reader is referred to Lloyd et al. (2014) and Crosier et al. (2014) . By merging data from the CIP-15 and CIP-100 probes we were able to construct ice PSDs from 45 μ m up to 6.2 mm. We did notice an occasional problem with phase misclassification during the processing of the in situ data; this occurred only in the presence of drizzle drops (i.e., a few hundred micrometers in diameter) which sometimes appear slightly
. For further details of these instruments and the processing of the data, the reader is referred to Lloyd et al. (2014) and Crosier et al. (2014) . By merging data from the CIP-15 and CIP-100 probes we were able to construct ice PSDs from 45 μ m up to 6.2 mm. We did notice an occasional problem with phase misclassification during the processing of the in situ data; this occurred only in the presence of drizzle drops (i.e., a few hundred micrometers in diameter) which sometimes appear slightly