“…An interesting question is to explain why the CDSD is wider than predicted and the presence of the large droplet sizes in the tail of the distribution (e.g., Siebert and Shaw, 2017), which might be related to the fast-rain process in the atmosphere (e.g., Göke et al, 2007). Several pos- 15 sible mechanisms have been proposed, including the existence of giant cloud condensational nuclei (GCCN, usually defined as aerosols with dry diameter larger than few µm) (e.g., Feingold et al, 1999;Yin et al, 2000;Jensen and Lee, 2008;Cheng et al, 2009;Jensen and Nugent, 2017), lucky cloud droplets (e.g., Kostinski and Shaw, 2005;Naumann and Seifert, 2015;Lozar and Muessle, 2016), mixing with environmental air (e.g., Lasher-Trapp et al, 2005;Cooper et al, 2013;Korolev et al, 2013;Yang et al, 2016), supersaturation fluctuations (e.g., Chandrakar et al, 2016;Siebert and Shaw, 2017), and enhancement of collision 20 efficiency due to turbulence or charge (e.g., Paluch, 1970;Grabowski and Wang, 2013;Falkovich and Pumir, 2015;Lu and Shaw, 2015). Recently, Jensen and Nugent (2017) investigated the effect of GCCN on droplet growth and rain formation using a cloud parcel model.…”