[1] Measurements of NO Y condensation on cirrus particles found in stratospherically influenced air sampled during the SOLVE-I mission are analyzed and compared with data from other field studies of HNO 3 or NO Y condensation on ice. Each field study exhibits an order of magnitude data spread for constant HNO 3 pressures and temperatures. While others assumed this distribution is due to random error, the data spread exceeds instrument precision errors and instead suggests HNO 3 removal had not attained equilibrium at the time of sampling. During the SOLVE-I mission, condensation on ice was a significant sink for HNO 3 despite submonolayer surface coverages; we therefore propose condensation of HNO 3 on lower-stratospheric cirrus particles is controlled by kinetics and will occur at a kinetically limited rate. Furthermore, we suggest the low accommodation coefficient for HNO 3 on ice combined with relatively short-lived clouds causes highly scattered, limited HNO 3 uptake on cirrus particles. We couple laboratory data on the accommodation coefficient of HNO 3 on ice with field surface coverage data in order to generate a ''cloud clock'': a calculation to determine the age of a cloud parcel. Data from the aforementioned field studies are compared to theoretical models for equilibrium surface coverage on the basis of laboratory data extrapolated to atmospheric temperatures and HNO 3 pressures. This comparison is difficult because most of the atmospheric data are probably not at equilibrium and follow a condensation time curve rather than an equilibrium surface coverage curve. Finally, we develop a simple mathematical solution for the time required for HNO 3 condensation on ice.