Understanding cirrus ice crystal number variability for different heterogeneous ice nucleation spectra
S. C. Sullivan, R. Morales Betancourt, D. Barahona and 4 more
Atmospheric Chemistry and Physics · 2016
doi:10.5194/acp-16-2611-2016 (opens in a new tab)
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Abstract
Along with minimizing parameter uncertainty, understanding the cause of temporal and spatial variability of the nucleated ice crystal number, <i>N</i><sub>i</sub>, is key to improving the representation of cirrus clouds in climate models. To this end, sensitivities of <i>N</i><sub>i</sub> to input variables like aerosol number and diameter provide valuable information about nucleation regime and efficiency for a given model formulation. Here we use the adjoint model of the adjoint of a cirrus formation parameterization (Barahona and Nenes, 2009b) to understand <i>N</i><sub>i</sub> variability for various ice-nucleating particle (INP) spectra. Inputs are generated with the Community Atmosphere Model version 5, and simulations are done with a theoretically derived spectrum, an empirical lab-based spectrum and two field-based empirical spectra that differ in the nucleation threshold for black carbon particles and in the active site density for dust. The magnitude and sign of <i>N</i><sub>i</sub> sensitivity to insoluble aerosol number can be directly linked to nucleation regime and efficiency of various INP. The lab-based spectrum calculates much higher INP efficiencies than field-based ones, which reveals a disparity in aerosol surface properties. <i>N</i><sub>i</sub> sensitivity to temperature tends to be low, due to the compensating effects of temperature on INP spectrum parameters; this low temperature sensitivity regime has been experimentally reported before but never deconstructed as done here.
Abstract licence: CC BY
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