Abstract
Abstract. Simulations of cirrus are subject to uncertainties in model physics and meteorological input data. Here we model cirrus clouds along air mass trajectories, whose extinction has been measured with an elastic backscatter lidar at Jungfraujoch research station in the Swiss Alps, with a microphysical stacked box model. The sensitivities of these simulations to input data uncertainties (trajectory resolution, unresolved vertical velocities, ice nuclei number density and upstream specific humidity) are investigated. Variations in the temporal resolution of the wind field data (COSMO-Model at 2.2 km resolution) between 20 s and 1 h have only a marginal impact on the trajectory path, while the representation of the vertical velocity variability and therefore the cooling rate distribution are significantly affected. A temporal resolution better than 5 min must be chosen in order to resolve cooling rates required to explain the measured extinction. A further increase in the temporal resolution improves the simulation results slightly. The close match between the modelled and observed extinction profile for high-resolution trajectories suggests that the cooling rate spectra calculated by the COSMO-2 model suffice on the selected day. The modelled cooling rate spectra are, however, characterized by significantly lower vertical velocity amplitudes than those found previously in some aircraft campaigns (SUCCESS, MACPEX). A climatological analysis of the vertical velocity amplitude in the Alpine region based on COSMO-2 analyses and balloon sounding data suggests large day-to-day variability in small-scale temperature fluctuations. This demonstrates the necessity to apply numerical weather prediction models with high spatial and temporal resolutions in cirrus modelling, whereas using climatological means for the amplitude of the unresolved air motions does generally not suffice. The box model simulations further suggest that uncertainties in the upstream specific humidity (± 10 % of the model prediction) and in the ice nuclei number density (0–100 L−1) are more important for the modelled cirrus cloud than the unresolved temperature fluctuations if temporally highly resolved trajectories are used. For the presented case the simulations are incompatible with ice nuclei number densities larger than 20 L−1 and insensitive to variations below this value.
Highlights
Cirrus clouds are an important component of the climate system because they influence the radiative budget by scattering solar radiation back to space and by trapping longwave radiation in the troposphere
To capture most of the variability that is represented in numerical weather prediction (NWP) models with a horizontal grid spacing of 2.2 km, trajectory data should be used at least at a 5 min temporal resolution
For the cirrus cloud investigated in this study, the modelled extinction profile matches very well with the observations if trajectory data are used at a temporal resolution of 1 min or higher and wind field data at a resolution of 5 min or higher
Summary
Cirrus clouds are an important component of the climate system because they influence the radiative budget by scattering solar radiation back to space and by trapping longwave radiation in the troposphere. The balance between these two mechanisms determines the overall radiative effect of cirrus clouds on the climate. We note here that the overall radiative forcing effect by cirrus clouds is smaller than the effect of liquid and mixed-phase clouds situated further down in the troposphere (Chen et al, 2000; Sherwood et al, 2014; Kienast-Sjögren et al, 2015). The uncertainties in the radiative forcing of clouds in climate models can to a large part be attributed to uncertainties considering low clouds and convective mixing (Sherwood et al, 2014)
Published Version (Free)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have